... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...

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• Celestial Mechanics
• Practice in Astrophysics
• WARNING MISSION: Background

... ARTICLE: The Adventurous Search For The Astronomical Unit . ... Kepler himself had suggested to use the rare occasions of Venus transiting (crossing) the solar disk to measure our distance to the planet. ... Due to the orbital inclination of Venus against the ecliptic of 3.5°, a Venus transit is so rare that it happens only at intervals of 121.5 years, 8 years, 105.5 years, 8 years and so on. ... Crabtree witnessing the transit of Venus 1639 . ... Transits of Venus - The Quest for the Solar Parallax...

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... We publish 16 Doppler imaging temperature maps for the years 1994-2002 of the active RS CVn star II Peg. ... Through Doppler imaging we want to study the spot evolution of the star and in particular compare this with previous results showing a cyclic spot behaviour and persistent active longitudes. ... The derived temperature maps are quite similar to the ones obtained earlier with a different methods, the main differences occurring in the spot latitudes and relative strength of the spot structures....

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... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...

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• http://selena.sai.msu.ru/Bus/Publications/SSR-11(Busarev).pdf
• http://selena.sai.msu.ru/Symposium/ant.doc
• http://selena.sai.msu.ru/Symposium/ant.pdf

Measurement of Sky Brightness at the Iranian National Observatory Davoud Afshari1 and Sadollah Nasiri1,2 1Physics Department, Zanjan University, Zanjan 45195-313, Iran; Institute for Advanced studies in Basic Science (IASBS), Zanjan 45195-1159, Iran; Measurement of light pollution 2 Introduction Among 34 candidate sites at the central part of the country, 5 sites namely Garkesh (in Kashan ), Kolahbarfi(in Kashan ), Deynava (in ... One of these is light pollution. ...

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Stellarium 0.12.3 . ... Classes . ... SpaceShipObserver Class Reference . An observer which moves from from one position to another one and/or from one planet to another one. ... SpaceShipObserver (const StelLocation &startLoc, const StelLocation &target, double transitSeconds=1.f) . ... Get whether the life of this observer is over, and therefore that it should be changed to the next one provided by the getNextObserver() method. ... Get the next observer to use once the life of this one is over. ...

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• Stellarium: gSatWrapper Class Reference
• Stellarium: ScreenImage Class Reference
• Stellarium: StelObject Class Reference

WIDE-BAND STUDY OF X-RAY PULSARS WITH SUZAKU T. Enoto1 , R. Miyawaki1 , M. Kokubun1 , K. Makishima1 , Y. Terada2 , T. Mihara2 , M. Nakajima2 , M. Suzuki2 , A. Bamba2 , A. Senda2 ... Department of Physics, Kanazawa University 11 Department of Technology, Miyazaki Univerity 1 7 ABSTRACT A summary is given on the timing accuracy verifications of the Hard X-ray Detector ( HXD ) on board the Suzaku satellite ... Key words: Suzaku, HXD, Crab pulsar, PSR1509-58, A0535+26,. ...

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• http://hea.iki.rssi.ru/integral06/papers/G06_Tsygankov01-22Jan07_11:45:59.pdf
• http://hea.iki.rssi.ru/conf/hea2010/Presentations/24/Titarchuk.pdf
• Second Spectrum-RG/eROSITA Conference

Электронная библиотека астронома-любителя. ... архив RSN . ... Ru.Space.News: . Апрель 1998 . ... Дата: 30 апреля 1998 (1998-04-30) От: Alexander Bondugin Тема: MGS Views Mars Pathfinder Landing Site Привет всем! ... Дата: 30 апреля 1998 (1998-04-30) От: Alexander Bondugin Тема: Surprises from SOHO include tornadoes on the Sun [1/2] Привет всем! ... Дата: 30 апреля 1998 (1998-04-30) От: Alexander Bondugin Тема: Mars Global Surveyor Prepares To Enter Solar Conjunction Period Привет всем! ...

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• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 07 мая...
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 14 февраля
• Электронная библиотека астронома-любителя. RU.SPACE.NEWS - архив за 24 марта

The most up-to-date information related to atmos 3.0 are collected here due to constantly increasing interest to MASS/DIMM processing software... atmos 3.0 is still beta , so the latest version is 2.97.5 (there is also 2.98.x branch which absorbs new features) . ... M' line: . ... free seeing and its relative error . ... dimm seeing and its relative error (if dimm data are present, zeros otherwise) . ... dimm turbulence power and its relative error (if dimm data are present, zeros otherwise) . ...

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... 8 February , 2014 SAI seminar (Ryde et al 2010) 5 Thermal emission from GRB jet progenitor observer photon jet Photosphere (=1) · · · · Photons are not produced at the photosphere We have to calculate radiative transfer We need to know where the photons are produced We construct the expression for effective optical depth in relativistic flow considering random walk process in relativistic flow SAI seminar 6 8 ... 8 February, 2014 SAI seminar 28 ...

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• http://master.sai.msu.ru/static/YaB_100/20/Khlopov.pdf

... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...

33. LX200 repairs

34. http://solarwind.cosmos.ru/txt/2011/presentations/Magnetosphere/Bespalov.pdf

35. Спец.выпуск N5 (октябрь, 1999).

36. Solar Physics Department

37. Space Scientific and Education project of Lomonosov Moscow State University

38. The Observer: российские и американские ученые создали космическую яхту с

39. http://vega.inp.nsk.su/~inest/startest.doc

40. The Sunspot Observer - About authors