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41. http://www.iki.rssi.ru/comp/2015/Chur_obzor.pdf
Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational appearance and physical models of plasma structures in clusters of galaxies. ... The knowledge of the complex dynamical and feedback processes is necessary to understand the energy and matter balance as well as to constrain the role of the non-thermal components of clusters. ...
[ Текст ]  Ссылки http://www.iki.rssi.ru/comp/2015/Chur_obzor.pdf -- 59.9 Кб -- 02.11.2015
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42. IESP-2M Results Page
. An example of ULF electromagnetic fields detection by the IESP-2M instrument. The figure presented is the dynamic spectrogram. E and B components are measured in satellite coordinates. Observations were made in the auroral region. Electromagnetic turbulence, which was observed mostly in electric components, is typical for this phenomenon. Fig.1 .
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/auroral/iesp2m.htm -- 2.0 Кб -- 26.11.1996
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/auroral/iesp2m.htm -- 2.0 Кб -- 26.11.1996
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43. http://ip.rsu.ru/~vorobyov/project2.htm
. -!> download . Left: Consequtive explosion of 20 supernovae during 30 Myr. Right: Single hypernova (GRB) explosion with the total energy equivalent to 20 supernovae. The simulation was performed using a 2D Eulerian hydro code. The animation was done using IDL. -!>
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~vorobyov/project2.htm -- 3.9 Кб -- 27.09.2007
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44. http://www.ipa.nw.ru/conference/2002/sovet/PS/MELNIKOV.PS
... Lightcurves of two satellites of Saturn, namely Hyperion (S7) and Phoebe (S9), were modeled using algorithms and programs developed for calculat­ ing the rotational dynamics and constructing theoretical lightcurves of planetary satellites. ... The problem of fitting an observed lightcurve with the model one is solved by varying the initial data and values of the parameters of the problem. ... The value of the MLCE calculated for the deduced initial data and values of the parameters is close to zero....
[ Текст ]  Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/MELNIKOV.PS -- 28.9 Кб -- 19.08.2002
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45. http://www.wro.org/scodova/observations.html
... Observations . Objects . ... Canis Major . ... Canis Minor . ... Leo . ... Leo Minor . ... Ursa Major . ... Ursa Minor . ... Herschel 2500 . ... Herschel 400 (I) . ... Globular Clusters . ... AL Globular Club . ... AL Planetary Club . ...
[ Сохраненная копия ]  Ссылки http://www.wro.org/scodova/observations.html -- 38.5 Кб -- 03.12.2012
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46. Data bases of Natural Satellites. Documentation. Structure
Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/DocStructe.htm -- 11.4 Кб -- 18.05.2009
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