Vertical Structure of the Galactic Disk in the Solar Neighborhood . ... It was found that the Sun lies 9?2 pc above the plane of hte Galactic disk in the direction of North Galactic pole and that F0-F9 stars contribute 0.0035M /pc 3 to the density of the Galactic disk. ... THE DENSITY OF F STARS IN THE PLANE OF THE DISK љљљљљSince our sample is comlete to within 50 , the Z obs distributions shown in Fig.2 make it possible to determine the number of F stars per unit volume of the Galactic disk. ...

Surveys in Geophysics (2005) 26: 95­133 DOI 10.1007/s10712-005-1874-4 с Springer 2005 MAGNETOSHEATH INTERACTION WITH THE HIGH LATITUDE MAGNETOPAUSE S. SAVIN1, A. SKALSKY1, L. ZELENYI1, L. AVANOV1, N. BORODKOVA1, S. KLIMOV1, V. LUTSENKO1, E. PANOV1, S. ROMANOV1, V. SMIRNOV1, YU. YERMOLAEV1, P. SONG2, E. AMATA3, G. CONSOLINI3, T. A. FRITZ4, J. BUECHNER5, B. NIKUTOWSKI5, J. BLECKI6, C. FARRUGIA7, N. MAYNARD8, J. PICKETT9, J. A. SAUVAUD10, J. L. RAUCH11, J. G. TROTIGNON11, Y. KHOTYAINTSEV12 and K. STASIEWICZ12

... How can I participate in AAAP to elevate my own interests and contribute in a way that helps advance the club and the future of amateur astronomy? ... Well known to AAAP from her significant role with the Sloan Digital Sky Survey in which Princeton is a key player, Dr. Knapp will speak to us about her research on Brown Dwarfs. ... 2003 ­ A Year of Progress in AAAP Reflecting back over the past year, I am struck by the contributions of many members which continue to solidify our club. ...

The possibility of recovery of the vertical distribution of the magnetic field in umbrae by line width differences S.G. Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru Abstract. This article studies the possibility of recovery of the vertical distribution of the magnetic field in the photospheric layers of sunspot umbra by the Difference of the Line profile Absolute Widths of neutral zirconium ? ... 2) Line profiles for cold models have extended wings. ...

ABSTRACTS 10-th International Gamow Summer School "Astronomy and beyond: Astrophysics, Cosmology and Gravitation, Cosmomicrophysics, Radio-astronomy and Astrobiology" (Ukraine, Odessa, Chernomorka, 23-28 August, 2010) MEMORIAL SESSION SERGEY ALEKSANDROVICH SNEGOV (1910-1994) ­ OUSTANDING PHYSICIST, COSMOLOGIST, ASTRONOMER AND WRITER ­ VISIONARY TO A 100-ANNIVERSARY FROM BIRTHDAY Pahomov A.G. PFUM, Moscow It is possible to judge a condition of an astronomical science on literary works of time. ...

Plasma (from Greek plasma- modeled, formed) is a gas with high ionization where the concentrations of positive and negative charges are equal (quasineutrality). ... The high temperature plasma (T~10^B - 10^8R) from the deuterium and tritium is investigated for thermonuclear controlled synthesis. The low temperature plasma (TS 10^5K) is used in different gas discharged devices (gas lasers, plasma generators, plasma engines and others). Back . ...

... Next Routine] [List of Routines] NAME: ADD_HEADER PURPOSE: addition information from FITS-headers MPFS-frames DESCRIPTION: The function computes the total exposure, mean value zenit distance and modified FITS header CALLING SEQUENCE: Result =ADD_HEADER( headers ) CATEGORY: reduction MPFS-data INPUTS: Headers = String array FITS-headers from the MPFS data OUTPUTS: Header = String array containing the header from the FITS file. ... OPTIONAL INPUT KEYWORD PARAMETERS: BEFORE = Keyword string name. ...

... Tte tables of ionosphere and plasmasphere parameters are contained in a file param.tbl. ... Latitude Longitude Numbers of tables for (degree) (degree) Month Wm=10 Wm=100 Wm= 150 80 30 March 1 - 3 397-399 793-795 80 150 March 4 - 6 400-402 796-798 80 270 March 7 - 9 403-405 799-801 60 30 March 10 - 12 406-408 802-804 60 150 March 13 - 15 409-411 805-807 60 270 March 16 - 18 412-414 808-810 40 30 March 19 - 21 415-417 811-813 40 150 March 22 - 24 418-420 814-816 40 270 ...

... An Electronic Version of Volume I of the General Catalogue of Variable Stars with Improved Coordinates N. N. Samus'1,2 , * , V. P. Goranskii2 , O. V. Durlevich2 , A. V. Zharova2 , E. V. Kazarovets1 , E. N. Pastukhova1, M. L. Hazen3 , and T. M. Tsvetkova Institute of Astronomy, Russian Academy of Sciences, ul. ... Subsequently, we are planning to publish new versions of the GCVS Volumes II and III, as well as of the catalog of suspected variable stars (the NSV catalog). ... Stars, No. ... Stars Obs. ...

... Астрософт (Модератор: tlgleonid ) > . IRAF: установки и использование . ... Ответ #20 : 21 Январь 2011, 11:20:39 ? Цитата: d_w от 21 Январь 2011, 11:12:54 Олег, а можно пункт 4 по-подробнее? ... Записан . ... Error while reading login.cl file - may need to rebuild with mkiraf . ... Последнее редактирование: 21 Январь 2011, 17:30:31 от d_w ? ... Цитата: d_w от 22 Январь 2011, 00:34:12 Монтируем образ, из-под любого юзверя в консоли sudo -s . ... Цитата: Олег Малый от 22 Январь 2011, 13:07:55 . ...

Supernovae 2011by in NGC 3972 . This page is devoted to information on Supernova 2011by in NGC 3972 . ... vsnet-campaign-sn 1055] nearby SN Ia 2011by . vsnet-campaign-sn 1058] nearby SN Ia 2011by . ... Polish Society of Amateur Astronomers 2011by page . ... 2011/04/25.947 . ... 2011/04/26.823 . ... 2011/04/26.855 . ... 2011/04/27 . ... 2011/04/27.332 . ... 2011/04/27.913 . ... 2011/04/27.937 . ... Joel Nicolas . ... JM Llapasset . ... Marc Serrau . ... Back to Bright Supernovae - 2011 . ...

Sternberg astronomical institute activities on site testing programs review Victor Kornilov comprehensive/characterization/of/astronomical/sites > kislovodsk/russia/2010/october/4-9 > Introduction This presentation responds on our activity in 5 last years only, inspite of that in SAI site testing researches have been started many years ago. ... More detailed discussion is devoted to MASS and DIMM measurements processing, some additional effects which were taken in account in last year. ...

... Здесь собраны функции, необходимые для работы программы. #ifndef VIGG0_H #define VIGG0_H int FindMatrix( string InputString, string SearchString1, string SearchString2); void Invert ( string In); void ComplementaryStr( string In); void Swap( string objA, string objB); class Integer_Node { int Node_handles; Integer_Node * Node_next ; public: Integer_Node( int new_carry): Node_handles(new_carry), ... NO=0)\t"; cin>>ComplementScanActive; cout<<"Want new locus scan start signal? ...

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