text:
Q: Updating IP addresses in Apache Ambari I am running an Ambari installation (1.7.0) on HDP (2.2.0.0-2041).  After rebooting one of the machines, the internal IP address changed.  This means that Ambari can't find it.  (We're running on AWS EC2, so the hostnames have the form ip-x-x-x-x.)
How do I inform Ambari of the new ip address?  The only option I've found so far is to add a new host, but as I understand this will wipe the machine clean.

A: This great blog post helped us:
http://www.swiss-scalability.com/2015/01/rename-host-in-ambari-170.html
Basically you will need to log into Ambari's database.  (Not the GUI, the actual backend database).  It's best to read the blog post in its entirety, but I am appending the important secret sauce that actually makes things happen.
If you're on mysql:
SET FOREIGN_KEY_CHECKS=0;
BEGIN;
UPDATE ambari.clusterhostmapping set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.configgrouphostmapping set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.host_role_command set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hostcomponentdesiredstate set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hostcomponentstate set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hostconfigmapping set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hoststate set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hosts set host_name = '${new-name}' WHERE host_name = '${old-name}';
COMMIT;
SET FOREIGN_KEY_CHECKS=1;

If you're on postgresql:
ALTER TABLE ambari.clusterhostmapping DROP CONSTRAINT clusterhostmapping_cluster_id;
ALTER TABLE ambari.configgrouphostmapping DROP CONSTRAINT fk_cghm_hname;
ALTER TABLE ambari.host_role_command DROP CONSTRAINT fk_host_role_command_host_name;
ALTER TABLE ambari.hostcomponentdesiredstate DROP CONSTRAINT hstcmponentdesiredstatehstname;
ALTER TABLE ambari.hostcomponentstate DROP CONSTRAINT hostcomponentstate_host_name;
ALTER TABLE ambari.hostconfigmapping DROP CONSTRAINT fk_hostconfmapping_host_name;
ALTER TABLE ambari.hoststate DROP CONSTRAINT fk_hoststate_host_name;

BEGIN;
UPDATE ambari.clusterhostmapping set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.configgrouphostmapping set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.host_role_command set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hostcomponentdesiredstate set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hostcomponentstate set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hostconfigmapping set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hoststate set host_name = '${new-name}' WHERE host_name = '${old-name}';
UPDATE ambari.hosts set host_name = '${new-name}' WHERE host_name = '${old-name}';
COMMIT;

ALTER TABLE ambari.hoststate ADD CONSTRAINT fk_hoststate_host_name FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);
ALTER TABLE ambari.hostconfigmapping ADD CONSTRAINT fk_hostconfmapping_host_name FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);
ALTER TABLE ambari.hostcomponentstate ADD CONSTRAINT hostcomponentstate_host_name FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);
ALTER TABLE ambari.hostcomponentdesiredstate ADD CONSTRAINT hstcmponentdesiredstatehstname FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);
ALTER TABLE ambari.host_role_command ADD CONSTRAINT fk_host_role_command_host_name FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);
ALTER TABLE ambari.configgrouphostmapping ADD CONSTRAINT fk_cghm_hname FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);
ALTER TABLE ambari.clusterhostmapping ADD CONSTRAINT clusterhostmapping_cluster_id FOREIGN KEY (host_name) REFERENCES ambari.hosts(host_name);


text:
Australia Is About to Make It Easier to Visit — Here's What's Changing
Although travelers to Australia are still required to be vaccinated, the country is lifting its requirement of a pre-departure COVID-19 test.
Alison Fox
Alison Fox is a Travel + Leisure contributor. She has also written for Parents.com, The Wall Street Journal, and amNewYork. When she's not in New York City, she can be found at the beach or on the slopes.
Photo: Saeed Khan/Getty Images
Australia will eliminate its pre-arrival test requirements for international travelers next month, just weeks after reopening its borders to the world.
The requirement will be lifted on April 17, Greg Hunt, the minister for health and aged care, said in a statement.
"The emergency period was a crucial early decision in Australia's pandemic response," Hunt said, adding, "Shutting the international borders early was a tough but decisive action, which enabled Australia to manage the pandemic and minimize the loss of life."
Australia fully reopened to international visitors on Feb. 21 and currently requires travelers be fully vaccinated and show proof of a negative COVID-19 PCR test taken within three days of their flight or show proof of a negative rapid antigen test taken under medical supervision within 24 hours of their flight.
Going forward, international travelers will still have to be vaccinated and must wear a mask while on international flights, according to Hunt.
Additionally, on April 17, Australia will also drop restrictions on cruise ships into and within Australian territory. Following that announcement, Royal Caribbean announced several Australian cruises for 2023 and 2024 sailing out of Brisbane and Sydney.
Australia has become the latest country to drop pre-arrival testing for international tourists, joining popular tourist hotspots like South Africa, Canada, the Netherlands, and Thailand. Others have gone even further and eliminated COVID-19-related border protocols completely, including Iceland, Ireland, and the United Kingdom.
In the United States, all international travelers, including U.S. citizens, are still required to get tested within one day of flying to the country, but airlines and travel groups have urged the Biden administration to lift those pandemic-era restrictions.
Alison Fox is a contributing writer for Travel + Leisure. When she's not in New York City, she likes to spend her time at the beach or exploring new destinations and hopes to visit every country in the world. Follow her adventures on Instagram.
Thailand Is Making It Easier for Vaccinated Tourists to Visit — Here's How
Canada Eliminates Pre-arrival Testing for Vaccinated Visitors
Countries That Are Open to COVID-19 Vaccinated Travelers
Canada to Drop All COVID-19 Travel Restrictions on Oct. 1 — What to Know
Thailand to Eliminate All Pandemic-related Travel Restrictions This Week — What to Know
Australia Drops All Remaining Pandemic-related Entry Rules — What to Know
New Zealand Eliminates Vaccine, Testing Requirements for Travel — What to Know
Anguilla Just Dropped Its Pre-arrival Testing for Vaccinated Travelers— What to Know
New Zealand Welcomes Cruise Ships Back as Borders Fully Reopen
U.S. to Drop COVID-19 Testing Requirement for Travelers Entering the Country
These Major Cruise Lines Just Dropped COVID-19 Testing Requirements for Shorter Sailings — What to Know
Belize Just Dropped All COVID-19-related Entry Restrictions — What to Know
The Bahamas Just Eliminated All Pre-arrival Testing for Vaccinated Travelers
Norwegian Cruises to Allow Unvaccinated Passengers Starting in September
Japan Is Making It Easier for Tour Groups to Visit — Here's How
U.S. Virgin Islands Ending All COVID Travel Restrictions for American Travelers — What to Know

redpajama_set_name: RedPajamaCommonCrawl


Luanda – The Angolan renowned singer and songwriter Filipe Mukenga will sing his own classics at the "Show do Mês" (Show of the Month)) project, this Saturday and Saturday, the artist himself has revealed.
Filipe Mukenga will be performing songs like "Nvula", "Weza", "Blues Pala Nguxi", "Fruto Maduro", "Filho de Cabinda", "Dikixi", "Kianda Kianda", "Eu vi Luanda", "Ndilo Keva" and "Mulogi".
The veteran artist will be backed by the Show do Mês band.
Filipe Mukenga started his career in 1964, at the time making a type of music strongly influenced by the western pop music, particularly the Beatles, as the artist himself has revealed.
He recorded his first álbum, entitled « Novo Som », in 1990, having also featured in the album of other artists, such as the « Mingos & Samurais » album of the renowned Portuguese musician Rui Veloso.
« Kianda Kianda », his second album, was recorded in Paris, edited by Lusáfrica and released in 1994. The next work, a music project, came out in 1996 with the name « O Canto da Sereia: o Encanto« , which he co-produced with the singer and songwriter Filipe Zau.
The « O Canto da Sereia: o Encanto » album features several famous Angolan artists, and others, such as Carlos Burity, Katila Mingas, Paulo Flores, Dino, Eduardo Paim and Fernando Tordo.
In 2003 he released the album « Mimbu Iami » recorded in Brazil and Portugal.
In 2008, Filipe Mukenga, alongside Filipe Zau, received the Common Ground Music Award prize, organised by the NGO Search for Common Ground.
His last album entitled « Nós somos nós » was recorded in Brazil, with the participatio and collaboration of renowned Brazilian names like Zeca Baleiro, Ivan Lins and Martinho da Vila.
The Show do Mês project, which started in 2014, aims to valorise Angolan music and musicians, retrieve the works of veteran musicians and give space to new talents.


The Leiper-Smedley Trail is a six-foot-wide, paved, multi-use trail links the historic Leiper House and Park to Smedley Park; and allows access to Strath Haven High School and Middle School and the Community Arts Center. The trail, built during the Blue Route construction, is over two miles long and allows walkers, joggers and bike riders the opportunity to enjoy the Crum Creek Valley. Parking for those who wish to use the trail is available at the Leiper House, mid Avondale Road, and Smedley Park.


text:
<?php

use Illuminate\Database\Seeder;
use ViKon\EveSDE\Models\Inventory\ControlTowerResource;
use ViKon\Utilities\ConsoleProgressbar;

class InvControlTowerResourcesSeeder extends Seeder {
    use ConsoleProgressbar;

    protected $output;

    protected $structure = [
        0 => 'control_tower_type_id',
        1 => 'resource_type_id',
        2 => 'purpose',
        3 => 'quantity',
        4 => 'min_security_level',
        5 => 'faction_id',
    ];

    /**
     * Run the database seeds.
     *
     * @return void
     */
    public function run() {
        DB::table('inv_control_tower_resources')->delete();

        $this->output = $this->command->getOutput();

        $this->initProgressbar();
        $this->startProgress('<info>Inserting data:</info> inv_control_tower_resources');
        $this->setProgressMax(339);

        $data = include(__DIR__ . '/data/inv_control_tower_resources_table_data.php');
        foreach ($data as $row) {
            $this->create($row);
        }
    }

    protected function create($values) {
        $data = [];
        foreach ($this->structure as $i => $key) {
            $data[$key] = $values[$i];
        }
        ControlTowerResource::create($data);
        $this->progress();
    }

}

redpajama_set_name: RedPajamaGithub


Changing career in your 50s - how not to fall off a cliff!
Standing in front of my security cabinet in the Foreign & Commonwealth Office, I spun the combination lock for the last time. After 28 years, with postings in Beijing, Moscow, Berlin and London, I was about to walk out of a high-prestige, secure, established job, into – the unknown.
When people ask me why I left the Diplomatic Service, I always say there were push and pull factors.
On return to the UK after 8 years overseas, I knew I wanted to re-establish roots in London and stay. From my time as the No. 3 in the Berlin Embassy I also knew that I did not want to be an Ambassador: living in the public eye and socialising every evening with strangers did not appeal.
But it was the pull factors which triggered my decision to change career in my 50s. Coming back to London I took a job in the HR function running our coaching operation. I got to train as a coach myself and that was it – I fell in love with coaching and realised that the one-to-one contact and helping others to achieve their potential meant more to me than all the foreign policy in the world.
Nonetheless it took three years of agonising and if it hadn't been for the support and challenge from my own excellent coach, I would never have made the decision to take early retirement and build a second career as a coach and workplace facilitator. Why not?
After 28 years, a workplace becomes more than just that. It is a place where you feel a sense of achievement and competence; you have made friends; you have a common culture and language where you feel you belong. The thought of losing all that overnight paralysed me. But my coach introduced me to the helpful concept of 'wedges'. Rather than think of career change or retirement as a perilous leap from one high block, over a cliff edge, to another, the transition could be gradual, with the career diminishing then tailing off as the post-retirement phase starts up and blossoms.
How to make this work? Could you reduce your hours in your job to start building your post-retirement dream one day a week? Use your evenings to lay the foundations of your new career? Find opportunities in your current job to branch out into your areas of future interest? And once you start the transition, don't fail to draw on any expertise, support or contacts from the past career – there will be more there than you think.
The idea of being asked what I do and no longer being able to say "I work for the Foreign Office" appalled me. In fact, for some months after I retired, my answer was "I used to work for the Foreign Office"! It is hard to let go of the status a career gives us, especially when you don't yet know the new answer, or the answer is "I'm retired".
So a good hard look at your sense of self is inevitable. What really matters to you? What are you proud of in yourself that isn't tied to your career? Experiment with introducing yourself in different ways even before you leave. And reflect on the question - what that you value in yourself does your current career suppress or inhibit?
What will I live on?
I was lucky; I had the cushion of a partner in full-time employment so there was a period of grace before I had to be bringing home any bacon. But the money side of it was nonetheless also scary. The best advice I got about this was to examine my finances ruthlessly: you may have more options than you think. What expenditure could you forego? How much do you actually need to function month to month? What other resources can you draw on – home equity, loans, friends – to tide you over. And remember the wedge model – you may not need to give up all previous income before you establish your new source of earnings.
So how did changing career in my 50s work out?
finally, don't underestimate the powerful force of serendipity. Many leads which I thought would bring me future work went nowhere. But this was more than compensated for by the chance encounters and thrilling surprises once I got out there networking, as well as the dormant contacts which magically started coming out of the woodwork.
Of course, I also had moments of despair and uncertainty. There are many challenges to changing career in your 50s and it seems a much safer option to plough on until 'real' retirement. Only you know what you might miss if you don't take that chance.
Pamela is a coach, mindfulness trainer and HR consultant.


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text:
Meteoritics & Planetary Science, Volume 41 (2006)
Meteoritics & Planetary Science
All of UA Campus RepositoryCommunitiesTitleAuthorsIssue DateSubmit DateSubjectsPublisherJournalThis CommunityTitleAuthorsIssue DateSubmit DateSubjectsPublisherJournal
JournalMeteoritics & Planetary Science (152)AuthorsKoeberl, Christian (6)Ormö, Jens (4)Barlow, Nadine G. (3)Buseck, Peter R. (3)Folco, L. (3)Franchi, I. A. (3)Garvie, Laurence A. J. (3)Gilmour, I. (3)Hörz, Friedrich (3)Kearsley, A. T. (3)View MoreTypestext (152)Article (130)Proceedings (19)Book review (3)SubjectsAbsolute dating (1)Accretion (1)acrylic (1)aerogel (2)Ages (1)View More
Meteoritics & Planetary Science is an international monthly journal of the Meteoritical Society—a scholarly organization promoting research and education in planetary science. Topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors and meteorites, asteroids, comets, craters, and tektites.
Meteoritics & Planetary Science was first published in 1935 under the title Contributions of the Society for Research on Meteorites. In 1947, the publication became known as Contributions of the Meteoritical Society and continued through 1951. From 1953 to 1995, the publication was known as Meteoritics, and in 1996, the journal's name was changed to Meteoritics & Planetary Science or MAPS. The journal was not published in 1952 and from 1957 to 1964.
This archive provides access to Meteoritics & Planetary Science Volumes 37-44 (2002-2009).
Visit Wiley Online Library for new and retrospective Meteoritics & Planetary Science content (1935-present).
Contact the University Libraries Journal Team with questions.
Meteoritics & Planetary Science, Volume 41, Number 12 (2006)
Meteoritics & Planetary Science, Volume 41, Number 9 (2006)
Meteoritics & Planetary Science, Volume 41, Number 8, Supplement (2006)
Noble gas space exposure ages of individual interplanetary dust particles
Kehm, K.; Flynn, G. J.; Sutton, S. R.; Hohenberg, C. M. (The Meteoritical Society, 2006-01-01)
The He, Ne, and Ar compositions of 32 individual interplanetary dust particles (IDPs) were measured using low-blank laser probe gas extraction. These measurements reveal definitive evidence of space exposure. The Ne and Ar isotopic compositions in the IDPs are primarily a mixture between solar wind (SW) and an isotopically heavier component dubbed fractionated solar (FS), which could be implantation-fractionated solar wind or a distinct component of the solar corpuscular radiation previously identified as solar energetic particles (SEP). Space exposure ages based on the Ar content of individual IDPs are estimated for a subset of the grains that appear to have escaped significant volatile losses during atmosphere entry. Although model-dependent, most of the particles in this subset have ages that are roughly consistent with origin in the asteroid belt. A short (<1000 years) space exposure age is inferred for one particle, which is suggestive of cometary origin. Among the subset of grains that show some evidence for relatively high atmospheric entry heating, two possess elevated 21Ne/22Ne ratios generated by extended exposure to solar and galactic cosmic rays. The inferred cosmic ray exposure ages of these particles exceeds 107 years, which tends to rule out origin in the asteroid belt. A favorable possibility is that these 21Ne‐rich IDPs previously resided on a relatively stable regolith of an Edgeworth‐Kuiper belt or Oort cloud body and were introduced into the inner solar system by cometary activity. These results demonstrate the utility of noble gas measurements in constraining models for the origins of interplanetary dust particles.
Frontier Mountain 93001: A coarse-grained, enstatite-augite-oligoclase-rich, igneous rock from the acapulcoite-lodranite parent asteroid
Folco, L.; D'Orazio, M.; Burroni, A. (The Meteoritical Society, 2006-01-01)
The Frontier Mountain (FRO) 93001 meteorite is a 4.86 g fragment of an unshocked, medium-to coarse-grained rock from the acapulcoite-lodranite (AL) parent body. It consists of anhedral orthoenstatite (FS13.3 +/- .04 WO 3.1 +/- 0.2), augite (FS6.1 +/- 0.7 WO42.3 +/- 0.9; Cr2O3 = 1.54 +/- 0.03), and oligoclase (Ab80.5 +/- 3.3 Or 3.1 +/- 0.6) up to >1 cm in size enclosing polycrystalline aggregates of fine-grained olivine (average grain size: 460 +/- 210 micrometers) showing granoblastic textures, often associated with Fe,Ni metal, troilite, chromite (cr# = 0.91 +/- 0.03; fe# = 0.62 +/ 0.04), schreibersite, and phosphates. Such aggregates appear to have been corroded by a melt. They are interpreted as lodranitic xenoliths. After the igneous (the term "igneous" is used here strictly to describe rocks or minerals that solidified from molten material) lithology intruding an acapulcoite host in Lewis Cliff (LEW) 86220, FRO 93001 is the second-known silicate-rich melt from the AL parent asteroid. Despite some similarities, the silicate igneous component of FRO 930011 (i.e., the pyroxene-plagioclase mineral assemblage) differs in being coarser-grained and containing abundant enstatite. Melting-crystallization modeling suggests that FRO 93001 formed through high-degree partial melting (greater than or equal to 35 wt%; namely, greater than or equal to 15 wt% silicate melting and ~20 wt% metal melting) of an acapulcoite source rock, or its chondritic precursor, at temperatures greater than or equal to 1200 degrees C, under reducing conditions. The resulting magnesium-rich silicate melt then underwent equilibrium crystallization; prior to complete crystallization at ~1040 degrees C, it incorporated lodranitic xenoliths. FRO 93001 is the highest-temperature melt from the AL parent-body so far available in laboratory. The fact that FRO 93001 could form by partial melting and crystallization under equilibrium conditions, coupled with the lack of quench-textures and evidence for shock deformation in xenoliths, suggests that FRO 93001 is a magmatic rock produced by endogenic heating rather than impact melting.
The Meteoritical Society, 2006-01-01
Surface electronic states of meteoritic nanodiamonds
Garvie, Laurence A. J.; Buseck, Peter R. (The Meteoritical Society, 2006-01-01)
The C K edge of Orgueil nanodiamonds (C-delta diamonds) was acquired by electron energy-loss spectroscopy (EELS), with an energy resolution of 300 meV. The spectra show peaks at 282.5, 284.7, and 286.4 eV, which occur in the band gap below the main diamond edge and are absent from the bulk diamond spectrum. These peaks are attributed to transitions from degrees C 1s surface core levels to unoccupied surface states, and arise from single and pi-bonded dangling bonds and C-H bonds. A shoulder to the main absorption edge at 287.8 eV may correspond to hydrocarbon adsorbates. These results can be used to further our understanding of C-delta diamond structure and may reveal the presence of a fullerene-like surface. The unique surface electronic states of the C-delta diamond surfaces are expected to affect their optical properties, which are dependent on features such as extent of H coverage, particle size, and surface structure.
Alkali-feldspathic material entrained in Fe,S-rich veins in a monomict ureilite
Warren, Paul H.; Huber, Heinz; Ulff-Møller, Finn (The Meteoritical Society, 2006-01-01)
The Elephant Moraine (EET) 96001 ureilite contains a remarkable diversity of feldspars, which occur as tiny (no more than 60 micrometers maximum dimension) grains within a few Fe,S-rich (now weathered to mostly Fe oxide) veins. Molar S:Fe ratio in the veins averages 0.08 0.02. The veins meander and feature large fluctuations in apparent width; they appear to have entered this monomict breccia by a gentle, percolative process, not by violent impact injection. The feldspars are accompanied by a diverse suite of K-rich (and generally also Ti-rich) feldspathic glasses, and also major proportions of silica and pyroxene, which is largely fassaitic. A rhnite-like phase is also found, and, as inclusions in one of the fassaites, a Cr-poor spinel-like phase. The feldspars mostly feature remarkably high K/Na compared to feldspars of comparable An from polymict ureilites. The EET 96001 feldspathic component was probably once part of a thin basaltic crust on a ureilite asteroid. The spinel included in one of the fassaites formed at remarkably high fO2 (apparent oxidation state of iron: 41 atom% Fe3+), suggesting that the parent magma possibly assimilated near-surface water (however, the Fe3+was not directly measured, and has conceivably been affected by terrestrial weathering; also, there is no assurance that this fassaite originated together with the typical feldspar). We speculate that the feldspathic component was mixed into the dense, Fe,S-rich vein material, and very soon thereafter the Fe,S-rich vein material was emplaced adjacent to the EET 96001 host ureilite, at an advanced stage in a chaotic catastrophic disruption and partial reassembly process that affected all ureilites. The high-K nature of the EET 96001 feldspathic component, including the feldspathic glasses, suggests that fractional fusion may not have been as common during ureilite anatexis as has been inferred from recent studies of clast assemblages in polymict ureilites.
Shock waves-Phenomenology, experimental, and numerial simulationi
Macroscopic subdivision of silica aerogel collectors for sample return missions
Ishii, H. A.; Bradley, J. P. (The Meteoritical Society, 2006-01-01)
Silica aerogel collector tiles have been employed for the collection of particles in low Earth orbit and, more recently, for the capture of cometary particles by NASA's Stardust mission. Reliable, reproducible methods for cutting these and future collector tiles from sample return missions are necessary to maximize the science output from the extremely valuable embedded particles. We present a means of macroscopic subdivision of collector tiles by generating large-scale cuts over several centimeters in silica aerogel with almost no material loss. The cut surfaces are smooth and optically clear allowing visual location of particles for analysis and extraction. This capability is complementary to the smaller-scale cutting capabilities previously described (Westphal 2004; Ishii 2005a, 2005b) for removing individual impacts and particulate debris in tiny aerogel extractions. Macroscopic cuts enable division and storage or distribution of portions of aerogel tiles for immediate analysis of samples by certain techniques in situ or further extraction of samples suited for other methods of analysis. The capability has been implemented in the Stardust Laboratory at NASA's Johnson Space Center as one of a suite of aerogel cutting methods to be used in Stardust sample curation.
TOF-SIMS analysis of Allende projectiles shot into silica aerogel
Stephan, Thomas; Butterworth, Anna L.; Hörz, Friedrich; Snead, Christopher J.; Westphal, Andrew J. (The Meteoritical Society, 2006-01-01)
Powdered Allende projectiles were fired into silica aerogel at 6.1 km/sec in order to evaluate particle retrieval and analysis techniques for samples from the Stardust mission. Since particles may disintegrate and ablate along the penetration paths in a high-porosity aerogel, TOF-SIMS analysis may be a suitable method to determine the distribution of such materials along the tracks as well as potential compositional modifications. Therefore, two 350 micrometer-sized tracks, residing at the surface of a keystone specimen that was flattened between two silicon chips, were analyzed. TOF-SIMS allows for a detailed study of the chemical composition of particles that survived the impact mostly intact and of fine-grained material from disintegrated projectiles. In the investigated keystone, material from light gas gun debris dominated. Besides the two tracks, a continuous, 40-micrometer-thick surface layer of implanted material - probably gun residue - was found. One of the two analyzed tracks is compositionally distinct from this surface layer and is likely to contain residual material of an Allende projectile. The analyses clearly demonstrate that tracks, resulting from impactors in the 5-10 micrometer size range, can be successfully analyzed with TOF-SIMS.
Annual Author Index
Annual Subject Index
Differentiation and evolution of the IVA meteorite parent body: Clues from pyroxene geochemistry in the Steinbach stony-iron meteorite
Ruzicka, A.; Hutson, M. (The Meteoritical Society, 2006-01-01)
We analyzed the Steinbach IVA stony-iron meteorite using scanning electron microscopy (SEM), electron microprobe analysis (EMPA), laser ablation inductively-coupled-plasma mass spectroscopy (LA-ICP-MS), and modeling techniques. Different and sometimes adjacent low-Ca pyroxene grains have distinct compositions and evidently crystallized at different stages in a chemically evolving system prior to the solidification of metal and troilite. Early crystallizing pyroxene shows evidence for disequilibrium and formation under conditions of rapid cooling, producing clinobronzite and type 1 pyroxene rich in troilite and other inclusions. Subsequently, type 2 pyroxene crystallized over an extensive fractionation interval. Steinbach probably formed as a cumulate produced by extensive crystal fractionation (~60-70% fractional crystallization) from a high-temperature (~1450-1490 degrees C) silicate-metallic magma. The inferred composition of the precursor magma is best modeled as having formed by greater than or equal to 30-50% silicate partial melting of a chondritic protolith. If this protolith was similar to an LL chondrite (as implied by O-isotopic data), then olivine must have separated from the partial melt, and a substantial amount (~53-56%) of FeO must have been reduced in the silicate magma. A model of simultaneous endogenic heating and collisional disruption appears best able to explain the data for Steinbach and other IVA meteorites. Impact disruption occurred while the parent body was substantially molten, causing liquids to separate from solids and oxygen-bearing gas to vent to space, leading to a molten metal-rich body that was smaller than the original parent body and that solidified from the outside in. This model can simultaneously explain the characteristics of both stony-iron and iron IVA meteorites, including the apparent correlation between metal composition and metallographic cooling rate observed for metal.
Hydrocode modeling of the Sierra Madera impact structure
Goldin, T. J.; Wünnemann, K.; Melosh, H. J.; Collins, G. S. (The Meteoritical Society, 2006-01-01)
We present the first hydrocode simulations of the formation of the Sierra Madera structure (west Texas, USA), which was caused by an impact into a thick sedimentary target sequence. We modeled Sierra Madera using the iSALE hydrocode, and here we present two best-fit models: 1) a crater with a rim (final crater) diameter of ~12 km, in agreement with previous authors interpretations of the original structure, and 2) a crater ~16 km in diameter with increased postimpact erosion. Both models fit some of the geologic observational data, but discrepancies with estimates of peak shock pressure, extent of deformation, and stratigraphic displacement remain. This study suggests that Sierra Madera may be a larger crater than previously reported and illustrates some of the challenges in simulating impact deformation of sedimentary lithologies. As many terrestrial craters possess some amount of sedimentary rocks in the target sequence, numerical models of impacts into sedimentary targets are essential to our understanding of target rock deformation and the mechanics of crater formation.
Mobile element analysis by secondary ion mass spectrometry (SIMS) of impactite matrix samples from the Yaxcopoil-1 drill core in the Chicxulub impact structure
Newsom, H. E.; Nelson, M. J.; Shearer, C. K.; Dressler, B. O. (The Meteoritical Society, 2006-01-01)
The concentrations of the fluid mobile trace elements lithium, beryllium, boron, and barium were measured in samples of the altered matrix of several impactite breccias of the Yaxcopoil-1 drill core using secondary ion mass spectrometry (SIMS) to determine the extent of transport due to aqueous or hydrothermal processes. Three of the elements, Li, Be, and B, have higher concentrations in the upper suevite impact breccias than in the lower impact melt deposits by factors of 3.5, 2.2, and 1.5, respectively. Lithium and B are the most enriched elements up section, and appear to have had the greatest mobility. The similar fractionation of Li and B is consistent with fluid transport and alteration under low-temperature conditions of less than 150 degrees C based on published experimental studies. In contrast to Li, Be, and B, the concentration of Ba in the altered matrix materials decreases upward in the section, and the concentration of Ba in the matrix is an order of magnitude less than the bulk concentrations, likely due to the presence of barite. The origin of the elemental variations with depth may be related to different protolith compositions in the upper versus the lower impactite units. A different protolith in the altered matrix is suggested by the Mg-rich composition of the lower units versus the Al-rich composition of the upper units, which largely correlates with the mobile element variations. The possibility that vertical transport of mobile elements is due to a postimpact hydrothermal system is supported by published data showing that the sediments immediately overlying the impactites are enriched in mobile elements derived from a hydrothermal system. However, the mobile elements in the sediments do not have to originate from the underlying impactites. In conclusion, our data suggests that the impactites at this location did not experience extensive high-temperature hydrothermal processing, and that only limited transport of some elements, including Li, Be, and B, occurred.
Petrology and geochemistry of a silicate clast from the Mount Padbury mesosiderite: Implications for metal-silicate mixing events of mesosiderite
Tamaki, M.; Yamaguchi, A.; Misawa, K.; Ebihara, M.; Takeda, H. (The Meteoritical Society, 2006-01-01)
Petrological and bulk geochemical studies were performed on a large silicate clast from the Mount Padbury mesosiderite. The silicate clast is composed mainly of pyroxene and plagioclase with minor amounts of ilmenite, spinel, and other accessory minerals, and it shows subophitic texture. Pyroxenes in the clast are similar to those in type 5 eucrites and could have experienced prolonged thermal metamorphism after rapid crystallization from a near-surface melt. Ilmenite and spinel vary chemically, indicating growth under disequilibrium conditions. The clast seems to have experienced an episode of rapid reheating and cooling, possibly as a result of metal-silicate mixing. Abundances of siderophile elements are obviously higher than in eucrites, although the clast is also extremely depleted in highly siderophile elements. The fractionated pattern can be explained by injection of Fe- FeS melts generated by partial melting of metallic portions during metal-silicate mixing. The silicate clast had a complex petrogenesis that could have included: 1) rapid crystallization from magma in a lava flow or a shallow intrusion; 2) prolonged thermal metamorphism to equilibrate the mineral compositions of pyroxene and plagioclase after primary crystallization; 3) metal-silicate mixing probably caused by the impact of solid metal bodies on the surface of the mesosiderite parent body; and 4) partial melting of metal and sulfide portions (and silicate in some cases) caused by the collisional heating, which produced Fe-FeS melts with highly fractionated siderophile elements that were injected into silicate portions along cracks and fractures.
Estimating shock pressures based on high-pressure minerals in shock-induced melt veins of L chondrites
Xie, Z.; Sharp, T. G.; De Carli, P. S. (The Meteoritical Society, 2006-01-01)
Here we report the transmission electron microscopy (TEM) observations of the mineral assemblages and textures in shock-induced melt veins from seven L chondrites of shock stages ranging from S3 to S6. The mineral assemblages combined with phase equilibrium data are used to constrain the crystallization pressures, which can be used to constrain shock pressure in some cases. Thick melt veins in the TenhamL6 chondrite contain majorite and magnesiowstite in the center, and ringwoodite, akimotoite, vitrified silicate-perovskite, and majorite in the edge of the vein, indicating crystallization pressure of ~25 GPa. However, very thin melt veins (5-30 micrometers wide) in Tenham contain glass, olivine, clinopyroxene, and ringwoodite, suggesting crystallization during transient low-pressure excursions as the shock pressure equilibrated to a continuum level. Melt veins of Umbarger include ringwoodite, akimotoite, and clinopyroxene in the vein matrix, and Fe2SiO4-spinel and stishovite in SiO2-FeO-rich melt, indicating a crystallization pressure of ~18 GPa. The silicate melt veins in Roy contain majorite plus ringwoodite, indicating pressure of ~20 GPa. Melt veins of Ramsdorf and Nakhon Pathon contain olivine and clinoenstatite, indicating pressure of less than 15 GPa. Melt veins of Kunashak and La Lande include albite and olivine, indicating crystallization at less than 2.5 GPa. Based upon the assemblages observed, crystallization of shock veins can occur before, during, or after pressure release. When the assemblage consists of high-pressure minerals and that assemblage is constant across a larger melt vein or pocket, the crystallization pressure represents the equilibrium shock pressure.
A study of Mg and K isotopes in Allende CAIs: Implications to the time scale for the multiple heating processes
Ito, M.; Nagasawa, H.; Yurimoto, H. (The Meteoritical Society, 2006-01-01)
The measurements of magnesium and potassium isotopic compositions of refractory minerals in Allende calcium-aluminum-rich inclusions (CAIs), 7R-19-1, HN3-1, and EGG3 were taken by secondary ion mass spectrometry (SIMS). The 7R-19-1 contains 16O-rich and 16O-poor melilite grains and define a single isochron corresponding to an initial 26Al/27Al ratio of (6.6 +/- 1.3) x 10^(-5). The Al-Mg isochron, O isotope measurements and petrography of melilite in 7R-19-1 indicate that 16O-poor melilite crystallized within 0.4 Myr after crystallization of 16O-rich melilite, suggesting that oxygen isotopic composition of the CAI-forming region changed from 16O-rich to 16O-poor within this time interval. The 16O-poor melilite is highly depleted in K compared to the adjacent 16Orich melilite, indicating evaporation during remelting of 7R-19-1. We determined the isochron for 41Ca-41K isotopic systematics in EGG3 pyroxene with (4.1 +/- 2.0) x 10^(-9) (2-sigma) as an initial ratio of 41Ca/40Ca, which is at least two times smaller than the previous result (Sahijipal et al. 2000). The ratio of 41Ca/40Ca in the EGG3 pyroxene grain agrees within error with the value obtained by Hutcheon et al. (1984). No evidence for the presence of 41K excess (decay product of a short-lived radionuclide 41Ca) was found in 7R-19-1 and HN3-1. We infer that the CAI had at least an order of magnitude lower than canonical 41Ca/40Ca ratio at the time of the CAI formation.
Carbon and nitrogen in carbonaceous chondrites: Elemental abundances and stable isotopic compositions
Pearson, V. K.; Sephton, M. A.; Franchi, I. A.; Gibson, J. M.; Gilmour, I. (The Meteoritical Society, 2006-01-01)
We have undertaken a comprehensive study of carbon and nitrogen elemental abundances and isotopic compositions of bulk carbonaceous chondrites. A strategy of multiple analyses has enabled the investigation of hitherto unconstrained small-scale heterogeneities. No systematic differences are observed between meteorite falls and finds, suggesting that terrestrial processing has a minimal effect on bulk carbon and nitrogen chemistry. The changes in elemental abundance and isotopic composition over the petrologic range may reflect variations in primary accreted materials, but strong evidence exists of the alteration of components during secondary thermal and aqueous processing. These changes are reflected within the CM2 and CO3 groups and follow the published alteration scales for those groups. The nitrogen isotope system appears to be controlled by an organic host, which loses a 15N-rich component with progressive alteration. This study recommends caution, however, over the use of bulk carbon and nitrogen information for classification purposes; variance in relative abundance of different components in carbonaceous chondrites is significant and reflects intrameteorite heterogeneities.
Paleomagnetism and petrophysics of the Jänisjärvi impact structure, Russian Karelia
Salminen, J.; Donadini, F.; Pesonen, L. J.; Masaitis, V. L.; Naumov, M. V. (The Meteoritical Society, 2006-01-01)
Paleomagnetic, rock magnetic, and petrophysical results are presented for impactites and target rocks from the Lake Jänisjärvi impact structure, Russian Karelia. The impactites (tagamites, suevites, and lithic breccias) are characterized by increased porosity and magnetization, which is in agreement with observations performed at other impact structures. Thermomagnetic, hysteresis, and scanning electron microscope (SEM) analysis document the presence of primary multidomain titanomagnetite with additional secondary titanomaghemite and ilmenohematite. The characteristic impact-related remanent magnetization (ChRM) direction (D = 101.5 degrees, I = 73.1 degrees, alpha-95 = 6.2 degrees) yields a pole (Lat. = 45.0mdegrees N, Long. = 76.9 degrees E, dp = 9.9 degrees, dm = 11.0 degrees). Additionally, the same component is observed as an overprint on some rocks located in the vicinity of the structure, which provides proofs of its primary origin. An attempt was made to determine the ancient geomagnetic field intensity. Seven reliable results were obtained, yielding an ancient intensity of 68.7 +/- 7.6 micro-T (corresponding to VDM of 10.3 +/- 1.1 x 10^22 Am^2). The intensity, however, appears to be biased toward high values mainly because of the concave shape of the Arai diagrams. The new paleomagnetic data and published isotopic ages for the structure are in disagreement. According to well-defined paleomagnetic data, two possible ages for magnetization of Jänisjärvi rocks exist: 1) Late Sveconorwegian age (900-850 Myr) or 2) Late Cambrian age (~500 Myr). However, published isotopic ages are 718 +/- 5 Myr (K-Ar) and 698 +/- 22 Myr (39Ar-40Ar), but such isotopic dating methods are often ambiguous for the impactites.
Petrology of silicate inclusions in the Sombrerete ungrouped iron meteorite: Implications for the origins of IIE-type silicate-bearing irons
Ruzicka, A.; Hutson, M.; Floss, C. (The Meteoritical Society, 2006-01-01)
The petrography and mineral and bulk chemistries of silicate inclusions in Sombrerete, an ungrouped iron that is one of the most phosphate-rich meteorites known, was studied using optical, scanning electron microscopy (SEM), electron microprobe analysis (EMPA), and secondary ion mass spectrometry (SIMS) techniques. Inclusions contain variable proportions of alkalic siliceous glass (~69 vol% of inclusions on average), aluminous orthopyroxene (~9%, Wo1-4Fs2535, up to ~3 wt% Al), plagioclase (~8%, mainly An7092), Cl-apatite (~7%), chromite (~4%), yagiite (~1%), phosphaterich segregations (~1%), ilmenite, and merrillite. Ytterbium and Sm anomalies are sometimes present in various phases (positive anomalies for phosphates, negative for glass and orthopyroxene), which possibly reflect phosphate-melt-gas partitioning under transient, reducing conditions at high temperatures. Phosphate-rich segregations and different alkalic glasses (K-rich and Na-rich) formed by two types of liquid immiscibility. Yagiite, a K-Mg silicate previously found in the Colomera (IIE) iron, appears to have formed as a late-stage crystallization product, possibly aided by Na-K liquid unmixing. Trace-element phase compositions reflect fractional crystallization of a single liquid composition that originated by low-degree (~48%) equilibrium partial melting of a chondritic precursor. Compositional differences between inclusions appear to have originated as a result of a filter-press differentiation process, in which liquidus crystals of Cl-apatite and orthopyroxene were less able than silicate melt to flow through the metallic host between inclusions. This process enabled a phosphoran basaltic andesite precursor liquid to differentiate within the metallic host, yielding a dacite composition for some inclusions. Solidification was relatively rapid, but not so fast as to prevent flow and immiscibility phenomena. Sombrerete originated near a cooling surface in the parent body during rapid, probably impact-induced, mixing of metallic and silicate liquids. We suggest that Sombrerete formed when a planetesimal undergoing endogenic differentiation was collisionally disrupted, possibly in a breakup and reassembly event. Simultaneous endogenic heating and impact processes may have widely affected silicate-bearing irons and other solar system matter.


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text:
OUTSTANDING SCHOOLS
OUTSTANDING CLASSROOMS
Forest Hill Elementary School
What makes Forest Hill Elementary School Outstanding?
Forest Hill achieved School of the Year through dedicated implementation by their First-Grade
faculty (including Ms. Jamie Evans, Ms. Kathleen Fanelli, Ms. Felicia Santer, and Ms. Amy
Nicholls) and with support from their leadership including Principal Abdur Rahman.
School Demographics
The school serves 283 students in grades kindergarten through Fifth Grade.
The school serves a diverse population, 98% of which are on free/reduced lunch.
Corporate Sponsor
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Click here to learn about Camden City School District's TutorMate Classroom of the Year, Ms. Luppino!
© 2019 Innovations for Learning


text:
Sears Department Store and Auto Center to close this summer…
We don't normally post closures but this one has a "Store Liquidation" attached to it and we like those…lol!
From our friends at KPLC 7 News…
The Sears store and the Sears Auto Center store in Lake Charles are closing, corporate officials said.
The Auto Center is expected to close in early June and the department store is expected to close in mid-August, according to a Sears spokesperson. The store will begin its liquidations sale on May 25.
Kmart will remain open.
From Sears: "We are making the difficult, but necessary decision to close the Sears store and Sears Auto Center in Lake Charles. The store will close to the public in mid August 2018 and the Auto Center will close in early June. Until then, they will remain open for customers. The store will begin its liquidation sale on May 25. We have been strategically and aggressively evaluating our store space and productivity, and have accelerated the closing of unprofitable stores as previously announced. This is not an effort solely aimed at cost savings but is part of a strategy we' have been executing against as many of our larger stores are too big for our needs. Having fewer stores – and the right format – will help us bring Sears Holdings to a size and place to meet the realities of the changing retail world. Our members and customers can also shop at our other Sears locations, which are listed at http://www.sears.com/stores.html. The number of associates is not publicly available. Those associates that are eligible will receive severance and have the opportunity to apply for open positions at area Sears or Kmart stores."
Torchy's Tacos Proposed For Lake Charles
Interactive Tactical Gameplay is Coming to SWLA
Southwest Louisiana Balloon Festival Coming to Lake Charles …


text:
bitflags! {
    flags PDUIWindowFlags_: c_uint {
        const PDUIWINDOWFLAGS_NOTITLEBAR = 1 as c_uint,
        const PDUIWINDOWFLAGS_NORESIZE = 2 as c_uint,
        const PDUIWINDOWFLAGS_NOMOVE = 4 as c_uint,
        const PDUIWINDOWFLAGS_NOSCROLLBAR = 8 as c_uint,
        const PDUIWINDOWFLAGS_NOSCROLLWITHMOUSE = 16 as c_uint,
        const PDUIWINDOWFLAGS_NOCOLLAPSE = 32 as c_uint,
        const PDUIWINDOWFLAGS_ALWAYSAUTORESIZE = 64 as c_uint,
        const PDUIWINDOWFLAGS_SHOWBORDERS = 128 as c_uint,
        const PDUIWINDOWFLAGS_NOSAVEDSETTINGS  = 256 as c_uint,
        const PDUIWINDOWFLAGS_NOINPUTS  = 512 as c_uint,
        const PDUIWINDOWFLAGS_MENUBAR = 1024 as c_uint,
    }
}

#[repr(C)]
#[derive(Debug)]
pub struct PDVec2 {
    pub x: c_float,
    pub y: c_float,
}

#[repr(C)]
pub struct PDVec4 {
    pub x: c_float,
    pub y: c_float,
    pub z: c_float,
    pub w: c_float,
}

#[repr(C)]
pub struct PDRect {
    pub x: c_float,
    pub y: c_float,
    pub width: c_float,
    pub height: c_float,
}

#[repr(C)]
pub struct PDUIInputTextCallbackData {
    pub event_flag: c_uint,
    pub flags: c_uint,
    pub user_data: *mut c_void,
    pub event_char: c_ushort,
    pub event_key: c_ushort,
    pub buf: *mut c_char,
    pub buf_size: c_int,
    pub buf_dirty: c_int,
    pub cursor_pos: c_int,
    pub selection_start: c_int,
    pub selection_end: c_int,
    pub delete_chars: Option<extern "C" fn(data: *mut PDUIInputTextCallbackData, pos: c_int, byteCount: c_int)>,
    pub insert_chars: Option<extern "C" fn(data: *mut PDUIInputTextCallbackData, pos: c_int, text: *const c_char, textEnd: *const c_char)>,
}

#[repr(C)]
pub struct CPdUI {
    pub private_data: *mut c_void,
    pub set_title: extern fn(private_data: *mut c_void, title: *const c_char),
    pub get_window_size: extern fn() -> PDVec2,
    pub get_window_pos: extern fn() -> PDVec2,
    pub begin_child: extern fn(stringId: *const c_char, size: PDVec2, border: c_int, extraFlags: c_int),
    pub end_child: extern fn(),
    pub get_scroll_y: extern fn() -> c_float,
    pub get_scroll_max_y: extern fn() -> c_float,
    pub set_scroll_y: extern fn(scrollY: c_float),
    pub set_scroll_here: extern fn(centerYratio: c_float),
    pub set_scroll_from_pos_y: extern fn(posY: c_float, centerYratio: c_float),
    pub set_keyboard_focus_here: extern fn(offset: c_int),
    pub push_font: extern fn(font: *mut c_void),
    pub pop_font: *mut extern fn() -> c_void,
    pub push_style_color: extern fn(idx: c_uint, col: c_uint),
    pub pop_style_color: extern fn(count: c_int),
    pub push_style_var: extern fn(idx: c_uint, val: c_float),
    pub push_style_var_vec: extern fn(idx: c_uint, val: PDVec2),
    pub pop_style_var: extern fn(count: c_int),
    pub get_font_size: extern fn() -> c_float,
    pub push_item_width: extern fn(item_width: c_float),
    pub pop_item_width: *mut extern fn() -> c_void,
    pub calc_item_width: *mut extern fn() -> c_float,
    pub push_allow_keyboard_focus: extern fn(v: c_int),
    pub pop_allow_keyboard_focus: *mut extern fn() -> c_void,
    pub push_text_wrap_pos: extern fn(wrapPosX: c_float),
    pub pop_text_wrap_pos: *mut extern fn() -> c_void,
    pub push_button_repeat: extern fn(repeat: c_int),
    pub pop_button_repeat: *mut extern fn() -> c_void,
    pub begin_group: *mut extern fn() -> c_void,
    pub end_group: *mut extern fn() -> c_void,
    pub separator: *mut extern fn() -> c_void,
    pub same_line: extern fn(columnX: c_int, spacingW: c_int),
    pub spacing: *mut extern fn() -> c_void,
    pub dummy: extern fn(size: PDVec2),
    pub indent: *mut extern fn() -> c_void,
    pub un_indent: *mut extern fn() -> c_void,
    pub columns: extern fn(count: c_int, id: *const c_char, border: c_int),
    pub next_column: extern fn(),
    pub get_column_index: extern fn() -> c_int,
    pub get_column_offset: extern fn(column_index: c_int) -> c_float,
    pub set_column_offset: extern fn(column_index: c_int, offset_x: c_float),
    pub get_column_width: extern fn(column_index: c_int) -> c_float,
    pub get_columns_count: extern fn() -> c_int,
    pub get_cursor_pos: extern fn() -> PDVec2,
    pub get_cursor_pos_x: extern fn() -> c_float,
    pub get_cursor_pos_y: extern fn() -> c_float,
    pub set_cursor_pos: extern fn(pos: PDVec2),
    pub set_cursor_pos_x: extern fn(x: c_float),
    pub set_cursor_pos_y: extern fn(y: c_float),
    pub get_cursor_screen_pos: extern fn() -> PDVec2,
    pub set_cursor_screen_pos: extern fn(pos: PDVec2),
    pub align_first_text_height_to_widgets: *mut extern fn() -> c_void,
    pub get_text_line_height: *mut extern fn() -> c_float,
    pub get_text_line_height_with_spacing: extern fn() -> c_float,
    pub get_items_line_height_with_spacing: *mut extern fn() -> c_float,
    pub push_id_str: extern fn(strId: *const c_char),
    pub push_id_str_range: extern fn(strBegin: *const c_char, strEnd: *const c_char),
    pub push_id_ptr: extern fn(ptrId: *const c_void),
    pub push_id_int: extern fn(intId: c_int),
    pub pop_id: *mut extern fn() -> c_void,
    pub get_id_str: extern fn(strId: *const c_char) -> c_uint,
    pub get_id_str_range: extern fn(strBegin: *const c_char, strEnd: *const c_char) -> c_uint,
    pub get_id_ptr: extern fn(ptrId: *const c_void) -> c_uint,
    pub text: extern fn(fmt: *const c_char),
    pub text_v: extern fn(fmt: *const c_char, args: c_int),
    pub text_colored: extern fn(col: c_uint, fmt: *const c_char),
    pub text_colored_v: extern fn(col: c_uint, fmt: *const c_char, args: c_int),
    pub text_disabled: extern fn(fmt: *const c_char),
    pub text_disabled_v: extern fn(fmt: *const c_char, args: c_int),
    pub text_wrapped: extern fn(fmt: *const c_char),
    pub text_wrapped_v: extern fn(fmt: *const c_char, args: c_int),
    pub text_unformatted: extern fn(text: *const c_char, text_end: *const c_char),
    pub label_text: extern fn(label: *const c_char, fmt: *const c_char),
    pub label_text_v: extern fn(label: *const c_char, fmt: *const c_char, args: c_int),
    pub bullet: *mut extern fn() -> c_void,
    pub bullet_text: extern fn(fmt: *const c_char),
    pub bullet_text_v: extern fn(fmt: *const c_char, args: c_int),
    pub button: extern fn(label: *const c_char, size: PDVec2) -> c_int,
    pub small_button: extern fn(label: *const c_char) -> c_int,
    pub invisible_button: extern fn(strId: *const c_char, size: PDVec2) -> c_int,
    pub image: extern fn(user_texture_id: *mut c_void, size: PDVec2, uv0: PDVec2, uv1: PDVec2, tintColor: c_uint, borderColor: c_uint),
    pub image_button: extern fn(user_texture_id: *mut c_void, size: PDVec2, uv0: PDVec2, uv1: PDVec2, framePadding: c_int, bgColor: c_uint, tintCol: c_uint) -> c_int,
    pub collapsing_header: extern fn(label: *const c_char, strId: *const c_char, displayFrame: c_int, defaultOpen: c_int) -> c_int,
    pub checkbox: extern fn(label: *const c_char, v: *mut c_int) -> c_int,
    pub checkbox_flags: extern fn(label: *const c_char, flags: *mut c_uint, flagsValue: c_uint) -> c_int,
    pub radio_button_bool: extern fn(label: *const c_char, active: c_int) -> c_int,
    pub radio_button: extern fn(label: *const c_char, v: *mut c_int, v_button: c_int) -> c_int,
    pub combo: extern fn(label: *const c_char, currentItem: *mut c_int, items: *mut *const c_char, itemsCount: c_int, heightInItems: c_int) -> c_int,
    pub combo2: extern fn(label: *const c_char, currentItem: *mut c_int, itemsSeparatedByZeros: *const c_char, heightInItems: c_int) -> c_int,
    pub combo3: extern fn(label: *const c_char, currentItem: *mut c_int, itemsGetter: extern fn(data: *mut c_void, idx: c_int, out_text: *mut *const c_char) -> c_int, data: *mut c_void, itemsCount: c_int, heightInItems: c_int) -> c_int,
    pub color_button: extern fn(col: c_uint, smallHeight: c_int, outlineBorder: c_int) -> c_int,
    pub color_edit3: extern fn(label: *const c_char, col3: *mut c_float) -> c_int,
    pub color_edit4: extern fn(label: *const c_char, col4: *mut c_float, showAlpha: c_int) -> c_int,
    pub color_edit_mode: extern fn(mode: c_uint),
    pub plot_lines: extern fn(label: *const c_char, values: *const c_float, valuesCount: c_int, valuesOffset: c_int, overlayText: *const c_char, scaleMin: c_float, scaleMax: c_float, graphSize: PDVec2, stride: c_int),
    pub plot_lines2: extern fn(label: *const c_char, valuesGetter: extern fn(data: *mut c_void, idx: c_int) -> c_float, data: *mut c_void, valuesCount: c_int, valuesOffset: c_int, overlayText: *const c_char, scaleMin: c_float, scaleMax: c_float, graphSize: PDVec2),
    pub plot_histogram: extern fn(label: *const c_char, values: *const c_float, valuesCount: c_int, valuesOffset: c_int, overlayText: *const c_char, scaleMin: c_float, scaleMax: c_float, graphSize: PDVec2, stride: c_int),
    pub plot_histogram2: extern fn(label: *const c_char, valuesGetter: extern fn(data: *mut c_void, idx: c_int) -> c_float, data: *mut c_void, valuesCount: c_int, valuesOffset: c_int, overlayText: *const c_char, scaleMin: c_float, scaleMax: c_float, graphSize: PDVec2),
    pub sc_input_text: extern fn(label: *const c_char, xSize: c_float, ySize: c_float) -> *mut PDUISCInterface,
    pub slider_float: extern fn(label: *const c_char, v: *mut c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub slider_float2: extern fn(label: *const c_char, v2: *mut c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub slider_float3: extern fn(label: *const c_char, v3: *mut c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub slider_float4: extern fn(label: *const c_char, v4: *mut c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub slider_angle: extern fn(label: *const c_char, v_rad: *mut c_float, vDegreesMin: c_float, vDegreesMax: c_float) -> c_int,
    pub slider_int: extern fn(label: *const c_char, v: *mut c_int, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub slider_int2: extern fn(label: *const c_char, v2: *mut c_int, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub slider_int3: extern fn(label: *const c_char, v3: *mut c_int, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub slider_int4: extern fn(label: *const c_char, v4: *mut c_int, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub vslider_float: extern fn(label: *const c_char, size: PDVec2, v: *mut c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub vslider_int: extern fn(label: *const c_char, size: PDVec2, v: *mut c_int, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub drag_float: extern fn(label: *const c_char, v: *mut c_float, vSpeed: c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub drag_float2: extern fn(label: *const c_char, v2: *mut c_float, vSpeed: c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub drag_float3: extern fn(label: *const c_char, v3: *mut c_float, vSpeed: c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub drag_float4: extern fn(label: *const c_char, v4: *mut c_float, vSpeed: c_float, vMin: c_float, vMax: c_float, displayFormat: *const c_char, power: c_float) -> c_int,
    pub drag_int: extern fn(label: *const c_char, v: *mut c_int, vSpeed: c_float, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub drag_int2: extern fn(label: *const c_char, v2: *mut c_int, vSpeed: c_float, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub drag_int3: extern fn(label: *const c_char, v3: *mut c_int, vSpeed: c_float, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub drag_int4: extern fn(label: *const c_char, v4: *mut c_int, vSpeed: c_float, vMin: c_int, vMax: c_int, displayFormat: *const c_char) -> c_int,
    pub input_text: extern fn(label: *const c_char, buf: *mut c_char, buf_size: c_int, flags: c_int, callback: extern fn(*mut PDUIInputTextCallbackData) -> c_void, user_data: *mut c_void) -> c_int,
    pub input_text_multiline: extern fn(label: *const c_char, buf: *mut c_char, buf_size: c_int, size: PDVec2, flags: c_uint, callback: extern fn(*mut PDUIInputTextCallbackData) -> c_void, user_data: *mut c_void) -> c_int,
    pub input_float: extern fn(label: *const c_char, v: *mut c_float, step: c_float, step_fast: c_float, decimal_precision: c_int, extraFlags: c_uint) -> c_int,
    pub input_float2: extern fn(label: *const c_char, v2: *mut c_float, decimal_precision: c_int, extraFlags: c_uint) -> c_int,
    pub input_float3: extern fn(label: *const c_char, v3: *mut c_float, decimal_precision: c_int, extraFlags: c_uint) -> c_int,
    pub input_float4: extern fn(label: *const c_char, v4: *mut c_float, decimal_precision: c_int, extraFlags: c_uint) -> c_int,
    pub input_int: extern fn(label: *const c_char, v: *mut c_int, step: c_int, step_fast: c_int, extraFlags: c_uint) -> c_int,
    pub input_int2: extern fn(label: *const c_char, v2: *mut c_int, extraFlags: c_uint) -> c_int,
    pub input_int3: extern fn(label: *const c_char, v3: *mut c_int, extraFlags: c_uint) -> c_int,
    pub input_int4: extern fn(label: *const c_char, v4: *mut c_int, extraFlags: c_uint) -> c_int,
    pub tree_node: extern fn(str_label_id: *const c_char) -> c_int,
    pub tree_node_str: extern fn(strId: *const c_char, fmt: *const c_char) -> c_int,
    pub tree_node_ptr: extern fn(ptrId: *const c_void, fmt: *const c_char) -> c_int,
    pub tree_node_str_v: extern fn(strId: *const c_char, fmt: *const c_char, args: c_int) -> c_int,
    pub tree_node_ptr_v: extern fn(ptrId: *const c_void, fmt: *const c_char, args: c_int) -> c_int,
    pub tree_push_str: extern fn(strId: *const c_char),
    pub tree_push_ptr: extern fn(ptrId: *const c_void),
    pub tree_pop: *mut extern fn() -> c_void,
    pub set_next_tree_node_opened: extern fn(opened: c_int, cond: c_uint),
    pub selectable: extern fn(label: *const c_char, selected: c_int, flags: c_uint, size: PDVec2) -> c_int,
    pub selectable_ex: extern fn(label: *const c_char, p_selected: *mut c_int, flags: c_uint, size: PDVec2) -> c_int,
    pub list_box: extern fn(label: *const c_char, currentItem: *mut c_int, items: *mut *const c_char, itemsCount: c_int, heightInItems: c_int) -> c_int,
    pub list_box2: extern fn(label: *const c_char, currentItem: *mut c_int, itemsGetter: extern fn(data: *mut c_void, idx: c_int, out_text: *mut *const c_char) -> c_int, data: *mut c_void, itemsCount: c_int, heightInItems: c_int) -> c_int,
    pub list_box_header: extern fn(label: *const c_char, size: PDVec2) -> c_int,
    pub list_box_header2: extern fn(label: *const c_char, itemsCount: c_int, heightInItems: c_int) -> c_int,
    pub list_box_footer: *mut extern fn() -> c_void,
    pub set_tooltip: extern fn(fmt: *const c_char),
    pub set_tooltip_v: extern fn(fmt: *const c_char, args: c_int),
    pub begin_tooltip: *mut extern fn() -> c_void,
    pub end_tooltip: *mut extern fn() -> c_void,
    pub begin_main_menu_bar: *mut extern fn() -> c_int,
    pub end_main_menu_bar: *mut extern fn() -> c_void,
    pub begin_menu_bar: *mut extern fn() -> c_int,
    pub end_menu_bar: *mut extern fn() -> c_void,
    pub begin_menu: extern fn(label: *const c_char, enabled: c_int) -> c_int,
    pub end_menu: extern fn(),
    pub menu_item: extern fn(label: *const c_char, shortcut: *const c_char, selected: c_int, enabled: c_int) -> c_int,
    pub menu_item_ptr: extern fn(label: *const c_char, shortcut: *const c_char, p_selected: *mut c_int, enabled: c_int) -> c_int,
    pub open_popup: extern fn(strId: *const c_char),
    pub begin_popup: extern fn(strId: *const c_char) -> c_int,
    pub begin_popup_modal: extern fn(name: *const c_char, p_opened: *mut c_int, extraFlags: c_uint) -> c_int,
    pub begin_popup_context_item: extern fn(strId: *const c_char, mouse_button: c_int) -> c_int,
    pub begin_popup_context_window: extern fn(also_over_items: c_int, strId: *const c_char, mouse_button: c_int) -> c_int,
    pub begin_popup_context_void: extern fn(strId: *const c_char, mouse_button: c_int) -> c_int,
    pub end_popup: extern fn(),
    pub close_current_popup: *mut extern fn() -> c_void,
    pub begin_popup_context: extern fn(priv_data: *mut c_void) -> c_int,
    pub end_popup_context: extern fn(priv_data: *mut c_void),
    pub value_bool: extern fn(prefix: *const c_char, b: c_int),
    pub value_int: extern fn(prefix: *const c_char, v: c_int),
    pub value_u_int: extern fn(prefix: *const c_char, v: c_uint),
    pub value_float: extern fn(prefix: *const c_char, v: c_float, float_format: *const c_char),
    pub color: extern fn(prefix: *const c_char, col: c_uint),
    pub log_to_tty: extern fn(maxDepth: c_int),
    pub log_to_file: extern fn(maxDepth: c_int, filename: *const c_char),
    pub log_to_clipboard: extern fn(maxDepth: c_int),
    pub log_finish: *mut extern fn() -> c_void,
    pub log_buttons: *mut extern fn() -> c_void,
    pub is_item_hovered: *mut extern fn() -> c_int,
    pub is_item_hovered_rect: *mut extern fn() -> c_int,
    pub is_item_active: *mut extern fn() -> c_int,
    pub is_item_visible: *mut extern fn() -> c_int,
    pub is_any_item_hovered: *mut extern fn() -> c_int,
    pub is_any_item_active: *mut extern fn() -> c_int,
    pub get_item_rect_min: *mut extern fn() -> PDVec2,
    pub get_item_rect_max: *mut extern fn() -> PDVec2,
    pub get_item_rect_size: *mut extern fn() -> PDVec2,
    pub is_window_hovered: *mut extern fn() -> c_int,
    pub is_window_focused: *mut extern fn() -> c_int,
    pub is_root_window_focused: *mut extern fn() -> c_int,
    pub is_root_window_or_any_child_focused: *mut extern fn() -> c_int,
    pub is_rect_visible: extern fn(itemSize: PDVec2) -> c_int,
    pub is_pos_hovering_any_window: extern fn(pos: PDVec2) -> c_int,
    pub get_time: *mut extern fn() -> c_float,
    pub get_frame_count: *mut extern fn() -> c_int,
    pub get_style_col_name: extern fn(idx: c_uint) -> *const c_char,
    pub calc_item_rect_closest_point: extern fn(pos: PDVec2, on_edge: c_int, outward: c_float) -> PDVec2,
    pub calc_text_size: extern fn(text: *const c_char, text_end: *const u8, hide_text_after_double_hash: c_int, wrap_width: c_float) -> PDVec2,
    pub calc_list_clipping: extern fn(items_count: c_int, items_height: c_float, out_items_display_start: *mut c_int, out_items_display_end: *mut c_int),
    pub begin_child_frame: extern fn(id: c_uint, size: PDVec2) -> c_int,
    pub end_child_frame: *mut extern fn() -> c_void,
    pub color_convert_rg_bto_hsv: extern fn(r: c_float, g: c_float, b: c_float, out_h: *mut c_float, out_s: *mut c_float, out_v: *mut c_float),
    pub color_convert_hs_vto_rgb: extern fn(h: c_float, s: c_float, v: c_float, out_r: *mut c_float, out_g: *mut c_float, out_b: *mut c_float),
    pub is_key_down: extern fn(key_index: c_int) -> c_int,
    pub is_key_pressed: extern fn(key_index: c_int, repeat: c_int) -> c_int,
    pub is_key_released: extern fn(key_index: c_int) -> c_int,
    pub is_key_down_id: extern fn(keyId: c_uint, repeat: c_int) -> c_int,
    pub is_mouse_down: extern fn(button: c_int) -> c_int,
    pub is_mouse_clicked: extern fn(button: c_int, repeat: c_int) -> c_int,
    pub is_mouse_double_clicked: extern fn(button: c_int) -> c_int,
    pub is_mouse_released: extern fn(button: c_int) -> c_int,
    pub is_mouse_hovering_window: *mut extern fn() -> c_int,
    pub is_mouse_hovering_any_window: *mut extern fn() -> c_int,
    pub is_mouse_hovering_rect: extern fn(rectMin: PDVec2, rectMax: PDVec2) -> c_int,
    pub is_mouse_dragging: extern fn(button: c_int, lockThreshold: c_float) -> c_int,
    pub get_mouse_pos: *mut extern fn() -> PDVec2,
    pub get_mouse_drag_delta: extern fn(button: c_int, lockThreshold: c_float) -> PDVec2,
    pub reset_mouse_drag_delta: extern fn(button: c_int),
    pub get_mouse_cursor: *mut extern fn() -> c_uint,
    pub set_mouse_cursor: extern fn(ctype: c_uint),
    pub fill_rect: extern fn(rect: PDRect, color: c_uint),
    pub fill_convex_poly: extern fn(verts: *const c_void, count: c_uint, color: c_uint, aa: c_int),
    pub fill_circle: extern fn(pos: PDVec2, radius: c_float, color: c_uint, num_seg: c_uint, aa: c_int),
    pub image_create_rgba: extern fn(width: c_uint, height: c_uint) -> *mut c_void,
    pub image_update: extern fn(dest: *mut c_void, src: *const c_void, size: c_uint) -> c_void,
}

// !!! End of autogenerated data. !!!


Spectrum is a Star Trek: The Farthest Star title used to label stories that take place in an alternate universe from the main TFS timeline.
The following stories take place in an alternate universe that originated in "The Final Prophecy". This timeline branched off from the main timeline during Operation Return in 2373. The critical event is the destruction of the USS Defiant in the Bajoran wormhole and the failure to prevent the Dominion from reinforcing its position in the Alpha Quadrant.
"A New Path" Unknown (2376) In an alternate universe Terri Letac finds a new direction in her life after the fall of the Federation.
"The Final Prophecy" Unknown (2394) In an alternate universe where the Dominion won the Dominion War Jake Sisko finds himself on a path of prophecy and destiny.
Star Trek: Unity was a crossover Swiftfire was involved with. They are based on the continuity before SWF was merged into Star Trek: The Farthest Star and the continuity rebooted. As such they are currently considered to be in an alternate universe from TFS.
It is planned for these stories to be eventually rewritten to be consistent with TFS.
This story is based in an alternate universe where the Federation falls into civil war after the coup d'état by Admiral Leyton in 2372.
This story was partially released prior to the reboot. At the moment it is unsure if it will be rewritten or discarded.
"There's No Angels Here" Unknown (2374) While on a mission inside the Badlands the USS Swiftfire-A is attacked by three Vendoth warships. Outnumbered, outgunned and on the run the Swiftfire's situation looks grim but unknown to the crew there are two other beings that are on their side and willing to help.


text:
est le sixième album studio du groupe de death metal américain Obituary, sorti en .

Après huit années de pause , cet album marque le retour du groupe. Scott Burns, collaborateur de longue date (mais qui n'a pas travaillé avec Obituary depuis  en 1994), produit à nouveau l'album.

 est le dernier opus à présenter le guitariste Allen West.

Un clip est réalisé pour la chanson .

Liste des titres

Crédits

Membres du groupe
 John Tardy : chant guttural
 Frank Watkins : basse
 Trevor Peres : guitare rythmique
 Allen West : guitare rythmique et solo
 Donald Tardy : batterie

Équipes technique et production
 Production : Mark Prator, Obituary
 Producteur délégué : Scott Burns
 Ingénierie, mixage : Mark Prator
 Ingénierie (assistant) : Aaron Callier
 Mastering : Tom Morris
 Photographie : Daragh McDonagh
 Design : Trevor Peres
 Artwork, illustrations (pochette) : Andreas Marschall

Notes et références

Liens externes

Album musical sorti en 2005
Album d'Obituary
Album de death metal
Album produit par Scott Burns
Album publié par Roadrunner Records

redpajama_set_name: RedPajamaWikipedia


text:
Харла́мовка — деревня Долгоруковского сельского поселения Долгоруковского района Липецкой области.

География

харламовка находится в центральной части Долгоруковского района, в 3 км к югу от села Долгоруково. Располагается на берегах небольшой запруды, в истоке реки Снова.

История
Харламовка возникла не позднее второй половины XVIII века. Впервые упоминается в «Экономических примечаниях Елецкого уезда» 1778 года, как «деревня Харламовка, 3 двора. Поселена на земле, купленной помещиком И.И. Ильиным в Межевой канцелярии». Название по фамилии Харламов.

В «Списке населенных мест» Орловской губернии 1866 года значится как «деревня владельческая Харламовка при колодцах, 51 двор, 612 жителей».

В 1905 году Харламовка упоминается как одно из селений в приходе Троицкой церкви села Братовщина.

В 1932 году в Харламовке числится 552 жителя.

В 1928 году деревня вошла в состав Долгоруковского района Елецкого округа Центрально-Чернозёмной области. После разделения ЦЧО в 1934 году Долгоруковский район вошёл в состав Воронежской, в 1935 — Курской, в 1939 году — Орловской области, а с 6 января 1954 года в составе вновь образованной Липецкой области.

Население

Транспорт
Деревня Харламовка связана асфальтированной автодорогой с деревней Новинка и селом Долгоруково, грунтовой дорогой с деревней Ивановка.

На западе деревни находится железнодорожная станция Ост. плат. 479 км (линия Елец – Валуйки ЮВЖД).

Известные жители
 Ловчий, Адам Герасимович. Полный кавалер Ордена Славы. В годы Великой Отечественной войны – сапер. Уроженец города Кельце (Польша), после войны жил в деревне Харламовка.

Примечания

Ссылки
 Официальный сайт Долгоруковского района Липецкой области «www.dolgorukovo.org»

Населённые пункты Долгоруковского района


The Georgia Bulldogs have dropped to 14th in the College Football Playoff rankings that were released tonight by the Selection Committee. Georgia fell to Georgia Tech 30-24 in overtime on Saturday.
Prior to the Georgia Tech game, the Bulldogs had achieved their highest CFP ranking at No. 9. The Yellow Jackets have now moved up spots to No. 12.
Alabama remained in the top spot, and the Crimson Tide are followed by Oregon in 2nd, TCU in 3rd, and Florida State in 4th. FSU continues to fall even though they are undefeated.
Other ranked SEC teams include Ole Miss (12), Missouri (16), Auburn (19), and LSU (24).


text:
Jontrell Walker receives release from Ball State basketball
Jontrell Walker will have one season of eligibility left.
Jontrell Walker receives release from Ball State basketball Jontrell Walker will have one season of eligibility left. Check out this story on thestarpress.com: http://tspne.ws/2FViqjf
Ryan O'Gara, The Star Press Published 3:56 p.m. ET March 22, 2018 | Updated 3:57 p.m. ET March 23, 2018
The 6-foot-1 guard hasn't been with the program since early January after getting suspended.
Ball State's Jontrell Walker looks to shoot past IUPUI's defense during their game at Worthen Arena Saturday, Dec. 2, 2017. (Photo: Jordan Kartholl / The Star Press)Buy Photo
Jontrell Walker averaged 7.9 points and shot 38 percent from 3-point range.
MUNCIE, Ind. — Jontrell Walker has been granted his release from the Ball State men's basketball program, he announced on Thursday. The redshirt junior guard will graduate in May from Ball State and have one year of eligibility remaining. He will be eligible immediately.
Walker posted on Twitter, "I received my release today from Ball State. I appreciate everything Ball State has done for me but I feel it is in my best interest academically and athletically to continue my career at another university!"
Walker was suspended indefinitely on Jan. 6 after being arrested on preliminary charges of domestic battery and interfering with the reporting of a crime. He was not with the team for the duration of the season.
Whitford met with Walker on Thursday.
"I completely support Jontrell's decision," Whitford said when reached for comment. "He is going to be graduated in four years and give himself a chance to be part of this graduate transfer rule. We wish him nothing but the best going forward."
The 6-foot-1 junior averaged 7.9 points in his one season with the Cardinals. After transferring from Incarnate Word, he sat out the 2016-17 season and then provided a spark off the bench in the early part of the season, scoring 23 points against Oklahoma. He was inserted into the starting lineup on Nov. 25 against Indiana State, and Ball State rattled off nine straight wins until he was suspended.
Ball State has two scholarships available for next season.
I received my release today from Ball State. I appreciate everything Ball State has done for me but I feel it is in my best interest academically and athletically to continue my career at another university!
— Trell (@Trell_0) March 22, 2018
Teammates Trey Moses and Ishmael El-Amin tweeted their support.
Let's get it bro ✊🏾 you know I'm gonna miss you ! See you at the top https://t.co/XSEj4TY13d
— My names Trey nd I have a basketball game tomorrow (@treymoses32) March 22, 2018
One Love my brotha 💯 wherever you end up they getting a good one 💯‼ https://t.co/mozH2CbO4S
— Ishh El-Amin™ (@TheNextElAmin) March 22, 2018


Description: |POSITION CLOSED - STILL ACCEPTING RESUMES FOR FUTURE OPPORTUNITIES || Our Client is seeking a Nuclear I&C Procedure Writer for Soddy Daisy, TN. The assignment length will be 6-9 months long (possibly up to 1 yr.). || JOB DESCRIPTION: Candidates will have I&C Background and possess the ability to read, write and review I&C procedures. This is for several large nuclear projects.
Qualifications: || QUALIFICATIONS: || -PPA Certification Required -Nuclear Utility Experience writing I&C procedures -I&C Background Preferred -Minimum 5 years experience in Procedure Writing -Will need to submit 3 professional references along with resume for consideration.
Please complete this form and attach your resume in order to apply for this job.


90210 (Brenda Walsh for life!) and Charmed favorite, Shannen Doherty, broke all of our collective hearts when she announced that she had been diagnosed with breast cancer a little over a year ago.
Since then, the star received a single mastectomy in May, and has recently begun undergoing chemotherapy treatments to treat her illness. While one might have expected her to do so privately, keeping her most vulnerable moments hidden away behind closed doors, Shannen has done just the opposite.
The incredibly brave star has made the decision to be open about her journey, sharing both her highs and lows on social media for the world to see and opening herself up to connection with others sharing many of her same struggles.
Most memorable was this shot she shared of herself gazing into the distance just moments after she had shaved her head.
"Step 6," she wrote, a reference to the number of steps she went through that day to arrive at the starkly beautiful black and white pic.
Since then, we've seen her at her best, on days when she felt incredibly strong.
We've also seen her on the days she didn't feel quite so hot, more often than not accompanied by the ones who love her most. From her incredibly devoted husband, Kurt Iswarienko (who actually texted her, "Oh my God. You're hot with no hair" *SWOON*), to gal pal Sarah Michelle Gellar (who posted her own tribute to Shannen in a truly awesome #wcw moment), Shannen's friends and family have gathered around her to show their support, and none more so than her mother, Rosa.
"Step 1," she captioned the above shot prior to undergoing the scissors.
Now, the star has taken time out to thank her mother in a post that truly had us in tears. Showcasing her curled up in her mother's lap like a little girl as Rosa pokes her dimples, Shannen writes as follows.
WOW. Okay, we're gonna need a second to recover. What an inspiring woman and family!
Thank YOU for sharing your journey, Shannen — we're all behind you, 1,000%.
Are you touched by Shannen's personal journey? Share with us over @BritandCo.


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Long-duration energy storage should scale up 400x by 2040, bp, Siemens and ESS-backed group says
Published Nov. 23, 2021
Jason Plautz Contributor
Adeline Kon/Utility Dive
By 2040, deployments of long-duration energy storage systems should be scaled up approximately 400 times present day levels to build a worldwide cost-optimal net-zero energy system, according to a report released today by the Long Duration Energy Storage (LDES) Council.
In order to make LDES economically viable, the report finds that LDES costs must decrease by 60%. That would require a total investment of between $1.5 trillion and $3 trillion around the world between 2022 and 2040, which the report says is equivalent to the amount spent on transmission and distribution networks every two to four years.
Widespread deployment of LDES could provide up to 140 TWh of energy capacity by 2040, which would store 10% of all electricity consumed worldwide in a net-zero energy system. That would result in savings of 1.5 to 2.3 gigatonnes of carbon dioxide equivalent, 10 to 15% of today's power sector emissions, the report said.
Executives from 25 energy and technology companies launched the LDES Council during the United Nations climate change summit in Glasgow, Scotland, earlier this month. The group aims to educate companies, governments and utilities on LDES technologies and encourage policies to support mass deployment of long-duration storage, generally defined as energy storage systems lasting at least four hours. The technology, backers say, will be crucial to a decarbonized grid in order to store and dispatch energy at times when the sun is not shining or the wind is not blowing.
"I think a big reason for us to be part of the [UN] discussion is that this a real, doable thing," said Eric Dresselhuys, CEO of flow battery company ESS Inc. and a founding member of the council. "This isn't some theory about what could potentially be done from a policy perspective 20 years from now. Long-duration storage is a practical solution that's available today that can help make the energy transition real."
Other founding members of the council include bp, Siemens Energy, Highview Power, Form Energy and other storage and energy firms.
The Department of Energy announced in July an ambitious program to lower the cost of storage technology by 90% over the next decade, backed by government-funded research and pilot programs. California, as part of its goal to reach 100% renewable energy by 2050, has an interim target of deploying nearly 1 GW of long-duration storage by 2026. Although a number of large storage projects have launched in the past year, the vast majority of storage is based on shorter-duration lithium-ion technology.
The report — prepared by the LDES Council in collaboration with McKinsey & Company — says that LDES deployment could "accelerate rapidly in the next few years," especially as countries continue to expand renewable energy. Once renewables reach a 60 to 70% market share of bulk power systems, the report found, LDES will be catalyzed "as the lowest-cost flexibility solution." However, before that deployment can take place, technology costs need to drop significantly, in line with the cost reductions in other renewable technologies spurred by more research and market knowledge.
That's a finding widely shared by energy experts; a study published earlier this year in Nature Energy found that the energy capacity cost for an LDES solution would have to drop to $10 per kWh to fully displace nuclear power and would have to get to $1 per kWh to displace natural gas power plants with carbon capture and sequestration.
However, Dresselhuys said the current momentum behind the industry and the clear role for LDES defined in the report means there is reason to think the lofty deployment goals could be achieved.
"This is a huge market and even if the penetration in terms of percentages is relatively low, it's a really big and meaningful business with a bright future," said Dresselhuys. "I think we're right on the cusp."
DOE initiative seeks to drop long-duration storage cost 90% in a decade By Jason Plautz • July 14, 2021
Filed Under: Energy Storage
Elenathewise via Getty Images
High electricity rates impede crucial but costly technology investments to manage rising DER levels: utilities
Utilities want distribution system technologies for more DER visibility and control. But advocates want a new national stakeholder dialogue about the timing of spending for DER integration.
By Herman K. Trabish • Nov. 29, 2022
SYSO Technologies Breaks Through with 1 GW of Renewable Energy Under Management From SYSO Technologies
SYSO Technologies Breaks Through with 1 GW of Renewable Energy Under Management
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how do salmon go from freshwater to saltwater
What happens is that the kidney of the salmon is able to deal with the change from saltwater to freshwater by altering function and excreting a large volume of dilute urine. Salmon eggs are laid in freshwater streams typically at high latitudes. As the name implies, the machine spends ATP to operate on sodium (Na) and potassium (K) ions. However, like virtually all osmoregulators, the salmon is never in true equilibrium with its surroundings. Safety concerns are a bit more involved than with freshwater salmon fishing, so make sure that you prepare accordingly! It is not intended to provide medical or other professional advice. The Alaska Moose Hunting Guidebook is now available. If the environment is poor for en extended period, their learning ability declines. The work to develop this is already under way. The research group in Bergen is unique because its work is so interdisciplinary. In simple words, it is the ability of a solution to exert osmotic pressure upon a membrane. The fry quickly develop into parr with camouflaging vertical stripes. Source(s): Book: "The Salmon Fishing Adventure: How to Locate, Lure, and Land the Big Salmon and More." Numerous examples of fully freshwater (i.e., "landlocked") populations of the species exist throughout the Northern Hemisphere, including a now extinct population in Lake Ontario, which have been shown in recent studies to … While foraging and exploring the ocean during midlife. At … In a country where fish plays such an important role in society, a centre that can give new insight to important fundamental questions on brain function will also impact how we manage wild fish populations and improve aquaculture practices," says Ebbesson. In contrast, freshwater fish do not have a briny flavor and tend to have a milder flavor profile. Here they will also expand and centralise technological resources and neuroanatomical-databases. Nov 21, 2007 #1 Can saltwater fish be converted to freshwater, while slowly adding less salt in the tank? Sockeye Salmon Feeding. Adult salmon dine mostly on other fish. However, like virtually all osmoregulators, the salmon is never in true equilibrium with its surroundings. On the other hand, salmon and trout are euryhaline fishes, living part of their lives in freshwater and then migrating to their marine saltwater habitats. Dealing with Salt: Osmoregulation. First they must switch from using saltwater to freshwater. The centre will make it possible for researchers to take a closer look at specific regulation and functions in fish brains. Because fresh water is low in sodium, salmon need their gill cells to pump it in as they swim downstream. _____ 4. NKA is essential for numerous functions. Salmon go from saltwater back to their natal freshwater streams to spawn. Salt controls water absorption so the cells would gain water. Not that I'm aware … Salmon are also indicators of healthy river and marine ecosystems — as habitats degrade and disappear, so do salmon, and as salmon disappear, the quality of the ecosystem decreases as well, since salmon are an important source of nutrients. From a design perspective, the third change is very interesting. "We have presumed that changes in thyroid hormones have been important for normal smolt development, but we have not known how the hormone is activated and it specific roles," says Lars Ebbesson. Toolson briefly discusses how the salmon drink more water and concentrate their urine when entering the ocean, but then spends his best praise describing the NKA pumps. The researchers at Uni Research Environment have now found important clues that may provide an answer. They will also consume insects and shrimp. Through research here, they will be able to arrive at important answers to help both those who work with fish and those who work with people. Let's say you do want to go this route and use your bass boat in saltwater, what are some things you can do to protect your bass boat and get as much life out of it as possible. The salmon is an excellent osmoregulator. Atlantic salmon have been introduced to freshwater environments around the world. Joined Mar 12, 2007 Messages 1,896 Reaction score 0 Location Coventry, West Midlands. "This kind of integrative approach is important in order to solve challenges with regulation of life-history transitions, behavioural motivation and environmental and genetic modulation of adaptation. The tiny fish hatch and usually stay in the river for a year before migrating to the ocean or a large lake if transplanted. They live off of their body fat for a year or longer. Marlene Lorgen, Elisa Casadei, Elżbieta Król, Alex Douglas, Mike J. Birnie, Lars O.E. Steelhead and Kokanee are a couple of great examples of two different varieties of salmon that can live in both saltwater and freshwater. Atlantic salmon do not require saltwater. They found out that chronic stress can be a contributing factor preventing salmon from finding their way back to their rivers. Go. Atlantic, coho, and chinook salmon are the best-known anadromous fish. Salmon are born in freshwater, and have hyperosmotic body fluids -- they take in freshwater through the gills and excrete waste as urea. These tiny babies are called 'alevins' and they live in amongst the gravel on the stream's bed. Coho, Chinook and Kokanee (Pink) Salmon are readily available on the Lakes, and they are an amazing treat. That optimum level happens to be much less saline than seawater but a lot more saline than freshwater. The only North American one that doesn't is the Lake Trout. ... To ensure smooth game play, walk the students through the roles and rules of the game to ensure that each knows what to do and where to go before you start. Diet. Have any problems using the site? The recent work is a collaboration together with Senior Researchers Tom Ole Nilsen and Sigurd Handeland from his group, Professors David Hazlerigg from the University of Tromsø and Sam Martin at the University of Aberdeen. Therefore, the problems a salmon must deal with in fresh water environments are salt loss and water loading. Second, the kidneys have to drop their urine production dramatically. First, it must start drinking a lot of water. Atlantic salmon have a complex life history and go through several stages that affect their behavior, appearance, and habitat needs. The three year project is funded by the Research Council of Norway. Add this to the film's beautiful depictions of their life cycle, navigation, and remarkable sense of smell. As with most molecular machines, the details are, of course, much more complicated. Some fish that live in a saltwater environment, and only live in a saltwater environment, such as tuna, drink the very, very salty seawater. Or view hourly updated newsfeeds in your RSS reader: Keep up to date with the latest news from ScienceDaily via social networks: Tell us what you think of ScienceDaily -- we welcome both positive and negative comments. The research group shall now strive to become a Centre of Excellence in Integrated Fish Neurobiology. Nov 21, 2007 #2 Generally, no. Typically, salmon will hatch in freshwater streams and rivers and move to the oceans over their life, returning to the fresh water to reproduce. The new centre will offer researchers completely new knowledge and tools. 1 American Eel. He has been affiliated with the University of Bergen since he moved to Bergen as a post-doc fellow in 2000. They are anadromous, which means that they are … The key to success lies in the fact that the centre will combine expertise from various fields in neuroscience, functional neuroanatomy, behaviour, molecular biology, bio-informatics, ecology and fish physiology. Uni Research. We hope this brief survey of osmoregulation in the Pacific salmon enhances your appreciation of their multiple design features as shown in Living Waters. When they do come to Alaska, they're here in huge numbers. In salmon, special chloride cells are networked with accessory cells in "a mosaic of interlocked cell processes bound together by an extended, shallow apical junction" (PubMed). The parr remain in the rivers for as long as three years, during which time they continue to grow. In the study, they found that this deiodinase paralog that activates the thyroid hormone in the gills only increases when the fish reaches saltwater. Wikipedia has some simplified diagrams of the pump. But then you have these odd fish called "euryhaline" fish - like salmon, eels and striped bass - and they have to be able to tolerate huge changes in outside salinity, either because of their life-cycle, like the salmon, which goes upstream into freshwater to spawn, or if they live in an environment like an estuary where the river meets the sea. As rainbow trout do not breed in Scotland all rainbow trout fisheries rely on production of rainbow trout from freshwater aquaculture. MERGE CANCEL. For example, freshwater bass and salmon contain more folate and vitamin A than saltwater salmon and bass. notable examples are eels and salmon. "We do not necessarily believe that fish and humans are the same, but mechanisms in the brain occur in a similar way for fish as for humans. Salmon also have to pump out the chloride ions (Cl-) that result from dissolved ocean salt. First they must switch from using saltwater to freshwater. Freshwater fish need salt secreting gills in order to survive in salt water. When to fish for salmon is dictated by when they appear in these different locations.
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