... In electron-positron colliders, effect of the lattice modification by opposing bunch focusing on the equilibrium radiation emittance is important at high values of the space charge parameter, so one should correctly evaluate this dynamic radiation emittance of the weak beam, which may differ a lot from the nominal emittance, already in the linear beam-beam force model. ... The linearized beam-beam force is equivalent to focusing insertion in linear lattice of the collider. ...

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• http://vega.inp.nsk.su/~inest/astrolib/Sun/kursoviki/lines-c/lines.aux
• http://vega.inp.nsk.su/~inest/astrolib/zemax_rus.pdf
• http://vega.inp.nsk.su/~inest/PulnixTM1300.pdf

Elsevier Ed itorial System(tm) for JASR 2006 Manuscript Draft Manuscript Number: Title: Determination of K, Ar, Cl, S, Si and Al flare abundances from RESIK soft X-ray spectra Article Type: Contributed Paper Section/Category: E2.4 - Solar Magnetic Field and Activities Keywords: solar physics; X-ray flares ; spectroscopy; abundances Corresponding Author: Dr. J. Sylwester , Corresponding Author's Institution: Space Research Center First Author: J ... All flares were observed early Fig. ...

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• http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf

... Bad Astronomy . ... On Thursday, February 15th 2001 (and replayed on March 19), the Fox TV network aired a program called ``Conspiracy Theory: Did We Land on the Moon?'', hosted by X-Files actor Mitch Pileggi. ... Dust around the lander . ... However, it appeals to our common sense: when the sky is black here on Earth, we see stars. ... Bad: The program claims that when the top half of the lander took off from the Moon to bring the astronauts back into orbit, there was no flame from the rocket. ...

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• Phil Plait's Bad Astronomy: Mad Science
• Phil Plait's Bad Astronomy: Misconceptions

... Spacecraft that will search for planetary systems around 40 million stars and observe the largest explosions in the universe have been chosen as the next two missions in NASA's medium-class Explorer (MIDEX) program. ... The first mission, to be launched in 2003, is the Swift Gamma Ray Burst Explorer, a three-telescope space observatory for studying gamma ray bursts. ... During its three-year mission, Swift will also survey the sky for new black holes and other sources of cosmic gamma rays. ...

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• ПРИЛОЖЕНИЕ ј2 к Выпуску N2(16), март-апрель 1998

ПЕРЕЛ?К ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО . ... 2011 . ... Comets,Asteroids, Meteors, Meteorites, Astroblemes Craters" (CAMMAC 2011), Memorial International Conference, Vinnytsia, Ukraine, Sept. 18-23, 2011: Book of Selected Papers and Abstracts . ... Чол?й В.Я. Жаборовський В.П. П?дсистема визначення поправок програмного пакету Ки?в- Геодинам?ка++ . ... Укр. центру визначення параметр?в обертання Земл?/ ... В.Я. Чол?й. - К.: ВА?ТЕ . ... Медведський М.М. Укра?нська мережа ЛЛС у 2011 роц?: ...

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• Aspherical optics
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... Using the uvby -photometry and proper motion data for about 5500 F stars within 80 pc from the Sun, we have studied velocity ellipsoid parameters and obtained the following results. 1) The sizw of all wllipsoid semiaxes increase systematically for groups of stars with the decrease of both temperature (at constant metallicity) and metallicity (at constant temperature). ... As a result, each of the three parameters - temperature, metallicity and velocity dispersion - is an age indicator. ...

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• Anomalous Absorption Theory
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. + Auto-translation from russian . + Регистрация пользователей . + Вход в Астротоп + Напомнить пароль + Блог + ЗАРЯ + Exit . Уважаемый Гость ! . Напомнить пароль . Ваш логин: пароль: Can't execute (SELECT name FROM groups WHERE id= ) in astrotop database: ОШИБКА: ошибка синтаксиса (примерное положение: ")") LINE 1: (SELECT name FROM groups WHERE id= ) ^

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• AstroTop-100 - обработка результатов опроса

... MHz time of max Peak Mean UT UT Min. (10 -22w/m 2 Hz) 05.04 2804 40 F 00.14.3 00.14.7 1.2 4.7 11.04 2804 40 F 01.56.3 01.56.4 4.1 8.5 20.04 2804 40 F 01.33.3 01.33.8 1.3 6.0 26.04 2804 2 S/F 03.46.5 03.47.6 3.1 6.8 26.04 2804 1 S 04.07.6 04.08.3 1.3 3.5 27.04 2804 1 S 03.29.1 03.29.6 1.0 4.0 28.04 2804 3 S 23.28.1 23.30.7 9.0 46.4 30.04 2804 42 SER 01.35.7 01.42.0 8.3 21.8 30.04 2804 42 SER ...

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• http://www.uafo.ru/tables/bursts/2007_burst.txt
• http://www.uafo.ru/tables/bursts/2008_burst.txt
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