... Сегодня: 10 апреля 2016 г. Сегодня 10 сентября в Японии на космодроме Йосинобу на острове Танегасима должен состояться запуск ракеты H-2A. Старт назначен на 21:20 по местному времени (12:20 мск), длительность окна запуска составляет 30 минут. ... Через 14 минут после запуска первым от ракеты должен отделиться спутник USERS. ... Спутник DRTS должен отделиться от второй ступени ракеты через 15 минут после USERS. ... Сегодня должна стартовать японская ракета H-2A . ...
Материалы по солнечной физике. ... SunWorld - комплекс для моделирования образования профилей Стокса фраунгоферовых линий . arXiv Sci-Hub (поиск по DOI) Solar abstracts (by Rutten) ссылки ARBIB поиск ALBERT . ... книги по астрономия, астрофизике на ph4s.ru . ... Solar Physics wiki Прием рукописей . ... Solar Influences Data Analysis Center (SIDC, Royal Observatory of Belgium) . ... 6-12 сентября 2015, КрАО. ... 24 сентября 2012, ГАО. 16-я всероссийская ежегодная конференция по физике Солнца . ...
The Second U.S. Naval Observatory CCD Astrograph Catalog ( UCAC2 ) Table of Contents 1) Introduction 2) Summary of the Project a) Observations and Instrumentation b) Reductions of UCAC Observations c) Computation of Proper Motions 3) Properties of the Catalog and Important Notes For the User a) Sky Coverage b) Completeness c) Positions, Proper Motions and Error Calculations d) UCAC2 Magnitudes e) 2MASS Photometry f) Non-stellar ... All stars in the UCAC2 have proper motions. ...
program kom; {$APPTYPE CONSOLE} uses SysUtils; const n_t =20; //кол-во городов n_os =50; //кол-во особей v_mut=1; //вероятность мутации для каждой особи(в %) v_cross=60;//вероятность скрещивания для каждой пары особей(в %) max=10; //максимальное расстояние между городами type TTowns=array[1.. n_t ,1.. n_t ]of byte; //массив, описывающий расстояния между городами TOsobi=array[1.. n_os +1,1.. n_t ]of byte; //массив хромосом var ...
Polycyclic aromatic hydrocarbons in HII regions: correlation with metallicity . ... We have perfomed the aperture photometry of HII regions using infrared images from telescopes Spitzer and Herschel at passbands 3.6, 4.5, 5.8, 8.0, 24, 70 and 160 m. Emission of PAHs are observed at passbands 3.6 - 8.0 m, 24 m is emission likely of hot small particles and finally large particles are responsible for emission at 70 and 160 m. We determine abundances of PAHs using model of Draine Li (2007) . ...
... 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. ...
RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... SSRT - Receiving systems . The SSRT has two independent receiving systems for recording solar observational data, and several ancillary receivers for checking, setting up and adjusting the instrument. The base receiving systen is a multichannel filter receiver for a simultaneous recording in 180 channels with the 500 kHz band each, adjusted at steps of about 600 kHz. ... Channel's band . ...
... Using the CFBDSIR wide field survey for brown dwarfs, we identified CFBDSIRJ214947.2-040308.9, a late T dwarf with atypically red J-Ks colour. ... SN 2009ip in NGC 7259 Electronic Telegram No. ... 7.09, [19.0; 2009 Aug. ... Accepted for publication in MNRAS Subjects: High Energy Astrophysical Phenomena (astro-ph.HE) The jet opening angle theta_jet and the bulk Lorentz factor Gamma_0 are crucial parameters for the computation of the energetics of Gamma Ray Bursts (GRBs). ...
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Ссылки http://master.sai.msu.ru/media/presentations/2012/arXiv05oct12_1.doc -- 81.0 Кб -- 07.10.2012 Похожие документы
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