If you're not able to, or simply don't want to read each little news blurb about Porsche Motorsports, there is no better way to stay in touch than by reviewing the monthly Porsche Motorsport Newsletter here on PorschePurist. Filled with interesting facts and figures about past and upcoming races, along with changes to team and crew, the Porsche Motorsport Newsletter is an easy way to keep up-to-date on this year's racing activities within the Porsche community.
The lightning work done on their 911 GT3 RSR in the pits of Flying Lizard Motorsports was the key to the first win of the season for Porsche's Joerg Bergmeister and Patrick Long at round two of the ALMS in Long Beach (17 April). With fresh tires the reigning champions won the fight for GT honors after 100 minutes. Their rivals had only changed drivers. In the LMP class, Klaus Graf and Greg Pickett brought home third with their Muscle Milk Cytosport RS Spyder. Both Porsche cars won the Michelin Green X Challenge environmental award.
Reigning champions Marc Lieb and Richard Lietz crossed the finish line first in their Felbermayr-Proton 911 GT3 RSR at round one of the Le Mans Series in southern France's Le Castellet (11 April). After eight hours, the works drivers held a two-lap advantage over the team's second Porsche, in which works driver Patrick Long together with Martin Ragginger and team owner Christian Ried conquered second.
Successful debut for Austrian Thomas Gruber and Dimitros Deverikos from Greece at the season-opener of the International GT Open on the Circuit Ricardo Tormo near Valencia (17 April). The duo snatched GTS victory at the wheel of the Autorlando Sport 911 GT3 R. In the Super GT class, Patrick Pilet/Raymond Narac yielded second with their IMSA Performance Matmut-911 GT3 RSR from race two (18 April).
The new 911 GT3 R goes from win to win on the world's toughest race track. Round three of the Nürburgring Long Distance Championship (24 April) went to Chris Mamerow and Porsche factory pilot Wolf Henzler with the 911 GT3 R of Mamerow Racing. Timo Bernhard, Romain Dumas and Marcel Tiemann had won the second race (10 April) in Manthey Racing's 911 GT3 R.
The innovative Porsche 911 GT3 R Hybrid continues its success streak. Joerg Bergmeister and Wolf Henzler claimed third at round two of the Nürburgring Long Distance Championship (10 April) piloting the GT with its 480 hp normally aspirated engine and two 60 kW (82 hp) electro-motors at the front axle. Two weeks later, Formula 1 pilot Nico Hülkenberg turned his first laps on the Nordschleife in a Porsche race car – and was taken with both the track and the Porsche 911 GT3 R Hybrid.
Niclas Kentenich and Sebastian Asch won the first race of the 2010 ADAC GT Masters driving an a-workx 911 GT3 R in the Motorsport Arena Oschersleben (10 April). Frank Schmickler/Kevin Estre secured second place in a Mühlner-Porsche 911 GT3 R. Race two went to René Rast/Tim Bergmeister at the wheel of a Mühlner-Porsche 911 GT3 Cup S. GT Masters debutant Rast gave an impressive performance with his slick-shod car on a wet track surface.
A brilliant performance by Autorlando Sport at the start of the season in Misano (24/25 April): Works pilot Patrick Pilet and Gianluca Roda proved unbeatable in the new 911 GT3 R at both GT3 races and brought home overall victory from the first race. Paolo Ruberti and Fabrizio Del Monte secured the GT2 win for Autorlando in the 911 GT3 RSR at race one, finishing second overall behind their team colleagues.
The Belcar Endurance Championship took off into the season on the Circuit Zolder (11 April) with the Porsche 911 GT3 R winning here as well. Starting from second on the grid in a 40-strong field, Marc Goossens and Maxime Soulet won the top GT3 class for Prospeed Competition almost one lap ahead of their rival in second.
The near-standard 911 GT3 Cup encounters purpose-built tubular frame race cars in the GT class of the Grand-Am. Nevertheless, thanks to a clever pit strategy, the long-established TRG squad claimed their first win of the season at race four on the Virginia International Raceway (24 April). Andy Lally shared the cockpit of the TRG-Porsche with Ted Ballou.
With two flag-to-flag wins from pole position at the Carrera Cup Asia race held as support to the Formula 1 Grand Prix in Shanghai (17/18 April), Christian Menzel launched his title defence campaign in the Star Chase 911 GT3 Cup. Porsche Asia Pacific announced a record grid line-up of 23 new 911 GT3 Cup racers.
While Nick Tandy (Konrad Motorsport) brought home his first win at round one of the Carrera Cup Deutschland (25 April) from pole position, a fight for the remaining podium spots raged behind the Briton. After 18 laps on the Hockenheimring, Niclas Kentenich clinched second starting from sixth, with Martin Ragginger ploughing his way through from ninth on the grid to claim the last podium step.
Seasoned racer Tim Harvey achieved four straight wins on the high-speed circuit of Thruxton (3/4 April) and in Rockingham (24/25 April) for Red Line Racing. But it was 23-year-old newcomer Euan Hankey who made headlines at his Porsche debut in Thruxton with positions three and two.
At the season-opener of the Carrera Cup Japan in Okayama (3/4 April) the reigning champion fulfilled all expectations: Y. Shimizu won both races. But, like in England, he also had a rookie hot on his bumper: H. Yasuoka was the sole competitor to match the champion's pace to secure second place twice.
Three wins on the Symmons Plains Raceway in Tasmania (10/11 Apr) catapulted reigning champion Matt Kingsley from zero points to the top of the table. After an accident he had left round one in Bathurst without any points. Kingsley's leap into the lead is an exact repeat of his 2009 season-opening.
Ex-Formula 1 driver Ricardo Rosset wins at his debut in the GT3 Cup Challenge Brasil in Jacarepaguá, with race two going to Clemente Lunardi (17/18 April). Alexandre Barros is the new points' leader with two second places.
Ludovic Badey and Kevin Estre are victors of the Carrera Cup France in Nogaro (4/5 April).
What's the True Price of Deferring Service on Your Porsche?


Children born in South Africa need to understand their RIGHTS.
Please note as per the "BILL OF RIGHTS" of the Constitution of the Republic of South Africa you as a Child are protected.
(2) A child's best interests are of paramount importance in every matter concerning the child.
(3) In this section "child" means a person under the age of 18 years.
Our mandate from GOD is to take care of all HIS CHILDREN and at u21church we will do that community by community as GOD guides us.


text:
Calculation of the dependence of the centrifugal constants of the molecule H2O on the quantum number v2 on the basis of the Morse oscillator
V. I. Starikov, Vl G. Tyuterev
An explanation is given in this paper for the anomalous dependence of the centrifugal distortion in flexible molecules of the type H2O on the "bending" quantum number v2 on the basis of the Morse oscillator. A computation of the dependence of the rapidly varying rotational, quartic, sextic constants of the molecule H2O on v2 describes the experimental behavior of these constants well.
Soviet Physics Journal
Опубликовано - авг 1982
quantum numbers
Starikov, V. I., & Tyuterev, V. G. (1982). Calculation of the dependence of the centrifugal constants of the molecule H2O on the quantum number v2 on the basis of the Morse oscillator. Soviet Physics Journal, 25(8), 762-765. https://doi.org/10.1007/BF00895258
Calculation of the dependence of the centrifugal constants of the molecule H2O on the quantum number v2 on the basis of the Morse oscillator. / Starikov, V. I.; Tyuterev, Vl G.
В: Soviet Physics Journal, Том 25, № 8, 08.1982, стр. 762-765.
Starikov, VI & Tyuterev, VG 1982, 'Calculation of the dependence of the centrifugal constants of the molecule H2O on the quantum number v2 on the basis of the Morse oscillator', Soviet Physics Journal, том. 25, № 8, стр. 762-765. https://doi.org/10.1007/BF00895258
Starikov VI, Tyuterev VG. Calculation of the dependence of the centrifugal constants of the molecule H2O on the quantum number v2 on the basis of the Morse oscillator. Soviet Physics Journal. 1982 Авг.;25(8):762-765. https://doi.org/10.1007/BF00895258
Starikov, V. I. ; Tyuterev, Vl G. / Calculation of the dependence of the centrifugal constants of the molecule H2O on the quantum number v2 on the basis of the Morse oscillator. В: Soviet Physics Journal. 1982 ; Том 25, № 8. стр. 762-765.
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redpajama_set_name: RedPajamaCommonCrawl


Team Meeting #0: Meet Oaklandish Impact!
For today's session, our group went through the Workshop Guide for Class 1 of the course. We started off the workshop with a brief exercise to introduce ourselves to the group, what we're currently working on and what we'd like to learn during the course. We then proceeded to play an Icebreaker called Visual Telephone to get our creative juices flowing. We each start by writing a phrase (silly or serious) on the top of a sheet of paper. The paper is passed to the person on the right and that person tries to draw the phrase, and this alternates until the sheet of paper comes back to the original owner. My phrase "Bears like to eat cupcakes" pretty much stayed the same throughout. However, I did learn that glitter is pretty difficult to draw on paper, as it ended up being mistaken for nails.
Use of more "I" statements, speak from individual experiences.
After discussing readings from our first class, we got right into the meat of today's workshop: Design a Better Commute! We split the group up into pairs and took turns interviewing to understand each other's morning commutes. Some things to keep in mind for these interviews was to be an active listener and to keep asking "Why?".
My partner, Lina, talked about her morning commutes of having to drive to multiple locations throughout the day. She typically drives because it's most the cost- and time-efficient, but prefers to find free parking as most people would. Sometimes she'll settle for having to pay for parking or parking a little further, and will go through multiple cycles to find parking, but usually won't spend more than 10-15 minutes looking for parking. If public transportation was more accessible, she would much rather prefer that option, but driving to each location to meet her clients currently suits her needs better.
We took the next five minutes to read over our notes and interpret our partner's needs from the interviews.
What are three unique aspects of your partner's commute?
Having to drive to multiple locations throughout the day.
Determined to find free parking.
Would use public transporation if more accessible.
What are three needs that your partner faces each month?
Get to meetings on time.
Have everything packed for the day.
For this section, we took fifteen minutes to brainstorm new solutions to improve our partner's commute. Some of my ideas for Lina included an app that helps you find free parking, co-sharing parking spaces, more locations on public transportation systems like BART and Muni, Clipper Card with unlimited monthly passes for the entire Bay Area, and parking garages.
It's time to get tangible! We worked on more physical/visual prototypes to imagine the possibilities and pitfalls of our solutions. I decided to go further with my free parking app idea, and started to draw out the visuals of my app.
After prototyping, we finally shared our ideas with the rest of the team.
Lina's idea for a driving co-op to solve the issue of having to drive to work everyday.
Chris' idea for Annie's request for the best bicycle ever!
Annie-Rose's idea for Chris' problem of commuting across different public transportation systems with a bike, including a work station for Caltrain!
Class 1 complete! See ya next week!


As a Senior Search Consultant Rob focuses on building lasting relationships with information technology professionals by enabling and enhancing their career prospects, providing market intelligence, and arranging well thought out introductions and interviews. He tailors a custom process to every one of his clients to bring information technology professionals the very best opportunities and hiring authorities the very best talent.
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text:
AdventureEnvironment
Why is 17-Year-Old Alec Loorz Suing the Government Over Global Warming?
Last May, while most normal high school students were out breaking curfew or killing time until summer, 17-year-old Alec Loorz from Oak View, California, had other plans: He was suing the federal government for global warming.
His lawsuit is part of a nationwide surge of youth-led litigation, filed in every state, arguing that the atmosphere is part of the public trust and that the government has an ethical responsibility to protect it for present and future generations. It's a bold move, especially since the so-called Public Trust Doctrine has never been used to protect something as invisible and intangible as the air we breathe and the atmosphere we live in. And never by plaintiffs who are too young to vote.
"The kids living today are the ones who have the most to lose," says Julia Olson, executive program director for Our Children's Trust, a nonprofit that's helping spearhead the iMatter legal campaign in partnership with Alec's organization, Kids Vs. Global Warming, and is releasing mini documentaries each month about the youth plaintiffs to raise awareness of the eco blitz. The federal case seeks to compel agencies to adopt a climate recovery plan by capping carbon emissions by 2012 and then reducing them by 6 percent a year starting in 2013, to put us on a trajectory to reach 350 parts per million of carbon dioxide in the atmosphere by 2100. "This is the minimum that Jim Hansen and other climate scientists say we need to get to a stable climate," Olson says.
While some of the petitions and lawsuits have been rejected and others await their day in court, Alec's federal suit appears to be on the fast-track—at least for now. A preliminary injunction hearing is scheduled for November 21, at which point the judge may decide to green light climate action immediately rather than let the process drag out. "We don't believe we have time to have the whole case litigated now," says Olson. "Emissions reductions are so urgent."
So urgent, in fact, that it may already be too late for Alec and the other youth climate plaintiffs. Even if a 6 percent recovery plan is implemented in 2013, Alec will be 104 by the time the climate returns to equilibrium. I checked in with the boy wonder of climate activism about taking the really long view.
RR: How'd you get involved in climate change?
AL: Watching "Inconvenient Truth" was the spark for me. Before that, I knew nothing. We barely recycled at home. When I saw the movie, something clicked inside of me. I was 12. The next day at school, I had a heated argument about global warming with my best friend. It made me so angry that I went home and spent hours looking up scientific reports and making a presentation to show my friend the next day. That's when I knew this was something I wanted to fight for.
Then what happened?
I wanted to be trained by Al Gore, but they rejected me. I was too young. Eventually I did get trained, and now I give presentations at schools around the country as part of the organization I started, Kids Vs. Global Warming. I think I've spoken to 250,000 people total so far.
A few weeks ago, The New York Times ran an editorial called "Where Did Global Warming Go?" How do you keep getting the message out given the backlash and naysayers?
Yeah, everyone in the environmental movement is wondering the same thing. Al Gore and his Climate Reality Project just released a new presentation arguing the real science. A lot of people are talking about green jobs instead, but that's avoiding the issue. The answer is going above that. It's bigger than climate change. It's sustainability. It's about living as if our future matters.
Do you get ever overwhelmed by how much there is to do?
That's the biggest thing I've struggled since I went to Iceland two years ago and saw the glaciers melting. The main thing I've figured out is to remember that my generation is being called to solve this crisis. We were born to help our community transition to a sustainable culture. I'm always impressed by what young people can do.
Like file law suits...What made you and your fellow plaintiffs decide to take legal action?
We are all in imminent danger. Scientists have said we have 10 years to make changes if we want to stabilize the climate by 2100—and that was back in 2005. We've already wasted five years. Climate change is a symptom of corruption and unsustainable mindset. We care more about money and power than we do about future generations. The judicial system is the only branch of government not bought out by corporate interests.
How does the public trust work?
The government has a legal responsibility to protect the atmospheres for future generations, and we have authority to take legal action against the government for not protecting this trust. It's like your dad gambling away your college fund. Young people can't vote. We have no official political recognition. All we can do is trust. Government has allowed money and power to come before our future. The courts have the ability to protect that trust.
Are you optimistic?
The lawyers are all pretty hopeful. If it goes through, it would be a landmark decision. Even if they try to compromise, at least it's on the table. If it were up to me, though, I wouldn't compromise. Six percent is the bare minimum of what we need. And for each year we don't do anything, that number goes up.
Even if we do get a climate recovery plan, we won't see the benefits of a stable climate within your lifetime. What's it like to realize that you might not be around to reap the benefits of your efforts?
It's kind of weird, but I feel like I'm dedicated to this fight. It's for the future.
What do you do to reduce your carbon footprint?
We recycle and compost, and I ride my bike as much as I can. We got rid of our SUV and have a smaller, more efficient car. We're working on a solar hot water system. And we changed our light bulbs—all that basic energy-saving stuff.
Is it hard to justify all the flying you do?
Yeah, pretty much one flight cancels out any positive action over the past year. I'd love not to travel. I travel about one week a month. I've started home schooling because I travel so much. But if I reach 100 people and they each talk to 10 people, that's 1,000 people. Still, if I were to think, how am I going to solve climate crisis on my own—that's unhealthy. This is an intergenerational issue. The government needs to be the one to make the plan. The scientists say that we still have a chance if we act now .
—Katie Arnold
@RaisingRippers
Filed To: Nature


text:
Are We on the Verge of Discovering an Earth-Like Exoplanet?
Filed under: astronomy,exoplanets,general science,misconceptions,podcast,skepticism,solar system formation,stars — Stuart Robbins @ 6:12 pm
Tags: astronomy, astrophysics, exoplanet, exoplanets, extra-solar planet, general science, misconceptions, podcast, science, skepticism, solar system, solar system formation, star
I announced awhile ago that I was on episode 347 of the Canadian, "The Reality Check" poscast where I talked about exoplanets and some hype — deserved or otherwise — about almost but never quite yet discovering Earth-sized exoplanets.
While they post a lot of links and other things on their website, they don't post transcripts of what we actually talk about. Since I spent a solid many minutes writing and editing my segment's text, I thought I'd post it here:
There's lots of ways to talk about exoplanets, but I'm going to take the traditional approach and start with a very broad but brief overview of how we have found the few-thousand known extra-solar planets, or "exoplanets" for short. There are five main ways.
The most obvious is the most difficult: Direct Imaging. This is where you take your telescope and would look at a star and see the planet around it. This is almost impossible with current technology, and we have less than 20 exoplanets found this way. It's so hard because the star is so bright relative to the planet and because most star systems are so far away. And obviously, if the planet is larger and farther away from the star, it'll be easier to see.
The second main method has also only produced about 20 planets so far: Gravitational Microlensing. Einstein showed that large masses bend light, and we can see this in space when an object that's far away passes behind a massive object that's a lot closer. The light from the background object gets distorted and magnified, much like a lens … a lens caused by gravity. If the foreground object happens to be a star, and that star has a planet, then that planet can make a detectable contribution to the lensing, not only in amount, but in the exact shape of the lensing effect.
The earliest actual successful method was a special form of what's called the Timing Method, specifically in this case, pulsar timing. Pulsars are incredibly dense stars called neutron stars, and we get a blast of radio waves every time one of its poles sweeps in the direction of Earth. These are so regular that any tiny perturbation can be detected and attributed to something weird, like a tiny planet tugging on it and so changing that regular spinning signal.
This is the same concept as the highly successful method that found the most exoplanets until a few years ago: Radial Velocity. The idea is that we normally think of a planet, like Earth, orbiting the sun. But it doesn't really. It *and* the sun orbit a mutual gravitational point called the "barycenter" that is between the two. For Earth and the sun, that point is VERY close to the sun's center, but it's not quite in the center. That means that over the course of a year, as Earth goes around that point, the sun will, too (on the opposite side of that point). So, it will wobble very very slightly as it orbits the barycenter.
We can't possibly observe this tiny tiny motion of other stars. BUT, we can use the light that star emits to do it by using the Doppler shift. That's the phenomenon where if something is moving towards you, the waves it emits become compressed, and if it's moving away from you, the waves get stretched out. The common example is a train whistle going from high to low pitch, but in astronomy, this is where the light is shifted to blue and then to red.
So, if the planet around another star is at its closest point to us, the star emits light and we see it all normal. As the planet starts to move away from us, the star starts to move very slightly toward Earth, and so its light will be very slightly blue-shifted. Then, the planet gets to its farthest point, and starts to move towards Earth, which means the star starts to move away, and we see its light red-shifted. This is an incredibly tiny effect, and the smaller the planet, the smaller the shift in the light. Or the pulsar timing change.
There was a lot of progress throughout the late 1990s and early 2000s in very high-resolution spectroscopy in order to get better and better at observing smaller and smaller planets. The easiest ones to observe are the largest because they make the biggest shift in the star's light, and ones that are closest to their star are easier because you don't have to observe as long. To observe a planet that has a 10-day orbit, you just have to observe that star for about a month from Earth to get decent statistics.
That's why all the exoplanets discovered early on were what are called "Hot Jupiters," since they were very large and very close to their stars.
The final method is the Transit Method. If a fly passes in front of a bright light, you can see a slight decrease in the light. If a bird passes in front of a light, you'll see a larger decrease in the light. Same thing here: A planet passes in front of the star and temporarily blocks part of the light from the star that we would see at Earth. The big issue with this method is that you have to have the fortuitous geometry alignment where the planet's orbit is just right so that it passes in front of its star as seen from Earth. The first one wasn't detected until 1999, but a decade later, the dedicated spacecraft COROT and then Kepler were launched to look for these, monitoring the same fields of the sky, tens of thousands of stars, moment after moment, looking for those brief transits. In 2014, Kepler released over 800 planets discovered with this method, more than doubling the total number known, and that was on top of its other releases and, to-date, it's found over 1000.
The transit method, despite the issue of geometry, is probably the best initial method. If you have the planet going in front of its star, then you know its alignment and you can follow-up with the radial velocity method and get the mass. Otherwise, the radial velocity method can only give you a minimum mass because you don't know how the system is oriented, you only know that radial component of velocity, hence its name.
With the transit method, you can see how much light is blocked by the planet. Knowing the star's type, you can get a pretty good estimate for the star's size, and knowing how much light is blocked means you can get the cross-sectional area of the planet and hence its diameter. For example, Jupiter would block 1% of the sun's light, and since area is the square of length, that means Jupiter is about 10% the sun's diameter. Since the sun is a type G V star, we have a good model for its radius, though of course we know its radius very well because we're in orbit of it. But that means not only can we get mass, but we can get size and density.
The transit method also lets us see if there's a large atmosphere. If the light from the star instantly blinks down to the level when the planet passes in front of it, then any atmosphere really thin or nonexistent. If there's a gradual decrease, then it's extended. If its extended, we can follow-up with something like the Hubble Space Telescope and actually figure out what that atmosphere is made of by looking at what colors of light from the star are absorbed as it passes through the planet's atmosphere.
And as with the radial velocity and timing methods, we know how long it takes to go around its parent star, and along with the star's mass from what kind of star it is, we can get the distance of the planet from the star.
Okay, so much for a brief overview. But for me, I've left out a lot.
Moving on, it should be somewhat apparent that the bigger the planet, and the closer to its star, the easier it is to observe with pretty much ANY of these techniques, except direct imaging or microlensing where you want a big planet that's far from its star. Big means big effect. Fast orbit means you don't have to observe it for very long to show that it's a regular, repeating signal best explained by a planet.
So, the question is then, can we detect an Earth-sized planet, and can we detect an Earth-like orbit? These are really two different questions and they depend on the technique you're using. If we want to focus on a the two main methods – radial velocity and transit – then the unsatisfying answer to the second is that we do finally have good enough technology, it is just a matter of finding it. With the 2014 Kepler data release, there were over 100 exoplanets that are less than 1.25 Earth's size. With the 2015 release, there are a total of 5 planets smaller than Earth or Venus, but they orbit their 11.2-billion-year-old star in just 3.6 to 9.7 days.
Even if we have observations for more than a year or two, for something as small as Earth, the level of signal relative to noise in the experiment is still pretty small, and you want a big signal relative to the noise. It's best to build up multiple years' worth of data to average out the noise to be able to really say that we have an Earth-like planet. For something like Jupiter, which orbits our sun in about 12 years, we'd need to observe at least two transits, meaning we're just now approaching the time when we would have a long enough baseline of data with some ground-based surveys, but that's also assuming we catch that planet for the few hours or days when it goes in front of its star versus the years and years that it doesn't, and that we do this repeatedly and don't chalk it up to sunspots.
This is why we really need long-term, dedicated surveys to just stare at the same place in space, constantly, measuring the light output of these stars to see if we can detect any sort of dimming, that's repeated, from a likely planet.
But, even if we find an Earth-like planet in terms of mass and diameter and location in its solar system, that's not enough to say it's Earth-like in terms of atmosphere and surface gravity and overall long-term habitability. It's just a first step. A first step we have yet to truly reach, but one that is reasonably within our grasp at this point.
But it's from the existing planets we know of that we get some of the hype that hits the headlines every few months, like "astronomers estimate billions of Earth-like planets exist in our galaxy alone." I'm not going to say that's fantasy, but it's loosely informed speculation based on extrapolating from a few thousand examples we now have from a very, VERY young field of astronomy.
Or, we'll get articles where the first sentence says, "Astronomers have discovered two new alien worlds a bit larger than Earth circling a nearby star." It's in the next paragraph that we learn that "a bit larger than Earth" means 6.4 and 7.9 times our mass, and they orbit their star in just a few days.
So as always, this is a case where, when we see headlines, we need to be skeptical, NOT susceptible to the hype, and read deeper. But that said, it is entirely possible that any day now we will find an exoplanet that is at least like Earth in mass, size, and distance from its host star.
Podcast #72: Solar System Mysteries "Solved" by PseudoScience, Part 1 – Iapetus
Filed under: astronomy,podcast,saturn,skepticism — Stuart Robbins @ 9:40 pm
Tags: argument from ignorance, astronomy, astrophysics, equatorial ridge, Hoagland, iapetus, mysteries, saturn, scientific skepticism, skepticism, skeptics, solar system, walnut moon, yin-yang moon
Exploding planets,
Alien spaceships … Why is
Iapetus weird?
The subject of this episode is Saturn's moon, Iapetus, and two mysteries about it that various branches of pseudoscience have claimed to solve: the brightness dichotomy via an exploded planet, and the equatorial ridge via a spaceship.
This is the first of what I plan to be a series much like "The Fake Story of Planet X" series — different mysteries of the solar system that have a pseudoscientific explanation and may or may not have a real science (agreed upon) explanation. Let me know what you think of the concept. Future ideas for shows are the Pioneer Anomaly and Mars' crustal dichotomy.
Otherwise, there's a bit of feedback and then I get into the puzzler from last time and one announcement.
Well, I sorta snuck in a second announcement — I'm headed to Australia, December 18 – January 20. I'll be centered in Melbourne (which I enjoy pronouncing as "Mel-born-EE") for most of the trip though should make it up to Sydney (I wanna see the Great Barrier Reef!). So, dinner in each city if I can round up enough interest. I'm slowly learning that Australia is not just a 5-hr drive across, so I'm less likely to make it to the eastern half. We'll see if I can increase my Australian listenership in the meantime to make a dinner here or there worth organizing.
Podcast Episode 61: Special Pleading with Large Impacts
Filed under: asteroids,astronomy,logical fallacy,podcast — Stuart Robbins @ 5:03 pm
Tags: astronomy, astrophysics, giant impact, impact crater, logical fallacies, logical fallacy, mercury, moon, solar system, solar system formation, special pleading, uranus, venus
A complaint I've heard is that the invoking of giant asteroid impacts to explain some odd solar system features (Venus upside-down, Uranus on its side, etc.) is just special pleading and as crazy if not more so than the pseudoscience ideas, like Velikovsky. While I obviously have my own opinion about Velikovsky in particular, I wanted to take an episode to talk about why giant impacts are used to explain some things, and whether we have a real reason to do so or if it's just our own way of making stuff up.
There isn't a new puzzler, though the one from last episode – send in your favorite planetary pareidolia – is still going on.
Some Boring New Results Show We're Still Not Going to Cross the Galaxy In December 2012
Filed under: astronomy — Stuart Robbins @ 11:22 pm
Tags: 2012, 2012 doomsday, 2012 galactic alignment, astronomy, doomsday, galactic alignment, IBEX, solar system, solar system motion through the galaxy
Many œons ago, I wrote about how we're not going to cross the galaxy's equator in 2012. It's one of those ideas about a physical galactic alignment that some people believe – we're really actually physically going to cross the equator/plane of the galaxy in December 2012 (or a window around that date) and bad stuff is going to happen as a result.
I explained in that post that, no, we're not. The latest data I had on-hand is:
[The sun] is about 35-70 light-years "above" it (since there's no "up" in space, you could also say it lies below it). It is also currently still traveling "upwards" in the direction of the North Galactic Pole at a rate of 7-8 km/sec.
It is also not on a perfectly circular orbit relative to the plane of the galaxy, moving presently inward at a rate of 10-11 km/sec. Its rotational velocity around the center of the galaxy is about 200 km/sec.
New research announced this past week changes that.
We're Still Okay
The new research comes from a Science paper by McComas et al. entitled, "The Heliosphere's Interstellar Interaction: No Bow Shock."
Without getting too much into the nitty-gritty details, the article talks about new observations by the Interstellar Boundary Explorer spacecraft, also known as IBEX. The craft has been observing neutral atoms – meaning that they have no net electric charge – to understand the environment of the galaxy that the solar system is moving through.
The new result from this article that's relevant to 2012 doomsday stuff is that the latest results from IBEX have revised the speed with which we thought the solar system was moving through the galaxy. We thought the sun was moving through the interstellar neighborhood at around 26 km/sec, but that value has now been revised downward to about 23 km/sec, or by around 11%.
NEW NASA DATA FROM NASA SCIENTISTS SEZ WE'RE ALL GONNA DIE!!!!!
Okay, but seriously folks, this is not a huge huge deal in terms of this upsets everything we thought we knew about the universe. This is how science works. New data comes in that has incrementally increased our understanding of something. We're still far from the plane of the galaxy, we're still moving away from the plane of the galaxy, just we're moving a little more slowly.
As in, we're not moving more quickly in the other direction towards the galactic plane so that we pass through it in seven months.
That's about all I have to say on this one. I found the paper a bit interesting and since it remotely applied to something that I'd discussed before, thought I'd share.
And it lets me muse about how people will use old data to support their pseudoscientific ideas and NOT revise them when new data comes out that differs (remember how 2012, back in 2004, was supposed to be a huge, ginormous, deadly solar max — something that's still repeated often?).
Which incidentally leads me to mention that I'm going to start a new segment with the next episode of my podcast, a "new news relevant to previous episodes." This'll be one of those news items on the May 16th episode.


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Deb's eyes show her so many things in the world that need to be captured in a photograph, so that they can be looked at more closely, be appreciated, and cherished – so many beautiful, wonderful, interesting, and unusual things. It is these things that she points her camera lens at: wide, sweeping vistas; the smallest details in a flower; subtle patterns of light and shadow; intricate reflections on water. She invites you to see some of the things that have caught her eye, her heart, and her spirit, and have been captured by her camera. Her hope is that you will find these things as captivating as she has.
I truly find inspiration everywhere! For me, the key is to quiet my mind and really see / feel / hear / smell / taste all that is around me. When I can do that, I am constantly amazed at what I find.
I like to go hiking at various places in and around Eugene: the entire Ridgeline Trail system, Fern Ridge Reservoir and all of the wetlands between town and Fern Ridge. I also love to go to the coast, up the McKenzie River, and into Central Oregon.
All images appearing on this website are copyright of Deb Ingebretsen. No image from this site may be reproduced in any form without specific written permission and to do so without such permission is an unlawful act which may result in legal action.
Deb believes she's been a photographer most of her life, starting when her parents gave her a Kodak Hawkeye Instamatic camera when she was around 9. She took photography courses in high school, where she was introduced to a SLR camera and the darkroom. From there, she photographed off-and-on, in between all the activities that fill a person's life. In 1999, she began to rediscover her passion for photography, and in early 2005 she quit her job and move to Missoula, Montana for five months to attend Rocky Mountain School of Photography's career training program.
Since then, she's made photography, creativity, and artistic expression a priority in her life, and something that she wants to celebrate and share with others.


Explore your practice deeper, learn to modify postures for your body, go further faster with hands on assists. These are just a few of the benefits you'll receive when you have your own private yoga teacher. Each session can be tailored to suit your physical or spiritual goals.


Having a crazy beard is one way of getting girls to notice you!
How to play the game "The Barber Shop Game"?
What Carl is yet to learn is that styling a beard can be lots of fun! You could just shave it all off, but why not try lots of different styles and shapes first? That's what we would do it we were a boy! You could leave a moustache, a goatee or serious sideburns. Just see what looks the silliest! Do you think it would be fun to work in a barber shop?
The Barber Shop is one of my favorites! We clearly have awesome taste! Come and play more of my fave hair games!


Thanks for visiting our Park Royal handyman website, we are specialists in house improvement and home repairs and maintenance in the Park Royal Greater London (Brent) W3 0 London area.
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.Our handymen are trained and qualified in numerous trades, including joinery, pipework, electrical, roofing, masonry, landscaping, just to mention a couple. On top of that, they are disciplined, well-disposed, and educated when it comes to health and safety, asbestos awareness, and manual handling. You can, for that reason, trust us to deal with practically any job within our field in an expert and acceptable way.
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Holyrood Palace and Gardens Private TourAlexander Alexander2019-11-25T21:27:00+00:00
Scotland/
Holyrood Palace and Gardens Private Tour/
Holyrood Palace and Gardens
Officially known as the Palace of Holyroodhouse,this is the Queen's residence when in Scotland. 'Holyrood Week' normally falls about the first week of July, during which the monarch attends parades, holds audiences and hosts a royal garden party for about 8000 people from all walks of life.
Originally this site housed a small abbey founded in 1128 by King David I, to which many buildings and later some royal lodgings were added. In 1430, James II was the first king to be born at Holyrood, and James III was married there. During his reign (1488-1513), James IV was a frequent visitor and in 1503 he built the first royal palace here as a home for his new bride, Margaret Tudor. Mary, Queen of Scots lived here from 1561 after her return from France, and here she married her two Scottish husbands in turn. Her chambers and the Darnley rooms are a highlight of any visit.
James VI lived at the palace from 1579 with a household of about 600 people. He carried out extensive repairs, but after he was crowned as James I of England he moved his court to London. Except briefly for Bonnie Prince Charlie, later Stewarts showed little interest in the palace.
Much later, Queen Victoria was a frequent visitor and during her reign (1837-1901) there was extensive renovation. After World War 1, major improvements were made to the State Apartments and Throne Room under King George V.
The gardens are extensive (10 acres/4 hectares) and full of historical interest. It was here that Mary, Queen of Scots practiced hawking, wild boar hunting, tennis and archery. Archery is still practised three times weekly in the gardens by the Royal Company of Archers who form the royal bodyguard in Scotland. The 'Royal ticket' allows visitors to combine visits to the palace, gardens and Queen's Gallery (with changing exhibitions).
Palace of Holyroodhouse
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www.rct.uk
Open annually except Christmas Day (25th December) and Boxing Day (26th December)
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Cook hash browns according to package directions; crumble and keep warm. Meanwhile, in a large bowl, whisk the eggs, chili powder, garlic and cumin. Set aside.
In a large skillet, cook the chorizo, jalapenos, peppers and onions over medium heat until meat is no longer pink, drain. Add reserved egg mixture; cook and stir over medium heat until eggs re set. Stir in salsa.
Spoon 1/2 cup hash browns and 1/2 cup egg mixture off center on each tortilla, sprinkle with 1/3 cup cheese. Fold sides and ends over filling and roll up. Wrap each burrito in waxed paper and foil. Serve warm with sour cream if desired. Cool remaining burritos to room temperature; freeze for up to 1 month.
To use frozen burritos; Remove foil and waxed paper. Place burritos 2 inches apart on an ungreased baking sheet. Bake uncovered at 350 degrees for 50 to 55 minutes or until heated through.


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Actis Asks: COVID-19 Survey 2.0
14 May 2021 Ed Williams, David Kunzmann,
Actis surveyed the senior leadership of its portfolio companies and its own professionals in early April 2020 to understand what was top-of-mind regarding COVID-19. A year on, we have re-run the survey to see how perspectives have changed.
In our survey last April, we had 113 respondents. This year's survey had 178 respondents. Any direct comparisons against data from last year are made with the caveat that the survey population is different.
One year ago, our survey indicated that while concern levels were growing, more than half (51%) of respondents were either neutral or not concerned about the impact of COVID-19 on their businesses. Since then of course, COVID-19 has caused nearly three million deaths and infected many hundred million people globally. Official case numbers are passing through 140 million as we write, but public health experts put the real toll at several times that level.
One year ago, many were describing the threat as "confined to China"; and yet while North America and Europe have accounted for more than half the global death toll, China has reported just 4,841 deaths at the time of writing. Latin America alone has recorded over 850,000 deaths.
Governments and leaders have taken different approaches to managing the virus, some imposing strict regional and national lockdowns, others dismissing it outright.
President Trump famously described the virus as "a hoax" and prompted widespread condemnation for suggesting that injecting detergent into the body could kill the virus; meanwhile, the late President Magufuli of Tanzania denied the virus posed any threat and insisted that inhaling steam and eating potatoes could cure COVID-19. By contrast, Australasian leaders adopted stringent lockdown measures early on and have seen very limited case numbers.
Ignoring or dismissing COVID-19 has to date not proved to be a roaring success.
Vaccines have arrived in record time, but at the same time new variants have arrived and spread, causing second and third waves around the world. Countries and politicians are racing against the virus – and each other – to vaccinate their populations in an effort to bring an end to the pandemic.
But how long will it take? When will it end? And how will life be different post-pandemic? Our survey sheds some light.
As the enormous task of vaccinating the world gathers pace there are, as ever, political and human barriers to overcome. As this survey highlights, there are stark differences in behaviour, approach and opinion around our markets.
Understanding these issues is hugely beneficial to Actis and our portfolio company management teams as we navigate the pandemic, sharing and learning as we go. Wellbeing is a major challenge and while financial statements may be signalling resilience, a wellbeing deficit may take longer to address.
The authors are both members of the Actis Value Creation Group (VCG), which brings professional expertise and works alongside management teams and Actis' investment professionals to maximize the value of our portfolio companies. It identifies areas of improvement for each business and is involved from the pre-investment and due diligence stages right through portfolio management and exit.
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The European Financial Management Association will hold its 28th Annual Meeting at the University of Azores, ISLAND OF S. MIGUEL, PORTUGAL, June 26-29, 2019.
SUBMISSION DEADLINE: January 15, 2019. Papers will be blind reviewed and authors will be notified by March 4, 2019.


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The New Kadimi Banquet Hall located in Rajouri Garden, Delhi has Banquet Halls. Hall can accommodate upto 100 guests in seating and 150 guests in floating.
Vegetarian food is served at this venue. Features of this wedding venues are : Food provided by the venue , Halls are air Conditioned , Decor provided by the venue , Packages starts at Rs 750 per plate for vegetarian menu and at Rs N/A for non veg menu.


An understanding of how and why designing complex interactive systems is difficult. Ideal audience members will be people involved in the design and implementation of hardware+software products.
This presentation will be jointly by Dr. Cory Kidd (CEO, Catalia Health) and Erica Yamada (director of UX, Catalia Health).
Catalia Health is currently the IDEO Startup in Residence, where we are working to create the next generation of interactive robotic interfaces for improving long-term patient engagement. Building on over a decade of work in proving the efficacy of this type of technology, we are bringing a new system to market in 2015 to help our customers better help their patients to manage chronic diseases. Catalia Health has customers ranging from specialty pharmacies to home health agencies to hospital systems, that will be using the hardware+software system to improve interaction with patients managing a variety of long-term conditions.
This talk will describe the design process of building an integrated hardware+software solution to focus on particular customer and end-user needs. In collaboration with the design firm IDEO and borrowing heavily from their user-centered design practices, our team has designed, tested, and implemented a system for creating engaging interactions with patients over extended periods of time.
Examples of the design criteria and constraints will be presented, along with snapshots of the process and challenges that were addressed along the way. Design inputs come from our background research in part, but largely from spending time with our customers and their patients in real-world settings. Our stories and presentation will be designed to highlight how to do this real-world research and turn the findings into components of an integrated product.
Cory and Erica will jointly present the talk with their respective views on the work. Erica is an expert in healthcare UX, coming from the Kaiser Permanente Center for Innovation before joining Catalia Health. She has extensive experience working with patients and healthcare professionals in a variety of settings, ranging from the operating theatre to the clinic to the home. Cory is a serial entrepreneur with nearly two decades of experience in healthcare technology. He completed a Ph.D. in the MIT Media Lab while working jointly at Boston University Medical Center, where he focused on applying interactive robots to the challenges of long-term behavior change.
Dr. Cory Kidd is the founder and CEO of Catalia Health, a healthcare technology company focused on delivering effective behavior change. Cory is a serial entrepreneur who has been working in healthcare technology for nearly two decades. His previous company, Intuitive Automata, created interactive coaches for weight loss. Prior to this, Cory received his M.S. and Ph.D. at the MIT Media Lab in human-robot interaction. While there, he conducted studies that showed the advantages of using a physical robot over screen-based interactions. Cory conducted an extensive study showing the efficacy of his weight loss coach in helping people to diet, and did work in local nursing homes with robotic companions for elderly individuals. He also received his BS in computer science at the Georgia Institute of Technology. While there Cory was a part of the Aware Home Research Initiative, a focused research effort that was looking for ways to allow older people to live in their homes longer.


Special Issue "Linked Data and Knowledge Graphs in Large Organisations"
Knowledge graphs are large networks of entities, their semantic types, properties, and the relationships that interrelate such entities over various topical domains. Through the explicit representation of knowledge in well-formed ways, knowledge graphs provide expressive and actionable descriptions of the domain of interest and support logical explanations of reasoning outcomes based on the context of an entity according to the graph.
Knowledge graphs have proved to be a powerful technology across different areas of artificial intelligence, including e.g. natural language processing and the semantic web, and have been adopted by industry for different purposes, including semantic search, automated fraud detection, intelligent chatbots, advanced drug discovery, dynamic risk analysis, content-based recommendation and knowledge management systems, to name but a few. It is no surprise that knowledge graphs were featured in Gartner's 2018 Hype Cycle as one of the emerging technologies in AI.
However, despite the success of public knowledge graphs, like DBpedia or Wikidata, or corporate ones, like Google's KG, knowledge graphs still face important challenges for widespread adoption by large and medium enterprises, which involve not only technical aspects but also social ones. Among them, we highlight: i) addressing coverage, freshness and correctness at a scale of billions of entities and assertions; ii) Identity management, linkage and entity unification ("are these two products the same?"); iii) interoperability and distributed ownership (80% of enterprise knowledge is locked in silos); iv) change and long-term evolution; and v) sharing and reuse of common parts of knowledge graphs amongst organizations.
We invite authors to submit original articles addressing these and other challenges related to knowledge graphs. To this purpose we offer four different types of submissions: i) research papers, including reproducible experiments; ii) reports from the trenches, i.e. in-use experiences, challenges and lessons learnt; iii) survey papers; and iv) blue sky ideas. While the first three are full-length papers of 30 pages max, submissions of the latter type must not exceed 12 pages.
For illustrative purposes, below we provide a list of possible topics, which are neither exhaustive nor mutually exclusive. We particularly welcome interdisciplinary research over multiple topics, as reflected by our Guest Editorial Board, which includes members from both academia and industry.


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Dr. Iraj Zandi: Appalled By Delay
by Tracy Weber
July 11, 2009, 5:29 a.m. EDT
In the midst of delicate eyelid surgery in April 2006, a patient who was supposed to be sedated yelled that the drugs weren't working.
Plastic surgeon Iraj Zandi turned to nurse Jennifer Bales: "Are you sure you gave me Demerol? Show me the bottle!"
Later, staffers checking the Fremont surgery center's drug locker found hairline cracks around the tops of vials of the painkiller. Bales, they later learned, had removed the drugs in all but two of the vials, then refilled them with saline, Zandi said. Any nurse would know the consequences for a patient: pain during surgery and possibly serious infection from unsterile saline, he said.
Zandi alerted police and reported Bales to California's Board of Registered Nursing. "They said, 'We can't stop her until we go through the process,' " he recalled. It was a frightening thought, he said: She could go to work anywhere.
Over months, Zandi and his staff relentlessly pushed for Bales' criminal conviction. In December 2006, Bales was found guilty of embezzlement for stealing drugs and hypodermic needles.
But it would be another year before the nursing board filed an accusation. The board's documents told Zandi something he hadn't known -- that several years before, Bales had allegedly pilfered drugs from a hospital. Bales failed to respond to the board's accusation, and her license was revoked in 2008.
Zandi's wife, Mitra Ara, who works at the practice, said she couldn't believe the board didn't act faster. "Somebody who takes away a painkiller from patients is capable of doing anything."
Tracy Weber
Tracy Weber is a senior editor at ProPublica. Previously, Weber was a senior reporter covering health care issues at ProPublica and, before that, she reported for the Los Angeles Times, the Los Angeles Herald Examiner and the Orange County Register.
@tracyweber


You are on your first date with someone who you really, really like, but you have no clue if he feels the same towards you. During this time, you want to have the ability to read minds so that you would be able to find out if he is into you just as you are into him. Always remember that the first date is like a make-or-break deal – either you will both discover enough common interests that could lead into the second date, or you will both realize that you are not compatible and bid your chances of a happy ever after (with him) goodbye.
I am sure that all of us are familiar with the adage "actions speak louder than words." The way his body gears towards (or repels away from) you is the easiest method to find out if your date is into you. If you find your date always leaning towards you, or if he does not move his knees away when yours accidentally touch his, then you know for sure that he likes you. Constantly looking at everything but you or moving his seat a few feet away from yours should always be taken as not-so good signs. Be observant.
A guy who does not find it difficult to open up to you is a sign that he is comfortable with you and that he can be himself in your company. Needless to say, this means that he really likes you and that he trusts you. If he really enjoys your company, he would not have a hard time talking to you about anything you could possibly talk about.
If your date likes you back, then he will subconsciously copy your movements. This just means that your guy is mindful of your every move and that he is curious to know how it feels to have his hands (and lips) around you every time you touch a part of your body, or lick your lips after a wonderful meal. Copying your movements also means that he wants his body to be attuned to yours and feel the connection between the two of you.
Here is where he is only aware of one thing: you. Everything else around him just comes in a blur. It is like you are the only person in existence, and you his world. The way he looks at you is also a giveaway to see if he likes you – his eyes are fixed intently on you, as if he is memorizing every pore, every inch of your face. He hardly pays attention to anyone else, be it that statuesque model-lookalike on the other table or if he spills a little water on his shirt just because his eyes are busy ogling at you.
As your first date comes to a close, see if he is in any hurry to say goodbye. Check during the ride home if he is constantly sending text messages, as if he is making other plans after dropping you off. Notice if the ride home is taking longer than usual (if it is, then it means that he is taking his time and just wants to spend more time with you). It is also a good sign if he keeps on putting off any plans to go home and frequently asking if you want to do anything else after your date, like to eat some dessert or grab a cup of coffee, or if he wants to stroll down the park and enjoy the "weather". If you catch him lingering even as you walk away, and makes sure that you are safely inside your home (or sometimes in your room), then you know for sure that he is into you.
More than anything, it is during the first date that you should pay much attention to. It is when you find out if you are compatible with each other that there is a bigger chance of having another date, or if you have absolutely nothing in common that spend one minute more with her is just a waste of both your time. More than a hard subject in school, chemistry is a very important component that should be present between two people on their first date, as it determines the likelihood of a lasting relationship.


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KHON KAEN, Thailand -- The Thai general election on March 24 will be the first since the widespread use of social media in the country and could yield clues to how these new ways of information dissemination affect the fortunes of political parties.
One of the parties that has seized on social media to promote itself is the Future Forward Party, led by Thanathorn Juangroongruangkit, a young billionaire who made his money in manufacturing auto parts. Hashtags related to him and his party dominated Thai Twittersphere after the political neophyte performed impressively during a recent public debate on party policies, pitting himself against pro-junta groups.
"Young voters get all their political information through smartphones, and they are attracted to Thanathorn's party because they can identify with its views that challenge the established system," Supinya Klangnarong, a former member of the National Broadcasting and Telecommunications Commission, the county's independent regulator, told the Nikkei Asian Review.
The easy access to social media platforms such as Line, Facebook, Twitter and Instagram has silenced the airwaves. Thailand's garrulous community radio stations were once a key information channel for political parties and played a crucial role during the last, successful general elections in 2011. Digital media surveys by international and local groups estimate that Thailand has 51 million social media users, of whom 41 million use Line and 49 million Facebook.
It was because of the reach of social media that a small party such as Future Forward is able to gain momentum and rattle the pro-junta Palang Pracharath party, which is backing Prime Minister Prayuth Chan-ocha for another term.
The regime's allies have hit back on social media, targeting Future Forward and parties affiliated with former Prime Ministers Thaksin and Yingluck Shinawatra who pose a genuine threat to the military.
Such campaigns on social media reach beyond the urban youth.
Cherdchai Tantisiri, a heart surgeon and former parliamentarian allied with the Thaksin camps, said that the pro-democracy group has been mapping out the reach of smartphones in Khon Kaen, one of the largest provinces in the northeast, and adjoining five provinces. "I was in a village last week and first asked people at a meeting who has smartphones, and all raised their hands," said Cherdchai recently from his Khon Kaen office.
"We have set up Line groups and networks in 2,500 villages across Khon Kaen," he added. "This has become an important network to stay in touch with our base and convey political information."
Cherdchai is a regional leader of a political party aligned with Thaksin, who absconded after he was convicted of corruption. Despite his troubles with the law, Thaksin remains a patriarch of the country's most influential political camp, which has won all elections since 2001. He was overthrown in a 2006 coup and is reviled by the military and the ultraconservative political establishment.
Seasoned observers said that the pro-democracy camps are tightening their grip in the northeastern provinces through the spread of new technological platforms.
"Social media has been playing a pivotal role to expand the political space and for people to get political information," said Buapun Promphakping, a social scientist at Khon Kaen University. "Nearly 30% of people in the villages in Isaan (as the northeast is known) are connected to Line or other kinds of social media."
Thailand has a 130% mobile phone penetration rate for a population of nearly 69 million. Over 90% of internet users go online via smartphones, according to the National Statistics Office of Thailand.
Thai conglomerates like Charoen Pokphand Group, a business ally of the regime, have played their part in this spread. True Corp., a subsidiary of CP Group and Thailand's largest telecom provider, has teams in villages offering free smartphones and phone lines every month.
Analysts say that the while Line attracts voters of all ages, Facebook is more popular with older voters, while Twitter and Instagram are popular with young, first-time voters, estimated to number about six million out of the over 50 million registered voters.
Back in Khon Kaen, the regional leader of Palang Pracharath is playing down the significance of social media in swaying voter sentiment. "We are not using social media, but going to meet people in person," Ekkarat Changlao said in his party's provincial headquarters. "Under the new election rules, parties cannot do much through smartphones."
The local real estate tycoon has been campaigning over the past seven months on a simple message: "Voting for us is a vote for Prime Minister Prayuth to continue as the prime minister." His face-to-face campaigns, he reckoned, will bear rewards at the polls.


 What does rubber plasticizer have?
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(1) paraffin rubber plasticizer has good oxidation resistance and light stability, but poor compatibility and low temperature. Therefore, in many applications, because paraffin rubber plasticizer has poor compatibility with rubber, it cannot provide good processing performance.
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The company known today as Rausch Funeral Home, P.A. began in 1974 when John O. Rausch and his wife Myrtle purchased, expanded and built their home onto the Buchanan Funeral Home located on Mt. Harmony Lane in Owings, MD. The funeral home business was established in the mid 1800's by Francis William "Mr. Billy" Hutchins, and remained in the Hutchins family name until 1969 when the business was sold to A. Kent Buchanan by William Harry Hutchins, Jr. at the time of his retirement. John's daughter Barbara "Bobbi" Rausch followed her father into the business as a licensed funeral director in the 1970's, and his son-in-law Bill Gross, also a licensed director, came into the business several years later. Rebecca Gross, Bill and Judy's daughter, joined the business as a licensed funeral director in 2009.
In 1989 the Rausch family purchased the Borgwardt Funeral Home in Port Republic from Donald Borgwardt. This facility was originally owned and operated by the Harkness family, and for several years prior by Robert Beall.
In 1992, upon John's retirement, the firm was restructured as Rausch Funeral Home, P.A. and Bobbi, Bill and his wife Judy serve as officers on the Board of Directors.
In February of 2007 the firm opened its third location on H.G. Trueman Road near the former Mill Branch Road intersection in Lusby, MD. This newly constructed facility created, for the first time, a local funeral home in the Lusby/Solomons area that serves the southern part of Calvert County, as well as southwest St. Mary's County.


Use 3 large eggs and one egg white beaten with 1 tablespoon water instead of the egg egg substitute, but you'll increase the SmartPoints value.
Adjust the broiler rack to 5 inches below the heat; preheat the broiler.
Combine the egg substitute, artichoke hearts, mozzarella, pimiento, parsley, salt, and pepper in a bowl; set aside.
Heat the oil in an ovenproof, medium skillet over medium-high heat; add the garlic and cook, stirring, until fragrant, about 30 seconds. Pour in the egg mixture, stirring to distribute it evenly. Reduce the heat to medium and cook until the bottom of the egg mixture is lightly browned, about 1 minute. Place under the broiler and cook until lightly browned on the top, about 2 minutes. Yields 1 frittata per serving.


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Home UM Athletics Collection Isabella Hutchison, coach of University of Miami women's tennis team
Isabella Hutchison, coach of University of Miami women's tennis team
Title Isabella Hutchison, coach of University of Miami women's tennis team
Summary Isabella Hutchison came to the University of Miami in 1965 to begin a women's intramural sports program. Hutchison went on to coach numerous sports, including tennis, golf, basketball and volleyball. She served as the Hurricanes' women's tennis coach from 1965 until her appointment as Director of Women's Athletics in 1977. Hutchison was inducted into the University of Miami Sports Hall of Fame in 2002. (http://www.umsportshalloffame.com/isabella-hutchison.html)
Note Indicated on paper attached to photo: "1974 Women's Intercollegiate Tennis Team, Left to right: Isabella Hutchison, coach; Cindy Ziff, Pam Sokol, Diane Armao, Faye Frankel, Lisa Robinette, Helen Weiner, Terry Salganik, Kitty van Allen"
Subject University of Miami -- Sports
University of Miami -- Tennis
Women athletes
Genre Photographs
Coverage Spatial Coral Gables (Fla.)
Physical Description 1 black and white photograph
Repository University of Miami. Library. University Archives
Collection Title University of Miami Athletics Collection
Collection No. ASU0010
Container Box No. 1
Folder No. 6
Folder Title: Tennis-Women's: Hutchinson, Isabela
Rights This material is protected by copyright. The copyright owner is unknown or unidentifiable. For additional information, please visit: http://merrick.library.miami.edu/digitalprojects/copyright.html
Standardized Rights Statement http://rightsstatements.org/vocab/InC-RUU/1.0/
Object ID asu0010000005
Digital ID asu00100000050001001
Type Still Image
Archive asu00100000050001001.tif
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