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PM Point Of View #85. Covid & the Art of Fundraising: A Theatre's Tale
With guest Amy Hand, Neal Racioppo, Roger Whyte, Laura Willumsen, Mara Mignogna, LeeAnet Noble, Alan Paul 23 April 2021
It was summer 2020. Covid-19 lingered on, with no end in sight. After months of canceled performances, funds were dwindling at Washington, DC's Shakespeare Theatre Company. Their last hope, the annual fundraising gala, was set for October. As the date drew near, it became clear that there would be no party. The staff had to come up with Plan B, and they had to do it fast. This is the story of a creative project team, dedicated to their mission. Their clear, agile response provides concrete and inspiring lessons in the power of Project Management.
Listen, learn, and get a free PDU!
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Amy Hand
Amy Hand is the General Manager at Shakespeare Theatre Company in Washington, DC. Prior to joining STC she served as the Operations Manager at San Francisco Ballet, the Associate General Manager at American Conservatory Theatre, and the Production Stage Manager for Atlanta Ballet.
Mara Mignogna
Mara Mignogna is the Development Events Manager at DC's Shakespeare Theatre Company, and oversees the planning of all of the Theatre's internal events including the 2021 Virtual Gala, Shakespeare Everywhere. Seeing the joy and lasting memories created fuels Mara's spirit for designing and executing events.
LeeAnet Noble
LeeAnet Noble is a Howard University graduate, and certified in Equity, Diversity, and Inclusion from Purdue University. As an actor, director, choreographer, musician, and writer, her career has spanned over twenty years, working with STOMP, The Irish Repertory Theatre, Disney's The Lion King Experience, and more. She is passionate about creating change and celebrating inclusivity through the arts.
Alan Paul
Alan Paul is a director of theater and opera, and the Associate Artistic Director of Shakespeare Theatre Company in DC. Alan is also the recipient of the 2014 Helen Hayes Award for Best Director of a Musical for his production of A Funny Thing Happened On The Way To The Forum.
Neal Racioppo
Neal Racioppo, Senior Director of Marketing and Communications for the Shakespeare Theatre Company, has been an arts marketer in Washington, DC since 2001, working with STC and Arena Stage. He oversees the strategies and processes for STC's earned revenue and communications strategies.
Roger Whyte
Roger Whyte is the Founder & Principal of RJ Whyte Event Production, established in 2010. With a background in technical theater and production, Roger has been able to apply his skills to events in both the in-person and virtual spaces. He is an expert in designing events that are on budget, achieve fundraising goals, run smoothly, and have people talking for years to come.
Laura Willumsen
Laura Willumsen is Senior Director of Development of the Shakespeare Theatre Company, responsible for all fundraising efforts. Prior positions include Institutional Major Gifts Officer at the Smithsonian's Freer|Sackler, Executive Director of the Pittsburgh Center for the Arts, Director of Marketing for Pittsburgh Opera, and Manager of the Folger Consort. Willumsen holds bachelor's and master's degrees in music performance.


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The Library of Congress > Researchers > Search Finding Aids > Rita R. Colwell papers, 1931-2004
Rita R. Colwell papers, 1931-2004
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The status of copyright in the unpublished writings of Rita R. Colwell is governed by the Copyright Law of the United States (Title 17, U.S.C.).
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The papers of Rita R. Colwell are open to research. Many collections are stored off-site and advance notice is needed to retrieve these items for research use. Access to digital content is available onsite only in the Manuscript Reading Room and requires advanced notice. Researchers are advised to contact the Manuscript Reading Room prior to visiting.
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redpajama_set_name: RedPajamaCommonCrawl


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Una estampida (voz de origen provenzal) es un movimiento desorganizado provocado entre animales en manada o una multitud de personas que colectivamente comienza a correr sin rumbo ni un propósito claro (aunque en el caso de las estampidas humanas, sí tienen propósito general y rumbo).

Las especies asociadas a este comportamiento en el mundo animal incluyen vacas, elefantes, gorgones, morsas, caballos salvajes y rinocerontes. Tanto en animales como en personas, puede tener efectos mortales, especialmente si cunde el pánico.

Estampidas bovinas
Algo inusual puede dar inicio a una estampida. Especialmente por la noche, algo como encender un fósforo, alguien montado a caballo, un caballo sacudiéndose, la caída de un rayo, una planta rodadora atravesando la manada, o «un caballo que corre a través de un rebaño dando patadas a una silla de montar que se ha enganchado bajo su vientre» son cosas que podrían causar estampidas.

Una gran estampida normalmente arrasa con todo a su paso. Para tratar al ganado, los vaqueros intentan hacer girar a la manada en movimientos circulares en lugar de correr hacia un acantilado o un río, y evitar daños la propiedad o a seres humanos. Las tácticas usadas para hacer que la manada se mueva en movimientos circulares incluyen disparar una pistola, lo que crea el ruido para que los líderes de la estampida se giren.

Los animales propensos a una estampida, especialmente ganado vacuno, tienen menos probabilidades de hacerlo después de haber comido y distribuidos en grupos más pequeños para digerir sus alimentos. Para reducir aún más el riesgo de estampidas, en ocasiones los vaqueros cantan o silban para calmar los rebaños inquietos al caer la noche. Durante su vigilancia nocturna evitan hacer cosas que podrían asustar a la manada e incluso se alejan antes de desmontar un caballo o encender un fósforo.

Frecuentemente la gente induce a propósito al ganado a un estampida como parte de la guerra o la cacería, como algunos nativoamericanos, quienes eran conocidos por causar que el bisonte americano muriera al saltar a un acantilado.

Estampidas humanas

Una estampida humana ocurre cuando una aglomeración de personas intenta desplazarse de forma repentina y con virulencia hacia una dirección, sin atener al buen orden o las consecuencias para los demás integrantes del grupo. A diferencia de las estampidas bovinas, donde la manada inicia un desplazamiento sin rumbo ni propósito claro, en el caso de las estampidas humanas sí que existe un motivo, un objetivo y un rumbo concreto (normalmente hacia salidas o puntos de evacuación).

Referencias

Enlaces externos

Desastres
Peligro (situación)

redpajama_set_name: RedPajamaWikipedia


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Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma
Edwin C. Douglass, Susan T. Rowe, Marc Valentine, David M. Parham, Roger Berkow, W. Paul Bowman, Harold M. Maurer
Texas College of Osteopathic Medicine
In three cases of alveolar rhabdomyosarcoma with variant translocations, two tumors contained an identical translocation, t(1;13)(p36.1;q14); the third tumor contained a t(8;13)(p21;q14). All three patients were 2 years old, markedly younger than the median age for patients with t(2; 13)‐positive alveolar rhabdomyosarcoma. The alteration of genetic material on chromosome 13 may be of primary importance in the development of alveolar rhabdomyosarcoma.
Genes, Chromosomes and Cancer
https://doi.org/10.1002/gcc.2870030611
Alveolar Rhabdomyosarcoma
Douglass, E. C., Rowe, S. T., Valentine, M., Parham, D. M., Berkow, R., Paul Bowman, W., & Maurer, H. M. (1991). Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma. Genes, Chromosomes and Cancer, 3(6), 480-482. https://doi.org/10.1002/gcc.2870030611
Douglass, Edwin C. ; Rowe, Susan T. ; Valentine, Marc ; Parham, David M. ; Berkow, Roger ; Paul Bowman, W. ; Maurer, Harold M. / Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma. In: Genes, Chromosomes and Cancer. 1991 ; Vol. 3, No. 6. pp. 480-482.
@article{7cae17f4bfb44fefb3067b74af55b692,
title = "Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma",
abstract = "In three cases of alveolar rhabdomyosarcoma with variant translocations, two tumors contained an identical translocation, t(1;13)(p36.1;q14); the third tumor contained a t(8;13)(p21;q14). All three patients were 2 years old, markedly younger than the median age for patients with t(2; 13)‐positive alveolar rhabdomyosarcoma. The alteration of genetic material on chromosome 13 may be of primary importance in the development of alveolar rhabdomyosarcoma.",
author = "Douglass, {Edwin C.} and Rowe, {Susan T.} and Marc Valentine and Parham, {David M.} and Roger Berkow and {Paul Bowman}, W. and Maurer, {Harold M.}",
doi = "10.1002/gcc.2870030611",
journal = "Genes, Chromosomes and Cancer",
Douglass, EC, Rowe, ST, Valentine, M, Parham, DM, Berkow, R, Paul Bowman, W & Maurer, HM 1991, 'Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma', Genes, Chromosomes and Cancer, vol. 3, no. 6, pp. 480-482. https://doi.org/10.1002/gcc.2870030611
Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma. / Douglass, Edwin C.; Rowe, Susan T.; Valentine, Marc; Parham, David M.; Berkow, Roger; Paul Bowman, W.; Maurer, Harold M.
In: Genes, Chromosomes and Cancer, Vol. 3, No. 6, 11.1991, p. 480-482.
T1 - Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma
AU - Douglass, Edwin C.
AU - Rowe, Susan T.
AU - Valentine, Marc
AU - Parham, David M.
AU - Berkow, Roger
AU - Paul Bowman, W.
AU - Maurer, Harold M.
N2 - In three cases of alveolar rhabdomyosarcoma with variant translocations, two tumors contained an identical translocation, t(1;13)(p36.1;q14); the third tumor contained a t(8;13)(p21;q14). All three patients were 2 years old, markedly younger than the median age for patients with t(2; 13)‐positive alveolar rhabdomyosarcoma. The alteration of genetic material on chromosome 13 may be of primary importance in the development of alveolar rhabdomyosarcoma.
AB - In three cases of alveolar rhabdomyosarcoma with variant translocations, two tumors contained an identical translocation, t(1;13)(p36.1;q14); the third tumor contained a t(8;13)(p21;q14). All three patients were 2 years old, markedly younger than the median age for patients with t(2; 13)‐positive alveolar rhabdomyosarcoma. The alteration of genetic material on chromosome 13 may be of primary importance in the development of alveolar rhabdomyosarcoma.
U2 - 10.1002/gcc.2870030611
DO - 10.1002/gcc.2870030611
JO - Genes, Chromosomes and Cancer
JF - Genes, Chromosomes and Cancer
Douglass EC, Rowe ST, Valentine M, Parham DM, Berkow R, Paul Bowman W et al. Variant Translocations of Chromosome 13 in Alveolar Rhabdomyosarcoma. Genes, Chromosomes and Cancer. 1991 Nov;3(6):480-482. https://doi.org/10.1002/gcc.2870030611
10.1002/gcc.2870030611
UNT Health Science Center contact form


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Monster Energy's Birk Ruud and Giulia Tanno Claim Freeski Big Air Gold Medals at the 2021 Kreischberg Austria World Cup Season Opener
Monster Energy's Birk Ruud and Giulia Tanno Claim Freeski Big Air Gold Medals at the 2021 Kreischberg Austria World Cup Season Opener
"Getting to the top here is an honor, and I am very proud of myself and the whole team. It is one of the sickest competitions I have participated in. The level of all the guys was completely insane." Monster Energy's Birk Ruud
KREISCHBERG, Austria (PRWEB) January 09, 2021
Way to start the new year! Monster Energy congratulates freeski athletes Birk Ruud and Giulia Tanno for earning gold in the Freeski Big Air Men's and Women's event, respectively, at the Kreischberg Austria World Cup today. Held as a closed-to-the-public event under strict Covid-19 safety guidelines at the popular Alpine resort, the nighttime event brought spectacular freeski aerial action to viewing audiences across the globe.
Both Ruud and Tanno had finished last year's FIS Freeski World Cup season by winning Crystal Globe trophies and just earned a head start with 1,000 World Cup points each in the 2021 ranking. These points are even more valuable considering that Kreischberg is the first qualifier for next year's Beijing 2022 Olympic Winter Games.
Without the usual crowds of spectators in attendance, this year's FIS Freeski World Cup season opener was broadcast live on television, streaming platforms and social media. Viewers were in for a world-class event, as the most competitive male and female freeskiers on the circuit brought their best aerial stunts to the site of the 2015 FIS Snowboard, Freestyle & Freeski World Championships.
As the newest addition to the Monster Energy freeski team, 20-year-old Ruud from Oslo, Norway, dominated a field of 60 international A-list riders on the giant aerial jump in the Men's Freeski Big Air event. The judges were looking for trick difficulty and creativity, which Ruud delivered on his two highest-scoring jumps of the day: The rookie put down a switch double cork 1800 for a score of 96.00 points on his first jump, then upped the ante with a perfectly landed double cinema mute grab 1800 for 97.20 points. With a total score of 193.20 points, Ruud claimed his fifth World Cup win.
"Getting to the top here is an honor, and I am very proud of myself and the whole team. It is one of the sickest competitions I have participated in. The level of all the guys was completely insane," said Monster Energy's Ruud upon claiming Men's Freeski Big Air Gold in Kreischberg.
As one of the youngest Big Air skiers on the circuit, Ruud has proven himself as a force to be reckoned with over the past few years. In 2016, Ruud won Freeski Slopestyle Gold at the Winter Youth Olympics at Lillehammer. He now has five FIS World Cup victories and four X Games medals (2 gold, 2 silver) under his belt, and heads into the 2021 season as a strong competitor.
In the Women's Freeski Big Air final, 22-year-old Tanno from Lenzerheide, Switzerland, faced off against a stacked field of the world's most competitive female freeskiers, including Estonian star athlete Kelly Sildaru. Undeterred by the competition, Tanno proceeded to put on a masterclass in style and precision as the reigning Crystal Globe holder.
While the rest of the field struggled to maintain consistently high scores, Tanno sealed her victory by sending a massive double cork 1080 safety and switch 1080 blunt across the gap. With an overall score of 173.40 points, Tanno took home gold at Kreischberg, her second FIS World Cup victory to date.
"When I launched this last jump, I tried it all for everything since I was already on the podium," said Monster Energy's Tanno after taking Men's Freeski Big Air Gold in Kreischberg.
Last year, Tanno took home the 2019/20 Big Air Crystal Globe trophy as the top rider of the season. Aside from Big Air, Tanno also competes in Slopestyle and claimed bronze in the discipline at X Games Norway 2020. Tanno's X Games total currently stands at four medals (2 silver, 2 bronze).
For more on Ruud, Tanno and the Monster Energy freeski team, visit http://www.monsterenergy.com. Also look forward to our ski and snowboard athletes bringing the stoke to X Games Aspen 2021 starting on Friday, January 29, 2021. Make sure to follow Monster Energy on YouTube, Facebook, Instagram, Twitter for exclusive behind-the-scenes looks as the 2021 freeski season continues.
About Monster Energy
Based in Corona, California, Monster Energy is the leading marketer of energy drinks and alternative beverages. Refusing to acknowledge the traditional, Monster Energy supports the scene and sport. Whether motocross, off-road, NASCAR, MMA, BMX, surf, snowboard, ski, skateboard, or the rock and roll lifestyle, Monster Energy is a brand that believes in authenticity and the core of what its sports, athletes and musicians represent. More than a drink, it's the way of life lived by athletes, sports, bands, believers and fans. See more about Monster Energy including all of its drinks at http://www.monsterenergy.com.
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More News For You
New Marijuana Bill Could Save The Country From Economic Ruin
There's a scary truth behind all these new skills we've learned and hobbies we've taken up this year, and all this free time we've had to binge-watch every show on every streaming service under the sun.
The ugly truth is that we're just staving off an economic crash caused by the isolation we've been forced to endure over the course of this pandemic. Restaurants, sports arenas, and concert halls have been destroyed by government rules and regulations restricting our plans to gather, and, with evictions allowed to resume at the end of the year as a federal moratorium expires, an economic catastrophe awaits.
Our nation could very fall into a massive recession, if not a full-on depression, lest we are gifted some new economic boom to the likes of the Gold Rush over 170 years ago.
And like some miracle handed down from the gods, the House of Representatives is considering a bill that could do just that.
This week the U.S. House of Representatives is expected to vote on a bill that would remove marijuana from the Controlled Substances Act and require federal courts to expunge many prior marijuana offenses. It will be the first time the full House will vote on ending the federal prohibition of cannabis.
Morgan Fox with the National Cannabis Industry Association says House passage would "send a really strong message to not only the rest of Congress, but to a lot of other states that the time to end prohibition has come."
The Marijuana Opportunity Reinvestment and Expungement Act (MORE Act), introduced by Rep. Jerry Nadler (D., N.Y.), would eliminate conflict between state and federal law and allow states to set their own marijuana policies.
"We don't need to have one size fits all. We just need to get rid of prohibition and then let the states do what the states are doing. It's essentially what the states have done already. They haven't waited for the federal government, which is why we have a lot of these discrepancies and challenges," said Rep. Earl Blumenauer (D., Ore.), who has long pushed for marijuana legalization.
The economic impact of marijuana has been monumental in the 30-some states where some form of the plant has been made legal or decriminalized. This could just be what the nation needs to get back on its feet after the COVID-19 crisis.
*The views and opinions expressed here are solely those of the author of the article and not necessarily shared or endorsed by FreedomClash.com*
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Elections 2012: Why the Economy Might Not Matter
James Quirk
@webquirks
November 05, 2012 05:56 EDT
As the US election day dawns, history suggests that the issues debated in a presidential campaign will not be ones that are most important to the next president.
As US Secretary of Defense, Donald Rumsfeld famously identified one category of risks in Iraq as "unknown unknowns" – those things that "we do not know we don't know." Nassim Nicholas Taleb developed the black swan theory, dealing with the occurrence of highly unlikely, nearly unpredictable and critically important events. History suggests that these are ways to look at the new presidential administration, too.
Much has been made of the economy during this 2012 campaign, and rightly so. Unemployment rates have risen to levels not seen in a generation, the annual budget deficits and total US government debt have soared, and the housing sector has continued to struggle. Over the course of the campaign, Governor Mitt Romney and his fellow Republican candidates have criticized the policies and performance of Barack Obama, while the president has cited the slow economic recovery as evidence of the severity of the crisis he inherited and proof that his policies are working. The media cacophony has surged at every minute movement of the unemployment rate, assessing its impact on the race.
Past evidence, however, suggests that the campaign issues of presidential candidates can be very different than the challenges they face once in office.
Senator Obama distinguished himself as the anti-war candidate in 2007 and 2008, opposed especially to the war in Iraq and the Guantanamo detention center for suspected terrorists. But a great financial crisis consumed much of his administration's energies, while Republicans continued to attack his signature achievement, national health care reform. The Obama administration struggled with how to handle democratic movements and their aftermath in Iran, Egypt, Libya and Syria, while it sharply increased drone attacks into Pakistan and Yemen. Suspected terrorists continued to be detained at Guantanamo.
Previous administrations have also been driven by events not in their campaign platforms. In 1999, Texas Governor George W. Bush announced his run for the presidency with a speech about compassionate conservatism: tax, social and educational policies. His campaign argued against the humanitarian intervention and nation-building of the Clinton administration. President Bush achieved his tax cuts and education reform, but after the 9/11 attacks, his next seven years were dominated by the wars in Afghanistan and Iraq and their long and costly nation-building efforts.
Arkansas Governor Bill Clinton wooed both Wall Street and labor unions in his "It's the economy, stupid" campaign in 1992. But it was the meteoric rise of a dot-com industry that barely existed at the time he took office, that led the American economy throughout the decade. Meanwhile, Clinton struggled with an unexpected Republican revolution, financial crises in Mexico and Asia (and almost Wall Street), military-led humanitarian missions in Haiti, Somalia, Bosnia and Kosovo, and historic legal and political issues stemming from his personal behavior.
Earlier cases are also instructive:
As a presidential candidate, Vice-President George H.W. Bush promised a "kinder, gentler nation" and help to "freedom fighters" in Afghanistan, Africa and Nicaragua. As president, he helped manage the peaceful reunification of Europe, and his popularity soared by leading a global military coalition to liberate non-democratic (and oil-producing) Kuwait. But tagged with his broken no-new-taxes pledge, he was not re-elected.
Ronald Reagan was a staunch anti-Communist, but later developed a world-changing relationship with Soviet reformer Mikhail Gorbachev.
Governor Jimmy Carter ran as an outsider and reformer in the wake of Vietnam and Watergate, but struggled with high inflation, the Soviet invasion of Afghanistan, and the relentless story of Americans held hostage in Iran.
Senator Harry Truman was famous for his investigations of the federal contracting system, yet is known for dropping atomic bombs on Japan (though he did not know of them before his presidency). He also presided over the Marshall Plan, NATO, the UN, the Cold War and the Korean War.
Herbert Hoover was a distinguished businessman, humanitarian, and powerful commerce secretary during a booming economy, but could not recover politically from the effects of the 1929 stock market crash. The examples go on and on.
Despite the current focus on the economy and Middle East, the challenges for the next presidential administration are likely to be as unpredictable as the collapse of the Soviet Union or the September 11, 2001 attacks or the Fukushima nuclear disaster. A very short list of possibilities ranges from traditional security concerns like chaos in Mexico, the Persian Gulf or the Korean Peninsula, to a "dirty" bomb in London, Bangalore or San Francisco. Crisis 2.0, like a successful cyberattack on air traffic control, energy infrastructure, the financial system, or the World Wide Web itself, would create untold havoc.
Add to these some good, old-fashioned troubles like a pandemic or drought. The H1N1 influenza virus (swine flu) in 2009 killed 14,000 people worldwide. But the 1918-1920 version, Spanish flu, killed tens of millions globally, infected more than a quarter of America and killed 0.5% of the US population, equivalent to 1.5 million people today. A catastrophic drought in America's heartland — or in Europe, China or India — would have regional and global economic and public health effects, with bread lines and food riots in unexpected places. Or, of course, the next administration's crisis could be something "unimaginable."
President-elect Bush did not know there were 19 men training to fly planes into buildings. President-elect Clinton had probably never heard of the future founders of Netscape and Amazon, nor President-elect Reagan a minor Politburo member named Gorbachev, nor President-elect Carter an aging, exiled Ayatollah.
For all the debate spin of who won or looked presidential or met expectations, there is a very fair chance that Governor Romney and President Obama do not know now — and even do not know that they do not know — the most important influences on the next four years of American and world history.
READ MORE IN THIS 360° SERIES
An Indonesian Reaction to Obama's Re-Election (Part II)
Jarno Lang • November 23, 2012
Purple America – The Best Election Maps
Donald Marron • November 12, 2012
INFOGRAPHIC: Meanwhile, on Planet America
FactBlink • November 06, 2012
Obligation to Speak
Uma Patel • November 06, 2012
US Presidential Campaign 2012
Atul Singh • October 04, 2012
Round One to Romney


That's right, before becoming the current home of the 16-foot Buddha that "floats" on a koi pond, Tao was originally a 19th century stable for Anderson Cooper's ancestors, the Vanderbilts. It was also renovated as a balconied cinema, before transforming into the present Asian wonderland.
Upon entering, you are literally instantly swept to a fantasy world that seems miles from the horns just outside on 58th street. In terms of ambiance, it would be difficult to find a more awe-inspiring culinary gallery. Our lunch was exceptionally delicious, as well.
Peking duck spring rolls drizzled with Hoisin sauce. The sweet potato and garlic of the Hoisin rounded out the tender and savory duck to such perfection, you don't even really need the mustard dipping sauce.
At our server's recommendation, we ordered the satay of Chilean sea bass on grilled asparagus. Never before has grilled sea bass given me goosebumps, and I need a bottle of the miso glaze in my refrigerator at all times.
The steamed vegetable dumplings were better than most, and certainly tastier than any yasai gyoza I have tried anywhere. Here, Tao successfully achieves a fresh garden filling with plump, al dente dumpling around a crispy cucumber salad.
Lobster wontons in shitake ginger broth.
Kieran (one of the few people in my life who actually craves fine Chinese cuisine and refuses to order take-out) gave the Kung Pao chicken his stamp of approval. I tasted this classic Szechuan dish, and would certainly have to agree... the chicken was exceptionally plump and juicy.
After settling the (very reasonable) bill, we felt as though we had just left the World Showcase at Disney's Epcot Center. And once the rice started expanding in our stomachs (as it inevitably does), we needed to walk off a few calories. I cannot more highly recommend a better post-Tao stroll than through the FAO Schwarz Manhattan megastore... We entered the famous giant, and Kieran yelped, "it's like were in Suri Cruise's bedroom!"
Kieran soft-shoed a riveting rendition of "Heart & Soul" on the "Big" Piano.
Matty was attacked by a Lego Chewbacca.
The store is literally three floors of rooms of toys connected by hallways of stuffed animals and dolls.
Matty and Kieran in the Clifford treehouse.
Sounds like a great day in New York.!!
Its nice to know there's someone like you who can find the cool and fun things in this town that makes me renew my love for this city.


Hey there! So sorry for the lack of updates lately. Anyways, here's a collective haul I got last month. I got several stuffs from L.A. colors because they were having a big sale. I knew I just had to have a lot of good stuffs. I'm also very happy my sister and I found these art deco nail polishes. Now, we wouldn't have a hard time designing our nails.
I also got myself the E.L.F. blush in peachykeen. Now this is something new from the range of blushes I have because this time, the shade is more coral-ish - peachy compared to my favorites- which are in pinks. I'm actually stuck with this blush right now. It kinda blends well with my complexion now after I got a little darker from sun exposure. I'm setting aside my other blushes first and I'll think this E.L.F. blush will go along way. Not to mention that is cheap too.
My sister and I also purchased these cute rings. I'm actually inlove with bow stuffs right now. From rings to necklaces, and tops. The first two rings were bought at Just G and the gold one I found at the SM Department store, accessories section. And finally, I found these pearl bangles. It was way cheaper from the ones I saw before that's why I'm so happy with these purchase. I actually saw them while I was paying at the counter at Genevieve Gozum.
I also bought a couple of tops. The black top I got from SM department store. It has a cute flower design and I also love the hemline which is weird. The white top is from Genevieve Gozum and the last 2 tops from Terranova. Lastly, I got myself a new pair of jeans from Levi's. I think this is from their new collection called Curves which says it hugs your curves perfectly. Kinda pricey for 3499php but I'm very contented with the fit. Everytime I buy a new pair, Levi's is actually my first choice because it fits on me well.
So I think that's it for now guys. I actually have more reviews due already. But I'm focusing on my review now. Next I'll be reviewing my current haul from Revlon (photoready foundation and 2 lipstick from their colorburst collection).
@abby: I actually got mine in Ayala Cebu, I'm pretty sure there are stores near you carrying L.A. colors. Thanks for the follow and comment dear!


text:
A lifetime on canvas and paper: "Ken Zonker: A Retrospective" opens at the Wynne Home
Few established artists can look back over their formative years and take sole credit for the success they've achieved.
It takes a multitude of professors, mentors, friends and family members to lend their support so that a student of the arts can find their place within the world.
For countless students at Sam Houston State University, one of those integral pillars of support came in the form of professor Kenneth Zonker, who taught art at the university for nearly four decades.
Zonker, an established and incredibly talented artist in his own practice, passed away in the spring of 2002, leaving a legacy of dedication to the university, along with an astounding portfolio of work which is now owned by his friends and colleagues in Huntsville, Walker County and all across the Lone Star State.
The Wynne Home Arts Center will be hosting an exhibition set to run from Jan. 30 through April 30 of Zonker's work, entitled "Ken Zonker: A Retrospective." The Wynne Home will be holding an opening reception for the exhibit tonight from 4:30 to 7.
"He lived simply, but passionately, spending his time teaching and creating his own art during the fall and spring semesters," said Roberta Plant, co-curator of the exhibit and Friends of the Wynne Home board member. "His summer months were spent traveling the world, cycling, climbing mountains, making new friends and meeting up with old friends from past travels. His passion for life and his artistic curiosity were inspiring and are reflected in the many works now on exhibit at the Wynne Home."
Spanning nearly every decade of Zonker's artistic practice, the exhibit showcases his unique styles, ranging from tight, pencil-drawn abstractions, to more robust and flowing self portraits in oil.
The sheer experimentation and breadth of the collection would lead an unknowing onlooker to believe they had stumbled upon a group exhibit, not one cast from a single artist.
"Those who visit the exhibit will see that he was always pushing his artistic boundaries, using different media and processes," Plant added. "His main love was pencil drawing and his works are extraordinary. Some are quite abstract, some very realistic, others are symbolic and many reflect his love for life and travel.
"Samuella Wynne Palmer and Ruth Wynne Hollingshead, donors of the Wynne Home Art Center, were very special friends and supporters of Ken Zonker's annual student art exhibit and sale at SHSU," Plant continued. "It is very special to see their childhood home now filled with Ken Zonker's art. Many collectors have generously loaned all of the pieces now on exhibit. It is a beautiful show, one of the best ever, I believe."
Born in Olney, Texas, in 1941, Zonker spent his early years in in Venezuela, where his parents worked as missionaries. The rugged peaks of the Andes Mountains operated as a perfect backdrop for a young painter's eye and the color and vivid shapes that he likely gleaned there is that of an artist's perfect dream, which now shows through in his vibrant work.
For his many students, Zonker was a passionate and caring professor. Known to be a hands-on teacher, Zonker would discuss fundamentals with each pupil as they worked, pushing them to improve their craft and technique in each assignment.
"His teaching style was very personal and very good," SHSU art major Travis Townsend told The Houstonian during a 2002 interview. "He would go up to his students as they were making their artwork and discuss with them, one-on-one, how they could make the artwork better."
"He was very into his students," SHSU art minor Lizzy Lynn also told the Houstonian. "He pushed their creativity in a fun way. He never put us down. That man made me better."
Zonker also left his mark on the faculty and staff at Sam Houston with his dedication to teaching, coupled with an unending drive to improve his own craft.
"Whenever I meet alumni of the art program from the 1960's, 70's, 80's, or 90's, they always mention Ken as someone who had an impact on their lives," SHSU professor and chair of the Art Department Michael Henderson said. "He also had a big influence on the art faculty who taught with him and I count myself as one of those people. I'm glad I got a chance to know him in my first year at SHSU before he passed away."
"Ken continues to teach through the students he inspired as they are now teachers and artist themselves, along with the scholarship in his honor that is given each year to a Sam Houston State University art student," Plant added. "I was fortunate to be his student and his friend and it was an honor to help put together this wonderful show. It's a must-see for both longtime admirers and those who will experience his art for the first time."
With the exhibition beginning tonight, an opening reception will be held from 4:30 to 7 p.m. and the public is invited to attend. For more information, call (936) 291-5424 or visit www.thewynnehome.com.
Author: Joshua Yates
Interdisciplinary artist Joshua Yates was born in Clearwater, Florida and moved to Houston, Texas at the age of two. He has received Bachelor of Fine Arts degrees with Highest Honors in Photography and Studio Art from Sam Houston State University while completing his Undergraduate Honors Dissertation in Performance Art Studies. With more than 10 years of experience behind the lens and a proven track record for enhancing digital and social media outlets, Yates has a passion for multi-platform journalism and visual communication in the digital space. He currently works as a Linux administrator for HostGator in downtown Houston.	View all posts by Joshua Yates
Author Joshua YatesPosted on January 30, 2016 March 7, 2017 Categories News Writing
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Legos are toys loved by all worldwide in both the hands, and sometimes painfully the feet, of children and adults alike around the globe. We have made great scultures or globs of connected cubes out of the interlocking pieces of plastic but the filmmakers took it a step further when they translated legos to the big screen with the first Lego Movie. They are now back again to bring us the eagerly awaited sequel that will pick up right where the first lego film left off.
Chris Pratt and Elizabeth Banks give us their insight into what it is like to be a lego seeing as how there is not real source material to draw from. Both describe how it is an honor to play a toy as timeless and universial as legos and Pratt even tells us how he feels as though he is in a simulation with all the amazing roles he has been given. Banks notes how she wishes he was as sassy as Wyldstyle as well as gives us her own personal poo-filled lego story that costars and audience eat up, as weird as that sounds. The second installment to the lego films comes out in February of next year so for now keep your eyes on the trailers.


Latest Update: – Another chance to all job hunter to make application form has provided by the RPSC for all candidates those not able to apply application form against Sub Inspector Posts. The Process to registration Application Form start from…… 27 June to 10 Sept 2018……… After fill application form candidates can correction application form in between ………..11 Sept to 17 Sept 2018…….
Finally the Rajasthan Government has announced RPSC SI Recruitment 2019. There is expected number of posts 340. Candidates those have interested to this recruitment now start preparation of examination. The Rajasthan Public Service Commission will soon start process to registration application form. Candidates those complete graduation degree can participate to RPSC SI vacancy 2019. It is great opportunity to all candidates those complete graduation degree and searching Govt Jobs in Rajasthan State. Candidates register application form before last date and start preparation of examination. More information RPSC SI Bharti 2019 candidates can read this article till last.
Still this RPSC SI recruitment 2019 notification have not released by Rajasthan State Government. soon after started these all invited posts online application form you all interested candidates can make submit them application form as soon as before going its last date of application. this RPSC SI Vacancy 2019 related all information will provide you just after released its official notification. The Application form submission last date has extend. According to notification of Rajasthan Public Service Commission now candidates can apply application form till 31 May 2018. for more information candidates keep stay connection with this page we will provide all information here.
There are education criteria to become part of RPSC Police SI Bharti 2019. Candidates need to have graduation degree from a recognized Institute or University.
The selection process to RPSC Police SI Bharti 2019 has importance to all application form applied candidates. The selection will be done based on written examination, Physical Test and documents verification. Candidates need to clear one by one all steps of recruitment. First of all they call to written examination.
Here is RPSC SI Bharti 2019 latest News. The Rajasthan Government has announced that it will soon start process to recruit 1100 candidates to vacant posts. Candidates those have interested to this recruitment they apply application form. If their application form has successfully accepted they start preparation of examination. Because after complete application form process, selection will be done based on written examination. Future Detail RPSC Sub Inspector vacancy 2019 candidates keep stay connection with this page.
The admit card have importance to all candidates for collect important information regarding to examination dates, Roll Number, Center and Much more. We suggest all applicant that without admit card you do not allow to attempted examination. Bring your hall ticket and get permission to appear in exam.


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Feudum: Rudders & Ramparts to Launch on Kickstarter March 1, 2019!
Published on January 30, 2019 by mark swanson.
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Published on October 07, 2018 by mark swanson.
Feudum: The Queen's Army is Now on Kickstarter!
Published on July 21, 2017 by mark swanson.


Before I launch into the recipe for Slow Cooked Lamb Shanks with Eschallots, Rosemary and Red Wine. I want to share something else with you.
I was thinking the other day about some of my frugal ways. I have travel on my mind again and am wondering how I am going to manage to get back to Europe. I need to save, save, save and as a result I did a mental note of what we already do to conserve our hard earned income.
One of the ways we save thousands a year, is not having a pool.
My darling mum has been ill in hospital and her pool has gone green. The pool man could not squeeze in a pool rescue for her, and these things are best dealt with in a speedy manner, lest they get even worse. So I spent all of Sunday in a Sydney heat wave, trying to clean it and filling it with chemicals to turn it blue again. Man were they expensive. Not to mention running the filter 24/7 for however long, until the water becomes clear. I can't wait to see the result, when I visit again later in the week. It better work.
Mental anguish aside, I actually love the current colour of the pool. It looks pretty against the jacarandas. What a shame the algae is so toxic. Of course the sensible thing would be to remove the jacaranda, which causes so may of the pool's problems. But it is seeded from one my grandmother gave to mum, when my parents built the house in 1964. Grandma had grown it in a jam jar, from a tree she had in Melbourne. That original tree was struck by lightening 20 years ago and was lost, but this one had previously grown on it's own from that tree. Although the practical thing would be to have it removed, the sentiment involved means mum just can't get rid of it. And it is a pretty centre piece to her back yard.
Madam was lying pool side as I scrubbed the walls with a steel brush. She said she was ready for the paparazzi, as she reclined on her towel.
I told her it was better to be famous for something creative, rather than just being famous for being famous. It all went over her head, but one has to wonder where a little girl absorbs a word and a concept like 'paparazzi'.
I took a shot of her and showed mum, who commented that hot pink is a great colour anywhere, any time. I have to agree.
I had to shoo my little one away when I was pouring chemicals into the pool. Happily she settled for a cold bath in her cozzie, rather than a swim in the green monster.
Another money saving technique, is using everything up in my freezer and putting the cash I save that week, in the holiday fund.
I found some lamb shanks at the bottom of a freezer draw and decided to make this.
Put the flour in a plastic bag with lamb shanks and shake to coat.
Place all ingredients in your slow cooker and cook on high for 6 hours.
Serving suggestion: Decant shanks into large individual ramekins, or pie dishes.
Top with remaining cooking juices and vegetables.
Garnish with extra rosemary, if desired.
You can find more easy family meals to make here.
Love lamb shanks too! Such great comfort food!
Yes it's fabulous on a cool night. Nothing beats comfort food.
We sure have had some great parties in that pool, but they truly are so much work. I'd love one if someone else did all the labour. Sadly Mr Beach House loves sailing too much.


text:
Martha, age 5.
First Grade School Photo
Laura (Mom), José (Dad), Patricia (11 years old), Martha (1½ years old), and Eddie (4 months). Taken July 27, 1997.
Martha Deanna Palacio was born on Friday, January 12, 1996, at 12:01AM, at Cedars-Sinai Medical Center in Los Angeles, California. She weighed 9 lbs 12.5oz. I, Laura Pulido), started labor on Wednesday, January 10, 1996 late at night. When we got to the hospital my contractions had started. The nurse offered anesthesia and told me that the contractions would be a lot more painful if I decided not to have anesthesia. They gave me an epidural. I was on the epidural for 24 hours before the doctor on-call decided to deliver Martha by C-Section. She never dropped. I was dilated, but the residents could not feel the baby's head.
When she was delivered the doctors took her to the side to "suction" her. Since this was my first baby I thought nothing of it. I did not question why the doctors were not showing me the baby. When they were through sucking all the gunk out of her airways, they wrapped her up in a blanket and put a knit cap on her head, just above her nose . They then showed me my baby. I saw this fair, flat nosed baby and thought to myself "she must be swollen from the long labor". She was taken to the NICU. I was told she had to be taken because it took them so long to make her breathe. I didn't find out about Martha's syndrome until the day after. The doctors had disguised her by wrapping her up in the blanket and putting the knit cap just-above her eyes. José, my husband, had been hand-gestured not to say anything.
The hospital genetics doctor and a social worker came to my room to explain to us that Martha was born with Apert Syndrome and what they knew about Aperts. In summary, the doctor said that Martha's syndrome affected her bones, that she would require surgeries throughout her life and he gave us an article on Apert Syndrome. The doctor explained that Martha's was a fresh mutation, since nobody else in either side of the family had this syndrome. The social worker gave us a list of resources and told us we could opt to give the baby up for adoption. I remember all this as if it was a dream. I really wasn't in touch with reality. I kept thinking everything was a dream and that I would wake up and none of it would have happened.
Martha was kept in the NICU for a week. During this week they ran all kinds of tests on her. A Neurologist came to talk to us and told us that Martha's brain was not normal. That they had taken a scan and that her brain did not have all the "lines" that a normal brain should have. She said that Martha would be "slow". Another doctor came to us and said that a yellowish-white fluid was coming out of Martha's nose and that it might be CSF (cerebral spine fluid) leaking out. We were freaking out. It wasn't CSF. I was feeling all kinds of different emotions. Happy because I was a mom for the first time, sad because my baby was born with a syndrome, angry at God for allowing my baby to have been born like she was, an on and on. Some of our relatives were saying to us, "We know what you're going through". This made us angrier. How could anyone know unless you've been there?
It is now a year and a half later. So far she has had three hand surgeries at Valley Presbyterian, David Auerbach, M.D. Both hands were operated on each time. The first surgery (on 6/6/96) was to separate the fingertips, which were fused. Unfortunately, during this operation she lost both middle fingers (the tips were removed and eventually the entire finger was taken out). The doctor said the bone was very weak and could not survive as a finger.
The second surgery was to separate the pinky and the thumb. Skin grafts were taken from the left and right groin. This one was done on 9/4/96. She had both arms in casts. The casts came off on 9/26/96.
Her third hand surgery was on 2/5/97. The bone removed from her middle fingers was used to straighten out her thumbs which were crooked.
Dr. Hryar Shahinian (he came to Cedars-Sinai from New York in August, 1996) did her first head surgery (cranial vault remodeling) on Monday, 9/30/96. Hrayr Shahinian, MD, is the Director of the new Skull Base Program. He has operated on many kids with Aperts and Crouzons. He's is a WONDERFUL doctor!
She has not been referred to a craniofacial team. When I spoke to the pediatrician and insurance group and explained to them what I had read about Aperts, and that Martha would need to be followed by a team of doctors, they gave me a list of doctors who contract with their HMO. They are not a group nor do they work as a craniofacial team. I'm taking everything one-day-at-a-time. She goes to her pediatrician (who also has never seen another baby with Aperts) about every other month for physical check ups.
Martha is like the other Aperts babies I've read about, very sweet and lovable. And, so far she appears to be very intelligent. She's been evaluated by a Regional Center and was rated to be normal, mentally. She'll be re-evaluated in a few months.
I wish people wouldn't stare. I expect them to look but how can we make them understand that, as with anybody else, it isn't polite to stare. Depending on my mood (and hormone level, I guess), sometimes I smile at the gawkers, sometimes I give them "dirty looks" and at other times I tell them off.
Martha has an older sister (Patricia, 11 yrs) and a baby brother (Eddie, 6 months). José (dad, 39), and Patricia are great help and support.
Martha just recently started walking (at about 19 months). She is having a ball and is very independent when she's trying to find her way around. I've locked all the drawers in the kitchen because she was going in them and taking out the pots and pans and spreading them on the floor.
Laura Pulido, September, 1997
The Many Faces of Martha and Family
After first hand surgery - separated fingertips
Martha's first birthday - 1/12/97
Martha's birthday cake, 1/12/97
Martha with Tricia and Eddie, 3/31/97
� 1997-2015 apert international, inc.
All photos and text are the property of the families represented and Apert International, Inc., and may not be used without their consent.


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Vue Bootstrap file input is a field which user can use to upload one or more files (photos, documents or any other file type) from the local storage.
Below you can see a number of Bootstrap file inputs created with Material Design for Bootstrap.
In this section you will find advanced information about the File Input component. You will learn which modules are required in this component, what are the possibilities of configuring the component, and what events and methods you can use to work with it.


text:
No Feeling Sorry
Rick Cowdery
A MEASURE of the injury whirlwind which has blown through Home Park could be realised by looking at the substitutes' bench which started Saturday's 2-2 Home Park draw against Oxford United.
The six – already one short – players on it had made 34 Argyle career starts between then – and Craig Tanner, who scored the second equaliser against the Pilgrims Sky Bet League 2 promotion rivals accounted for 23 of those. Sixteen-year-old Jordon Bentley was whistled up from the apprentice ranks to sit alongside Tyler Harvey, who had been out injured for several weeks.
Argyle began the match without Carl McHugh, Ryan Brunt, Oscar Threlkeld, Jordon Forster, Deane Smalley and Callum Hall, and ended it with Peter Hartley on that long list after he hobbled off at half-time.
Ben Purrington started his first league game of the season in central midfield and ended it at left-back; Gary Sawyer started at left-back and ended playing his first league game of the season at centre-back, in a back four that showed three changes from the one that had begun at Barnet four days earlier.
So, then, plenty of justification for Argyle captain Curtis Nelson to put forward for Argyle's failure to win?
He said: "You could easily say we had a chance to feel sorry for ourselves and say 'That's it' but I think we have done really well to dig out a point, and we worked hard to do that.
"Obviously, we were missing quite a few players and we can use that as an excuse, but it was a good point – nothing lost, nothing gained.
"For me, personally, it is not great, losing your partner-in-crime, but Gaz stepped in, and Ben Purrington, and both did brilliantly, so you have got to give a hand to both of them."
Nelse led by example, leveling Peter's 12th-minute own goal after a quarter of an hour, and displaying the same character as his team-mates to come back and level Kemar Roofe's first-half strike with Tanner's header 15 minutes from time.
"We have shown that during the season, as well," said Nelse. "There have been times when we've been behind, or [the opposition] have got an equaliser and we have shown character to come through; credit to the management team, the manager and the boys in the changing-room.
"It's always difficult to see one of your team-mate's injured but you have just got to wish them all the best for a speedy recovery.
"I'm gutted for all of them. Brunty's looks quite a long injury which is really unfortunate because he was hitting form and scoring goals; he's been doing really well. Obviously, Fozzie's come in and done well, too. I think he'll be back sooner, rather than later.
"We've shown today that people can come in and fill in; I have got to give credit to the manager and to the boys for having such a strong squad.
"It is not something we are going to necessarily worry about. It's a shame, because you don't want people injured, but hopefully we have one or two back next week against Accrington and we go again.
"It's another big game. I think it's important, as with every game, that we go to get three points."


Bangalore, May 27, 2016 – As a part of the Contextual Learning Programme and Canadian International School's (CIS) Community Service, today 36 students of Grade 7 painted murals on the pillars near the Kogilu Junction cross road, Yelahanka spreading messages such as "Be safe on the road", "Look out" and "Share the road" through visual arts. The students cleaned up the surrounding area as a contribution to "Swatch Bharat" initiative and also planted saplings around the jogging track of Yelahanka Lake.
Furthermore, Chief Guest, Mr. SR Vishwanath – MLA of Yelahanka Constituency painted the pillars along with the students. Mr Ravi – President of YUVA- Yelahanka, and Mr. Shiva Kumar – President of the Yelahanka Lake Association supported the CIS team at this initiative. Ms. Devaki Rao – Elementary and Middle School Visual Arts teacher at Canadian International School organized this event in order to provide engagement and practical learning to students for spreading social messages through visual art.
"Often students and teachers get used to art and craft sessions in the classroom. But today, we stepped out of our comfort zone to give an expression to our creativity. The 7th Grade students were excited about the entire process and experienced a beautification project with an objective behind it. The students have not only learnt about mural art but also the possibilities and limitations of it in the open space", said Ms. Devaki Rao – Elementary and Middle School Visual Arts teacher at Canadian International School.
Social Responsibility is a key facet of Contextual Learning. Contextual Learning is about making connections between what students are learning hands-on and how they are implementing the same understanding on-ground to connect with their community and environment.
"Painting the pillars today is a part of our giving back to the community and it's also a part of what Contextual Learning at Canadian International School is all about. The 7th grade students took up this initiative which will help the junction look more beautiful. It would be great if everyone could take up such initiatives in and around their locality. It will not take much to make the city look beautiful", said Mr. Shane Kells – Head of School at Canadian International School.
"This painting is not only for our school and having fun but also to tell people that we can change India in many different ways. I really liked doing this painting because it means something not only to us but also to the place and the people around", said Cloe Plaza – student of Grade 7, Canadian International School.


text:
Q: Performance user timings API measure not working properly when started from 'navigationStart' To measure the performance of an app using the performance user timigs API, I use the following code in the place where the application is loaded completely.
window.performance.mark('stop-step');
window.performance.measure('app_load_performance', 'navigationStart', 'stop-step');

While profiling, in the performance tab, the Timings section show the performance marker only when web app was refreshed in a browser window where the web app is already running.
If this is profiled from a new browser tab where the web app is newly executed, the profiling does not show the performance marker.
This is a react app. Could there be something that is limiting the application to show the performance marker from the new tab?

A: According to Mozilla Navigation and resource timings;

The performanceTiming API, a JavaScript API for measuring the
loading performance of the requested page, is deprecated but
supported in all browsers. It has been replaced with the
performanceNavigationTiming API.

What happens when there is no context and the mark navigationStart is pointed in the same page:

When the prompt for unload terminates on the previous document in the
same browsing context. If there is no previous document, this value
will be the same as PerformanceTiming.fetchStart.

And in the new API:

The Navigation Timing API provides data that can be used to measure
the performance of a web site. Unlike JavaScript-based libraries that
have historically been used to collect similar information, the
Navigation Timing API can be much more accurate and reliable.

Also if you scroll down in the new API page, you can see that the fetchStart mark has been marked for deprecation.
There is a high chance that for some reason your browser is no longer handling this mark. And the new library has no backward compatibility with the old one. So this would explain why you can see the performance when there is a previous document, but you can't see it when there isn't.

redpajama_set_name: RedPajamaStackExchange


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text:
\section*{\large\bit 1) Introduction}

Very soon after the formation of a neutron star,
thermal energies inside it drop below the energy gap associated with
neutron pairing. One therefore expects all but the outermost parts of
the crust to pass rapidly into a superfluid state \cite{Mi,Gi,PiAl}.
The critical angular velocity for vortex formation is negligibly small for
bodies of astronomical size and therefore, as first noted by Ginzburg and
Kirzhnits \cite{GiKi}, the star's interior will be threaded by vortex lines
parallel to the axis of rotation.\par
A stimulating review by Kirzhnits and Yudin \cite{KiYu1} discusses some of
the interesting and surprising general-relativistic effects associated with
superfluid neutron stars. Consider, for instance, an imaginary experiment
in which the star is initially at rest and a spin is imparted to the crust.
Lense-Thirring (frame-dragging) effects will make it appear that the
superfluid interior has been set into partial co-rotation, i.~e.~, the
contravariant azimuthal velocity $v_s^\phi = d\phi /dt$ with
respect to distant stationary observers will become non-zero.
If the crust is separated from the fluid by a small gap, then this induced
rotation can easily exceed the critical angular velocity without forming any
vortices. This is because the superfluid's orbital angular momentum,
proportional to the covariant component $v_{s\phi}$, remains zero.
The induced rotation also makes no contribution to the value of the
metric coefficient $g_{\phi t}$ (the ``gravimagnetic potential''),
whose non-vanishing is due entirely to the rotation of the crust.\par
Superfluid flow is in all circumstances irrotational.
For regular axisymmetric flows this implies $v_{s\phi}=0$,
i.~e.~, the superfluid can never acquire orbital angular momentum.
It is nevertheless able to entrap
angular momentum within the cores of its vortex filaments, which consist of
normal fluid. To simplify the description, one generally assumes that
it is permissible to replace the vortex array by a fictitious
``effective'' orbital flow ($v^{eff}_{s \phi}\neq 0$) when averaging
over macroscopic domains, i.~e.~, domains large compared with the vortex
spacing (about $10^{-2}cm$ for the Crab pulsar). The equivalence
assumption is that gravitational and other physical effects of the vortex
array are macroscopically indistinguishable from an effective orbital motion
having the same distribution of angular momentum. This seemingly innocent
assumption is called into question  in a recent analysis by Kirzhnits and
Yudin \cite{KiYu2}. The authors do not succeed in finding an acceptable
solution representing the contribution of a vortex line to the external
gravitational field of a spherical body in the linearized Einstein theory.
They conclude: ``The general formula relating the angular momentum
of a body with the asymptotic behavior of its gravimagnetic field
is invalid when vortex filaments are present.''\par
This conclusion is not easy to understand intuitively, since the
formation and slow migration of vortices into the superfluid from the
interface with the crust is macroscopically an axisymmetric process, which
conserves angular momentum locally and involves no appreciable
redistribution of mass. It is therefore hard to see how it can affect
the external gravitational field at all, much less suppress all
gravimagnetic effects, as the angular momentum of the crust gradually becomes
``vorticized''. In short, there is no obvious reason why spin and
orbital angular momentum should behave in a fundamentally different way
as sources of gravity.\par
The issue is perhaps elementary but clearly important because of the
potential implictaions for the gravitational dynamics of the binary pulsar
and gravitational radiation from neutron star mergers.
To remove any possible doubt it seems worth devoting some effort
to an explicit verification that bulk rotation and vortex filaments
are indeed equivalent in their gravitational effects, and this
is the object of our paper. In section 2 we review the phenomenological
form taken by the Einstein field equations for a medium which is
gravitationally polarized by alignment of internal spins. The effect of this
spin polarization on the gravimagnetic potential near infinity can be inferred
from an integral identity due to Komar, and this is discussed in section
3. These results are exact and valid for strong fields. If the gravitational
field is weak (i.~e.~non-relativistic) the linearized Einstein equations
provide a complete solution of the problem (section 4). Finally section
5 is devoted to the simplest realisation of the superfluid
neutron star within the framework of linearized gravity, namely a
spherical star of constant density with purely azimuthal, locally
irrotational flow. This flow corresponds to having a single vortex
filament along the axis. The origin of the contribution to the far-field
gravimagnetic field is traced back to the singularity of the flow along
the axis of rotation.

\section*{\large\bit 2) Einstein field equations for a medium with
internal spin}

Analogously to the Maxwell-Lorentz equations for a dielectric medium,
there is a statistically averaged form of the Einstein field equations
appropriate for the coarse-grained description of a gravitationally
polarized granular medium \cite{Isr1}. In the case of interest to us here
the polarization is a spin alignment of the granules.\par
At the sub-macrolevel, the material inside each granule is described by a
symmetric conserved tensor $T^{ab}_{micro}$, representing the
flux of 4-momentum, which couples to the Einstein tensor in the
standard way. On larger scales, it becomes meaningful to split the
complex motion of the material into a translational motion of the granules and
a distribution of internal spins. Correspondingly the coarse-grained average
$T^{ab}= <T^{ab}_{micro}>$ splits into $\mathcal{T}^{ab}$, the flux of
translational 4-momentum and a contribution from $S^{abc}$, the flux
of spin angular momentum (skew in the first two indices:
$S^{abc}=S^{[ab]c}$). Detailed analysis \cite{BaiIsr} shows
that the coarse-grained form of the Einstein field equations is
\begin{equation}\label{macein}
  G^{ab}=8\pi T^{ab}\quad\text{where}\quad T^{ab}={\mathcal T}^{ab} +
  \nabla_c U^{abc},\quad U^{abc} = \frac{1}{2}(S^{acb} + S^{bca} - S^{abc})
\end{equation}
The translational momentum flux ${\mathcal T}^{ab}$ is neither
symmetric nor in general (in a curved spacetime) conserved. The symmetry and
conservation  of $T^{ab}$ are equivalent to the conditions
\begin{equation}\label{sym}
  {\mathcal T}^{[ab]} = \frac{1}{2}\nabla_c S^{abc},\quad
  \nabla_b{\mathcal T}^{ab} = -\frac{1}{2} R^a{}_{bcd}S^{cdb}.
\end{equation}
Equations (\ref{macein}) are formally identical with the well-known
Belinfante-Rosen\-feld prescription for symmetrizing what is called
(in a field-theoretic context) the ``canonical'' stress-energy tensor
\cite{Wein1}.\par
The simplest illustrative example is a gas of spinning particles. If
the skew tensor $s^{ab}$ denotes the angular momentum of a particle,
$p^a$ its 4-momentum and $v^a$ its 4-velocity, then
$$
{\mathcal T}^{ab}(x) = \int N(x,p,s) p^a v^b \omega_g(p,s),
\qquad S^{abc}(x) = \int N(x,p,s) s^{ab}v^c \omega_g(p,s),
$$
where $N=N(x,p,s)$ is a distribution function and $\omega_g(p,s)$ the
invariant volume form on spin-momentum space. Here the asymmetry of
${\mathcal T}^{ab}$ arises from the non-collinearity of $p^a$ and $v^a$
for a spinning particle.

\section*{\large\bit 3) Tolman-Komar integral identities}

To check that the spin angular momentum concealed in (\ref{macein})
makes its proper contribution to the gravimagnetic potential $g_{\phi t}$,
it is simplest to appeal to the Tolman-Komar integral identities
(see e.~g.~\cite{FroIsrUnr}. These are rigorous general-relativistic
analogues of Gauss's flux theorem, which hold for spacetimes admitting
Killing-symmetries and relate volume integrals over the matter content
of an isolated system to surface integrals at infinity
\begin{align}
&\nabla_{(a}\xi_{b)} =0 \quad\Rightarrow\quad
\nabla^2\xi_b = - \xi_a R^a{}_b\nonumber\\
&\int\limits_{\partial\Sigma}\nabla_a\xi_b d^2\sigma^{ab} =
-8\pi \int\limits_{\Sigma} \xi_a(T^a{}_b -\frac{1}{2}
\delta^a{}_b T) d^3\sigma^b\nonumber\\
\end{align}
For stationary fields ($\xi^a=\partial_t^a$) we have Tolman's theorem
$$
m = \int(T^i{}_i -T^t{}_t)\sqrt{-g}d^3x,
$$
where the integration is over a $t=const$ 3-space, $i$ runs over the three
spatial coordinates, and the gravitational mass $m$ is defined by the
asymptotic form
$$
g_{tt}\approx -(1-\frac{2m}{r}) \qquad (r\to\infty).
$$
For an axisymmetric system, the gravitating angular momentum $ma$,
defined by the asymptotic form
$$
g_{\phi t}\approx -\frac{2ma\sin^2\theta}{r} \qquad (r\to\infty)
$$
in asymptotically spherical coordinates, is similarly given by
\begin{equation}\label{spin}
ma = \int T_\phi{}^t \sqrt{-g}d^3x,
\end{equation}
For our purpose  $T_\phi{}^t$ is most conveniently recast
in the covariant form $\xi^a T_a{}^b \nabla_b t$,
where $\xi^a=\partial_\phi^a$ is the axial Killing vector.
Making use of (\ref{macein}), the identity
\begin{equation}\label{spinid}
  U^{abc}-U^{cba}=S^{abc},
\end{equation}
and the Killing property that $\nabla_a\xi_b$ is skew, we find
$$
\int\limits_\Sigma \xi^a(T_a{}^b - {\mathcal T}_a{}^b)d^3\sigma_b =
\int\limits_\Sigma \nabla_c(\xi^a U_a{}^{bc}) d^3\sigma_b -
\frac{1}{2}\int\limits_\Sigma \nabla_c\xi_a S^{acb} d^3\sigma_b
$$
Since the total derivative integrates to zero, (\ref{spin}) becomes
\begin{equation}\label{spinorb}
  ma = \int{\mathcal T}_\phi{}^t\sqrt{-g}d^3x - \frac{1}{2}
\int S^{act}(\nabla_c\xi_a) \sqrt{-g}d^3x,
\end{equation}
in which the separate contributions of the orbital and
spin angular momentum are displayed explicitly.
To check that the second term has indeed the right form, we go to the
non-relativistic weak-field limit, in which we can set
$$
\xi_a \approx \rho^2\nabla_a\phi\qquad S^{\rho\phi t}\approx\frac{1}{\rho}
\epsilon^{\rho\phi z} S_z,
$$
in cylindrical coordinates ($\epsilon^{abc}$ is the three-dimensional
permutation symbol).
Then the second term in (\ref{spinorb}) reduces to $\int S_zd^3x$,
giving the $z$-component of the total spin angular momentum as it should.

\section*{\large\bit 4) Linearized theory}

In the case of weak fields we can obtain a complete solution to the
problem by integrating the linearized Einstein equations \cite{Wein2}.\par
In approximately rectangular coordinates the metric perturbation $h_{ab}$
and its trace-reversed form $\bar{h}_{ab}$ are ``small'' quantities
defined by
$$
g_{ab}=\eta_{ab} + h_{ab}\qquad \bar{h}_{ab} = h_{ab} - \frac{1}{2}h
\eta_{ab},
$$
where $\eta_{ab}$ is the Minkowski metric. The coordinate
freedom  allows us to impose the four (``harmonic'') gauge
conditions $\partial_a\bar{h}^{ab}=0$, with respect to which the Einstein
equations and their integrability condition (the linearized
conservation laws) reduce to the simple form
$$
G_{ab} = -\frac{1}{2}\partial^2\bar{h}_{ab} = 8\pi T_{ab}, \qquad
\partial_aT^{ab}=0,
$$
where $\partial^2$ denotes the Minkowski wave operator. We specialize to
stationary fields where the solution is
\begin{equation}\label{sol}
 \bar{h}_{ab}(x) = 4 \int T_{ab}(x')\frac{1}{|x-x'|} d^3x',
\end{equation}
and the conservation laws imply that (to linear order) the sources must obey
the constraints
\begin{equation}\label{lincon}
  \int J_i d^3x = \int T_{ij} d^3x =0, \qquad \int(x^iJ^k +x^kJ^i)d^3x =0
\end{equation}
where $J^i = T^{it}$ is the momentum density and the indices $i,k$ run
from 1 to 3.
(For instance the last of these follows from  the integration of
$\partial_i(x^i x^k J^l)$ over a bounded source and using
$\partial\cdot J =0$.)\par
The external field of a compact source, at distances large compared to its
dimensions, is thus given by
$$
\bar{h}_{ij}=0,\quad\bar{h}_{tt}= \frac{4m}{r}.
$$
To obtain the gravimagnetic vector-potential $A_i =\bar{h}_{it}= h_{it}$
we expand $|x-x'|^{-1}$ in (\ref{sol}) up to the first order in $x'$
and note (\ref{lincon}). This yields $A_i$ in terms of the source's angular
momentum $L_i$:
\begin{equation}\label{gravpot}
  A_i (x) = 2r^{-3} (x \times L)_i,\qquad L_i = \int (x\times J(x))_i d^3x.
\end{equation}
For an axisymmetric source it is convenient to switch to spherical
polar coordinates, for which
$$
A_i dx^i = -2r^{-3} (L^i x^k\epsilon_{ikl}dx^l) =
-\frac{2ma}{r}\sin^2\theta d\phi,
$$
where we introduced the conventional notation $L_z=ma$. Putting all this
together, we arrive at the standard form of the linearized stationary
exterior metric
$$
ds^2 = (1+\frac{2m}{r})(dx^2 + dy^2 + dz^2) -\frac{4ma}{r}\sin^2\theta
d\phi dt - (1-\frac{2m}{r})dt^2.
$$
To exhibit directly the separate contributions of spin and orbital
angular momentum to the gravimagnetic potential in (\ref{gravpot}),
let us assume the orbital 4-velocity $u^a$ non-relativistic,
so that we can set $u^t\approx 1$ and neglect $u^iu^i$.
To this order we may set
$$
S^{abc}=S^{ab}u^c,\qquad S^{ab}u_b=0,
$$
which implies $S^{it}=S^{ik}u_k$. From (\ref{macein}) we then find to
first order in $u^i$
$$
2U^{itk} = S^{ik} = \epsilon_{ikl}S_l,\qquad \partial_kU^{itk}=\frac{1}{2}
(\partial \times S)^i.
$$
The total momentum current $T^{it}$ in (\ref{macein})
therefore decomposes as
$$
J^i = \rho u^i + \frac{1}{2}(\partial \times S)^i.
$$
Substituting in (\ref{gravpot}) finally yields the expected result
$$
L^i = \int (x \times \rho u)^i d^3x + \int S^i d^3x,
$$
verifying that the angular momentum in vortices contributes in the
same way as orbital angular momentum to the gravimagnetic potential.

\section*{\large\bit 5) A simple example: gravimagnetic field of a single
vortex filament on the axis of a homogenous star}

In order to give a concrete realization of the situation discussed
in the previous sections let us consider the simplest possible model by
taking the superfluid velocity to be the irrotational
azimuthal flow $d\phi$ and assuming the mass-density to be constant
within the star.
The equation for the gravimagnetic potential (within the linearized
theory) become
\begin{equation}\label{gravimag}
*d{*d}A = *d{*F} = j = \theta(a-r) d\phi
\end{equation}
The fact that the ``velocity'' $d\phi$
becomes singular at the axis may be conveniently described by
taking the distributional identity
\begin{equation}\label{domega}
d\phi = \frac{xdy-ydx}{x^2+y^2} =: \omega_\phi \qquad
d\omega_\phi = 2\pi \delta^{(2)}(x) d^2x
\end{equation}
into account, where $\omega_\phi$ denotes the tensor-distribution on
${\rm I\!R}^3$, corresponding to $d\phi$. It is not closed and therefore
certainly not exact. This fact will actually be important in the description
of a vortex filament along the axis of rotation.
Integration of the equation for the gravimagnetic potential
(\ref{gravimag}) yields
\begin{align}\label{field}
 &d{*F}= *j = \theta(a-r)dr\frac{d\theta}{\sin\theta}\nonumber\\
 &{*F}= \omega_0 + \theta(a-r)(r-a)\frac{d\theta}{\sin\theta}
\qquad d\omega_0 =0 \Rightarrow \omega_0=df\nonumber\\
 &F= *df - \theta(a-r)(r-a) drd\phi
\end{align}
where $\omega_0$ denotes an ``integration constant'' (solution
of the homogeneous equation).  Since the second term in (\ref{field})
naively appears to be closed, one might be tempted to discard $\omega_0$.
However, in the light of (\ref{domega}) we find
\begin{align}\label{fil}
&dF=0=d{*d}f + \theta(a-r)(r-a)dr \> 2\pi\delta^{(2)}(x) d^2x,\nonumber\\
&\Delta f = *d{*df} = -2\pi\theta(a-|z|)(|z|-a)\frac{z}{|z|}\delta^{(2)}(x).
\end{align}
This shows that we cannot take $\omega_0$ to be zero,
which would have produced a gravimagentic field of compact support,
namely within the star.
It is precisely the existence of the filament, represented by concentrated
terms in (\ref{fil}), which gives rise to contributions which are not of
compact support
and therefore maybe detected in the far-field. Since our model is
sufficiently idealized it is possible to solve the Laplace-equation
for $f$ exactly.  The calculation is considerably facilitated by
taking a $z$-derivative of $\Delta f$, which simplifies
the inhomogeneity
$$
\Delta \partial_z f = 4\pi a\delta^{(3)}(x) - 2\pi\theta(a-|z|)
\delta^{(2)}(x),
$$
and gives rise to the solution
\begin{align}\label{potential}
  f &= -a \log\left(\frac{z}{\rho} + \sqrt{\frac{z^2}{\rho^2}+1} \right)
- \frac{1}{2}\left[
 (z-a)\log\left(\frac{z-a}{\rho} + \sqrt{\frac{(z-a)^2}{\rho^2}+1} \right)
\right.\nonumber\\
 &- \sqrt{(z-a)^2 + \rho^2}
- (z+a)\log\left(\frac{z+a}{\rho} + \sqrt{\frac{(z+a)^2}{\rho^2}+1} \right)
\nonumber\\
 &\left. + \sqrt{(z+a)^2 + \rho^2}
\right].
\end{align}
Inserting $\omega_0=df$ into (\ref{field}) turns the expression for $F$
into
\begin{align}\label{gravmagfield}
F &= \frac{-a}{\sqrt{\rho^2+z^2}}\left( dz-\frac{z}{\rho^2}\tilde{x}
d\tilde{x} \right) -\frac{1}{2}\left( dz
\log\frac{z-a + \sqrt{(z-a)^2+\rho^2}}{z+a + \sqrt{(z+a)^2+\rho^2}}\right.
\nonumber\\
&\left. + \left(\sqrt{(z+a)^2 + \rho^2}-\sqrt{(z-a)^2+\rho^2)}\right)
\frac{\tilde{x}d\tilde{x}}{\rho^2}\right) - \theta(a-r)(r-a) drd\phi.
\end{align}
Integration of (\ref{gravmagfield}) gives rise to the potential $A$

\begin{align}
A &= \left\{ \frac{\rho^2}{4} \log\frac{z+a + \sqrt{(z+a)^2+\rho^2}}
{z-a + \sqrt{(z-a)^2+\rho^2}} + \frac{z+a}{4} \sqrt{(z+a)^2+\rho^2}
\right.\nonumber\\
&\left. \hspace*{1cm}-\frac{z-a}{4} \sqrt{(z-a)^2+\rho^2} -a r -\frac{1}{2}
\theta(a-r)(a-r)^2  \right \} d\phi
\end{align}
which is not zero in the asymptotic region.

\section*{\large\bit Conclusion}
In this paper we reviewed the influence of spin and orbital angular
momentum of a material system on its gravitational field. Within
the general framework of gravitationally ``polarized'' matter
one can show that both of them contribute to the angular momentum
detected by an asymptotic observer. This investigation settles the
recently discussed issue about the imprint of vortex lines found in
a superfluid neutron star on the asymptotic gravitational field.
Specifically in the linearized approximation of general relativity,
one can obtain an explicit solution which clearly exhibits the
effect of the vortex line on the gravimagnetic potential.
\vfill
\noindent
{\bf Acknowledgement:} We would like to thank George Vlasov for
stimulating correspondence.

\newpage

redpajama_set_name: RedPajamaArXiv


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An index of 4,923 entries containing approximately 1.3 million pages of previously declassified documents, which have been released to NARA is provided. The documents are from the pre-World War I period through the end of World War II.
An index of entries containing over 50,000 pages of declassified documents which have been released to NARA in April 2011 is provided. These documents cover a time frame from before World War I though the 1960s.
The documents listed on this page were located in response to the numerous requests received by NSA on the subject of Unidentified Flying Objects (UFO). In 1980, NSA was involved in Civil Action No. 80-1562, "Citizens Against Unidentified Flying Objects Secrecy v. National Security Agency". Documents related to that ligitation are marked with "*". "XXXXX" has been inserted in a title if a portion of the title has been deleted prior to release. To select a document click on the document title, and wait for the PDF version to be downloaded to your local viewer. Approximate file sizes are given after each selection for user convenience.


integrated content from external sources, such as book covers, reviews, and author biographies.
With version 1.4, a new "collections" feature makes VuFind an excellent choice for a discovery interface for archival and similar collections where information is arranged hierarchically (e.g. fonds, series, item, etc.).
More information about VuFind is available from this page and the VuFind website.
Contact Andornot to discuss how a discovery interface can provide the best search experience and features for your users, no matter what type of information it includes.


Problem This customer was using DC generators and variable speed motors to pump liquid oxygen from their delivery vehicle into their customers' storage tanks. That scenario was proving far too costly to maintain, prompting them to seek an alternate delivery method.
Solution A Nexen M-800 clutch was mounted on a power takeoff from the tank truck's engine. The oxygen pump requires 17-18 hp to operate effectively. The power takeoff easily meets that, developing up to 26 hp at 1200 RPM. Clutch control is from the rear of the truck where there is also a dual throttle control for "revving up" after engagement of the clutch. Four conversions over to the new process took place immediately and others soon followed.
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