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http://www.stsci.edu/hst/wfc3/analysis/grism_obs/calibrations/wfc3_grism_master_sky.html.

21. http://www.winer.org/Logs/NightLog-2014-10-26.txt
Date: 10/26/2014 Time:06:02 Moon Age: 2.4 Available Observing Hours: 12.2 Observer: Instrument: Operator: Cage: Lebofsky and Crawfor 90PrimeOne Trueblood PF hours lost to: weather: 0.0 telescope: 0.0 instrument: 0.0 computer: 0.0 Time Temp Humidity Wind Vel. Wind Dir. Seeing Open 01:10 17.7 64 N/A N/A 1.0" Close 12:50 15.6 74 N/A N/A 1.3" _________________ Description ______________________ Seeing often 1.1". N/A above is due to Weatherhawk's being down. Able to observe 10 objects.
[ Сохраненная копия ]  Ссылки http://www.winer.org/Logs/NightLog-2014-10-26.txt -- 1.7 Кб -- 02.12.2014
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22. The Wind Spacecraft
The Wind spacecraft. ... It was designed to observe the solar wind approaching Earth, from a position near the Lagrangian point L1, and it is part of the International Solar-Terrestrial Physics (ISTP) Initiative . ... The original plan called for "Wind" to approach its final station over two years, undergoing two close encounters with the Moon to boost its speed. ... For additional details and updates, see the home page of the "Wind" mission. Exploration" home page (index) Glossary . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wwind.html -- 7.4 Кб -- 15.03.1999
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23. http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf
... Galaxies 99 Cosmic background with model of cloudy interstellar medium Yu. ... Figure 1: Averaged spectrum of the cosmic background I f in frequency range 0.25 200 MHz for the Galactic poles. ... First interpretation of the cosmic noise background spectrum at broad band frequency range 0.25 200 MHz with a model of the cloudy interstellar medium ISM is presented here. ... Synthesized background spectra I f for regions of the Galactic poles at the frequency range 0.25 200 MHz is presented in Fig. ...
[ Текст ]  Ссылки http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf -- 100.3 Кб -- 21.05.2007
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24. Near IR Astronomy with the ESO VLT
Next: CONICA: The high resolution Up: VLT Status and Instruments Previous: VLT First Light . ... Infrared instruments for the VLT . Instrument Summary . ... The already approved infrared instruments for the VLT are: . ... CONICA: Coude Near Infrared Camera (P.I. R. Lenzen, MPIA, Heidelberg) - an historical name as this instrument will be used for diffraction limited 1-5 m imaging, polarimetry and spectroscopy with the NAOS, Nasmyth Adaptive Optics System on UT1 (P.I. G. Rousset, ONERA ). ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node6.html -- 17.8 Кб -- 12.06.2006
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25. MAO NASU :: Topic: Fw: ASTRONET: Task 5.4 - observing schools (1/1)
... Recent Topics . ... MAO main . ... Fw: ASTRONET: Task 5.4 - observing schools . ... Subject: Re: ASTRONET: Task 5.4 - observing schools . ... with the organization and carrying out observing schools. ... second half of September, and which will be funded by the training and . ... intended for master and starting PhD students. ... actions on observing schools, providing access for students, Master . ... observing schools for master students. ... in form of observing schools for pre-PhD students. ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/index.php/ua/forum/info/154-fw-astronet-task-5-4-observing-schools -- 23.0 Кб -- 11.04.2016
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26. Curiosity observe de nouvelles traces dтАЩeau | Ciel et Espace
... Recherche dans le site : . Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualit†йs . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil Curiosity observe de nouvelles traces dтАЩeau . ... Sur Mars, Curiosity vient de mettre en †йvidence des veines de gypse, un min†йral hydrat†й, incrust†йes dans de la roche. ...
[ Сохраненная копия ]  Ссылки http://www.cieletespace.fr/node/10004 -- 30.3 Кб -- 09.04.2016
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27. Warbling Chirplet: Analysis of Signals of Oscillating Frequency
Next: CONCLUSION Up: CHIRPLET TRANSFORM SUBSPACES Previous: Nondilational Chirplet Transform . Suppose we choose a windowed sinusoidal FM signal for our mother chirplet. Such a signal has a frequency that periodically rises and falls (much like the vibrato of musical instruments or the wail of a police siren). ... Figure 14 . ... Using the warbling mother chirplet, we also computed the ``dilation-dilation'' ( ) plane of the chirplet transform (Fig. 16 ) for the pendulum data. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Chirplet.dir/node23.html -- 11.9 Кб -- 15.04.1998
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28. Iowa Robotic Telescope Facilities
... Iowa Robotic Telescope | ... Talon is based on OCAAS, a software suite developed by software engineer Elwood Downey ( Clear Sky Institute ) for use at the University of Iowa ?s first remote facility (the ATF, or Automated Telescope Facility). ... XObservatory : Telescope Control Interface . ... This program calls upon and coordinates much of the interrelated portions of the Talon architecture, and forms the primary control panel for the telescope, dome, and peripheral systems when used locally. ...
[ Сохраненная копия ]  Ссылки http://vega.inp.nsk.su/~inest/Talon(OCAAS)/Iowa%20Robotic%20Telescope%20Facilities.htm -- 37.9 Кб -- 25.01.2006
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29. (Untitled)
... For each observed position the table contains designation of object as in file of observations, the time of observation, the number and name/ preliminary designation of minor planet supposedly identical with observed object, the values of O – C (observed position minus computed one) in right ascension and declination expressed in arcsec, the difference O – C between observed magnitude and computed one, the code of observatory in the Observatory list (see Observatories section). ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user248j.htm -- 2.3 Кб -- 10.04.2016
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30. ASP: Education Newswire
... In a report on a recent information technology conference at Columbia University (Chronicle of Higher Education, 16 January 1998, p. A25), questions are raised with respect to the efficacy of computers in the classroom. ... The Summer Science Program is once again being held at The Thacher School in Ojai, California. ... The Consortium for Undergraduate Research and Education in Astronomy announces the Mount Wilson Summer Program for Undergraduates, August 12-25, 1998. ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/pubs/mercury/9802/m_a98.html -- 12.5 Кб -- 02.10.2012
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31. Mars mission team addressing vacuum leak on key science instrument |
... SUN MOON MERCURY VENUS MARS, JUPITER SATURN . ... Mars . ... Mars mission team addressing vacuum leak on key science instrument . ... A key science instrument that will be carried aboard NASA's Interior Exploration Using Seismic Investigations, Geodesy and Heat Transport (InSight) spacecraft being prepared for launch in March 2016 is experiencing a leak in the vacuum container carrying its main sensors. ... Only registered members of Astronomy.com are allowed to comment on this article. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/news/2015/12/mars-mission-team-addressing-vacuum-leak-on-key-science-instrument -- 68.5 Кб -- 10.04.2016
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32. http://www.cplire.ru/html/lab234/pubs/2011_07a.pdf
Operating of the superconducting integrated receiver channel of the TELIS atmospheric sounder. ... The noise temperature of the SIR was measured to be as low as 120 K, with an intermediate frequency band of 4 ­ 8 GHz in double sideband operation; the spectral resolution is well below 1 MHz. The SIR was implemented in the three-channel balloon-borne instrument TELIS (TErahertz and submillimeter LImb Sounder) that detects spectral emission lines of stratospheric trace gases (like ClO and BrO). ...
[ Текст ]  Ссылки http://www.cplire.ru/html/lab234/pubs/2011_07a.pdf -- 819.5 Кб -- 09.09.2011
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33. Galactic Gravitational Wave Background
Next: Extragalactic Gravitational Wave Background Previous: Transparency of the Stochastic . Let the sky be observed with a detector having a pencil beam diagram across. The number of stars per frequency decade that is swept by the detector is a function of celestial coordinates (say, galactic coordinates l , b ): . ... It is clear from the figure that for an all-sky detector the Galaxy becomes transparent above the frequency  Hz. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node82.html -- 10.0 Кб -- 04.03.1997
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34. Astro-2 and the UIT Experiment
We report here on those proposed UIT targets that, in fact, were successfully acquired. ... Note on Filters: . A1 centered at 2500 angstroms with a width of 1200 angstroms . ... NGC 2300 is in a small group of galaxies which has a substantial amount of X-ray emission. ... LUNA again for 777 through lots of filters. ... Supernova 1987A in the Large Magellanic Cloud was observed for 3740 seconds through B5, A1 and B1. ... NGC 5128 or Cen A was observed for 1454 seconds through the B1 filter. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/uit-t11.html -- 4.6 Кб -- 07.10.1996
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35. ON THE STRUCTURE OF 3.11.94 ECLIPSE CORONA
We present the results of our observations of the white-light corona in polarized light performed at Criciuma eclipse, Brazil. During the observation of 3.11.94 we have made five couple of pictures of the solar corona in polarization light. ... Koutchmy S., Molodensky M., Starkova L., Ershov A., Matsuura O .: ... Molodensky M., Starkova L., Koutchmy S., Ershov A .: ... Koutchmy S., Molodensky M.M., Starkova L.I . ... Koutchmy S., Molodensky M.M., Starkova L.I. Koutvitsky V. and Ershov A . ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/info/personalia/molodensky/Eclips94.htm -- 6.4 Кб -- 20.11.2009
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36. http://www.jsc.nasa.gov/history/oral_histories/SmithEE/SmithEE_Bio.pdf
EMERY E. SMITH, JR. ... Engineering, Christian Brothers College, Memphis, Tennessee (1964) Masters of Science in Electrical Engineering, University of Houston , Houston , Texas (1968) PRE-NASA EXPERIENCE: · U.S. Corps of Engineers NASA EXPERIENCE: NASA Manned Spacecraft Center /Lyndon B. Johnson Space Center , Houston , TX (19641996) · Aerospace Engineer , Support Planning Section, Flight Control Operations Branch , Flight Control Division (1964) · ... ECT E. E. Smith, Jr., ...
[ Текст ]  Ссылки http://www.jsc.nasa.gov/history/oral_histories/SmithEE/SmithEE_Bio.pdf -- 30.6 Кб -- 16.06.2006
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37. StarCalc Home Page [English]
Russian version of HP . ... StarCalc is the fastest professional astronomy planetarium & star mapping program for Windows 9x/ME/NT/2000/XP (StarCalc version for PocketPC computers you can found here ). ... Extensibility : This program is based on common "Plugin StarCalc interface to catalogs and object groups", which allows program to add new modules as Plugins. ... Welcome to the Pocket StarCalc Home Page: . ... Some bugfixes in eclipses" and line" plugins - see the new versions in downloads page. ...
[ Сохраненная копия ]  Ссылки http://www.m31.spb.ru/StarCalc/ -- 12.1 Кб -- 27.12.2004
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38. Amateur Telescope Makers of Boston
... The Amateur Telescope Makers of Boston, Inc. ATMoB) is an amateur astronomy club devoted to telescope making, observing, and studying the heavens. ... In 1973, the Bond Astronomical Society, another long-standing club, merged with the ATMoB making the club one of the oldest and largest general interest astronomy clubs in the country. ... The Amateur Telescope Makers of Boston, Inc. is an IRS designated 501(c)3 public charity organization. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
[ Сохраненная копия ]  Ссылки http://www.atmob.org/about/default.php -- 7.5 Кб -- 09.04.2016
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39. Laboratory of spectroscopy of defect structures ISSP RAS
... DLTS . ... Deep Level Transient Spectroscopy ( DLTS ) is a unique and powerful tool for the study of electrically active defects (known as traps) in semiconductors. DLTS can be used in one of two modes of operation; with Schottky diodes or with p-n junctions. ... The capacitance transient is measured as a function of temperature (usually in the range from liquid nitrogen temperature to room temperature 300K or above). ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lsds/en/methods/dlts.html -- 5.4 Кб -- 10.04.2016
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40. Light Curve Templete/Observing Form For Visual SNe Observers.
... The following charts/text are intended as tools for monitoring the Type Ia supernovae ( SNe ) event visually or photographically (utilizing telescope equipped CCD equipment).The files include: A replication of The Type Ia SNe , V- magnitude (with data point checks from other cited references)and color index (B-V) templete (to indicate a general color-related trend of the type Ia ... I believe this might help alleviate some of the problems involving the making of acceptable amateur light curves...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/mirrors/isn/snecurv.htm -- 8.3 Кб -- 02.02.2012
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