National Aeronautics and Space Administration . ... Story Musgrave (M.D.) . NASA Astronaut (Former) . ... Service Medal and an Outstanding Unit Citation as a member of the United States Marine Corps Squadron VMA-212 (1954); United States Air Force Post-doctoral Fellowship (1965-1966); National Heart Institute Post-doctoral Fellowship (1966-1967); Reese Air Force Base Commander's Trophy (1969); American College of Surgeons I.S. Ravdin Lecture (1973); NASA Exceptional Service Medals (1974 ...

... Show Times . ... Armagh Planetarium has a range of shows suitable for all the family. ... Due to the darkness and sound levels some shows are only suitable for children of six years and above. ... Please check the show descriptions (see below) for age ranges. ... AGE restrictions apply: NO ENTRY FOR CHILDREN UNDER SIX YEARS OLD . ... Live presenter-led show : Duration 25 mins . ... Specially produced by Armagh Planetarium, 'The Little Yellow Star' is a new show aimed at pre-school aged children. ...

NOTE: The storm sudden commencement data file was updated on 18 Feb 1998. o Revised data for 1968-1975 were taken from IAGA Bulletin No. ... Indices aa and storm sudden commencements"; see also IAGA Bulletin 39: " Supplementary Geomagnetic Data 1957-1975", including a new list of ssc's 1968-1975). ... From the monthly reports of Rapid Variations prepared by 43 magnetic observatories (see list page 121), a combined list of all events is compiled. ...

Isabel Leonor University of Oregon searched 25 S2 GRBs for coincident G-waves of duration ~1 ­ 10 ms used crosscorrelation method explored data conditioning in the frequency domain, included whitening and phase correction ­ luxury of limited on-source and off-source data to analyze injected signals to study sensitivity of pipeline used playground data with no GRB trigger data analysis code (standalone), injection and calibration scripts, written using Matlab ...

... Seminar archive . ... 30 min. ... Липунов В. М. ( МГУ, ГАИШ МГУ ) . ... Горбовской Е. С. ( ГАИШ МГУ, от группы МАСТЕР ) . Тюрина Н. В. ( ГАИШ МГУ ) . ... Руденко В. Н. ( ГАИШ МГУ ) . ... Пустовойт В. И. Download presentation . Липунов В. М. Download presentation . ... А.В.Тутуков(ИНАСАН), Л.Р.Юнгельсон, А.М.Черепащук (ГАИШ МГУ), Н.С.Кардашев, И.Д.Новиков, В.Н.Лукаш, А.Г.Дорошкевич (АКЦ ФИАН), А.Ф.Захаров (ИТФ), Г.С.Бисноватый-Коган (ИКИ), М.Е.Прохоров, К.А.Постнов (ГАИШ МГУ) , . ...

... Tonight's Sky . ... Some long-duration gamma-ray bursts are driven by magnetars . ... GAMMA-RAY BURSTS | ... This artist s impression shows a supernova and associated gamma-ray burst driven by a rapidly spinning neutron star with a strong magnetic field an exotic object known as a magnetar. ... The results show that the supernova following the burst GRB 111209A was not driven by radioactive decay, as expected, but was instead powered by the decaying super-strong magnetic fields around a magnetar. ...

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

... All angular values are expressed in degrees. ... But those who have the facilities for high-speed photometry could try to observe these phenomena. h m ° ° ° ° 2016 April 1 18 51.0 84.9 57.4 345 20 168378 1997 ET30; 17.8 ; 1.7 km; 7.2; 0.47s 18 58.0 67.3 45.6 325 26 U2 027489793 ; 10.6;14h06m06.171s;-12°01'21.53 19 05.0 49.6 38.1 307 22 2016 April 10 22 10.4 106.6 -31.2 311 75 297274 1996 SK; 20.3; 1.7 km; ...

Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Irvin M. Winer . ... Roof Status . ... Winer . ... Status . ... Roof State . ... 2016.04.09 16:10:02 . ... Roof closed at 2016.04.09 16:10:02 . Roof Position . ... Weather State . ... 0D:21H:11M:24S . ... Roof Control (Software) . ... 29D:21H:27M:33S . ... Roof Control (Hardware) . ... 29D:21H:27M:34S . ... Roof UPS State . ... GPS State . Engineering Page Winer Graphical Data Server Page(s) . ... 2013 Winer Observatory. ...

... What is the notion time? ... Generally speaking, it is an order of changing events, an order of constantly changing conditions of solids, Universe - being. ... The time, determined for the given longitude, is called the local time . ... A uniform system of time counting - ephemeris time is tested by observations of the Moon turning around the Earth. Fully independent from astronomic observation uniform system of the time counting is based on the concept of atomic second (see quantum watches ). ...

... The OC "Mir" orbit parametres before the final burns . ... Orbit period (in min) . ... Mean orbit altitude (km) . ... solar F 10.7 flux . ... F 10.7 <= 100 - low level; 100 < F 10.7 < 150 - medium level; F 10.7 >= 150 - high level . Orbit 86328(15) - the first burn bulding the descent orbit  D V 1 =9.3 m/s. After burn altitude H min = 188.2 km, H max = 219.2 km. Orbit 86329(16) - the descent orbit second impulse D V 2 =10.4 m/s. After burn altitude H min = 158.9 km, H max = 218.5 km. ...

... Within the transnational Access program of SOLARNET, European investigators can apply for observing time with the European instruments IBIS and ROSA , which are installed at the Dunn Solar Telescope of the US National Solar Observatory ( DST/NSO ). ... Periodic calls for proposals will be published for requesting SOLARNET observing time with the European instruments IBIS and ROSA, installed at the Dunn Solar Telescope of the US National Solar Observatory (DST/NSO). ... SOLARNET Access . ...

. €а . ETHOS 1 . €а . €а . €а . €а . €а . Narrow-band images of 300 second duration each were obtained with the FORS2 instrument attached to ESOтАЩs Very Large Telescope in Paranal, Chile, on 19 June 2010 (H Alpha+83 - red, OIII+50 - green, and OII+44 filters - blue). The full TIFF file is here . Credit and Copyright: B. Miszalski, R. Corradi, H. Boffin et al. Very Large Telescope image of ETHOS 1 . Back to main page . This page created by Henri Boffin on 15 December 2010. €а . €а

... In most cases it will however be necessary to compute an appropriate airmass using the COMPUTE/AIRMASS . ... It is important to keep in mind that ``mean airmass'' and ``mean atmospheric extinction correction'' are different from the values at mid-exposure, especially for larger zenith distances. ... For reasonable combinations of exposure time and zenith distance, the weighted mean airmass supplied by COMPUTE/AIRMASS should be appropriate. ...

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

... Total solar eclipse 2008 live from Novosibirsk On August 1, 2008, a total solar eclipse was being visible in Russia. ... The solar eclipse in Novosibirsk started at 9h41m UT and finished at 11h45m UT. ... Special Astrophysical Observatory of RAS eclipse expedition team made 3 channels live Web-cast of the eclipse from Novosibirsk in collaboration with . ... Total phase . ... It's preferably to install on computer VLC media player free program for Web-cast live receiving. ...

... The 11 th International Astronomy Olympiad has been held successfully in Bombay (Mumbai) on November 10-19, 2006. The duration of the Olympiad was 10 days, it is one day longer than usualy. ... The International Astronomy Olympiad has been held in Europe and Caucasus for nine times, the X IAO visited East Asia, and now it is the first time IAO coming to South Asia. ... Friday, November 10 - Day of arrival . ... Dr. Michael G. Gavrilov, Founding Chairman of the International Astronomy Olympiad, . ...

It could be that SETI signals have arrived at the Earth, but are lower then the noise level, and our receivers cannot detect them. ... Fig. ... It follows that two zones form around the star with civilization X: "Zone Yes", where its SETI signal can be detected, and "Zone No", where its signals are hidden by noise (Fig. ... In practice, it is more efficient to use a time factor, since the problem of SETI contact does not limit the duration of the signal element and semantic text. ...

A computer controlled low light photometer for nightglow observations. Hardware units of portable photometer for low light measurements, especially night glow emission is described. ... Interface card contain three channels of 24 bit counter, 4 channels of 12 bit ADC and the buffer bus for the controlled motors of the altazimuthal fork mounting and filters wheel, the position encoders. ... Where N( ) is output signal photometer generated input light flux F( l ) . ... PMT # . 599 . ...

Location: Zelenogorsk Prepared: 01 JUN 2002 Satellite Name: ISS Catalog Number: 25544 98067A Pass Type: Visible, MinAlt = 5 deg, MinHor = 3 deg -----------AOS----------- --MAX VISIBILITY-- ------LOS------ # LCL Date Time Azm LCL Time Alt Azm LCL Time Azm Duration 1 01 JUN 02 23:15:07 250.7 23:20:10 35 174.3 23:25:11 98.5 0:10:04 VIS : 23:15:52 248.6 23:20:09 35 175.4 23:24:29 100.5 0:08:37 2 02 ...