COMPARISON OF VLBI NUTATION SERIES WITH THE IAU2000A MODEL Z. MALKIN Institute of Applied Astronomy nab. ... A new Free Core Nutation model with variable amplitude and period (phase) is developed. ... Original differences 200 150 100 50 0 410 420 430 440 450 460 470 480 200 150 100 50 0 410 420 430 440 450 460 470 480 Differences after removing FCN model Figure 5: Spectrum of the differences between observed nutation series and the IAU2000A model, period in days, amplitude in µas. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm03h.pdf -- 235.9 Кб -- 01.03.2015 Похожие документы
Голова Приймально? ком?с?? ... Склад оргком?тету та жур? ол?мп?ад ун?верситету формуються на п?дстав? рекомендац?й факультет?в та затверджу?ться наказом ректора не п?зн?ше 10 березня 2009 року. ... Приймально? ком?с?? не п?зн?ше н?ж за 7 дн?в до початку ол?мп?ади та видаються голов? жур? з в?дпов?дного предмету в день проведення ол?мп?ади. ... Ц? протоколи жур? затверджуються Приймальною ком?с??ю. Результати ол?мп?ади оголошуються не п?зн?ше, н?ж через 10 дн?в п?сля проведення ол?мп?ади. ...
pic] К о н ф е р е н ц и я «Физика плазмы в солнечной системе» 14 - 18 февраля 2011 г., ИКИ РАН ПРОГРАММА ПОНЕДЕЛЬНИК, 14 ФЕВРАЛЯ 2011 г. 09.30-20.00 09.30-10.00 Регистрация. ... СОЛНЦЕ - активные области и магнитные поля Председатель: Обридко В.Н. 12.00 - 12.15 Никольская К.И., Могилевский М.А. О роли магнитных полей Солнца в процессе образования короны и солнечного ветра. ... 17.00 - 17.15 Орешина А.В., Сомов Б.В. Релаксация теплового потока в условиях солнечных вспышек. ...
... 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
... The CCD is back-illuminated and thinned for improved blue sensitivity and provides a quantum efficiency 80% in the wavelength ° range 45007500 A. The unbinned full frame readout time can be as fast as 1.1 s; this is achieved using a low noise amplifier operating at 1 MHz with an average read noise of order 6.9 e RMS. At the slow read rate of 100 KHz to be used for exposure times longer than a few seconds, we determine an average read noise of 3.9 e RMS. ...
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Ссылки http://www.apo.nmsu.edu/arc35m/Instruments/AGILE/Anjum/agile_char.pdf -- 286.8 Кб -- 02.09.2009 Похожие документы
... Testing of the Ground Based VLBI Stations Yevpatoria Simeiz Pushchino of the RadioAstron Mission A. E. Volvacha, V. I. Kostenkoa, M. G. Larionova, L. N. Volvacha, D. M. Muchab, A. S. Nabatovb, A. M ... and A. V. Kovalenkoa a Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia b Institute of Radio Astronomy, National Academy of Sciences of Ukraine, Kharkiv, Ukraine e mail: mgl@asc.rssi.ru Received December 16, 2013 Abstract ... Fig. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/cr_2015,53,209.pdf -- 417.8 Кб -- 09.06.2015 Похожие документы
RT And * CB EA RS 8.97 0.41 0.31 V 0.6289 v 170 000 170 000 F8V+K1 a 231110.1 +530133 SY And SA * EA 10.70 1.50 V 34.9085 060 027 A0+K1 001316.4 +434241 TT And * SA EA 11.50 1.50 0.10 V 2.7651 v 140 000 A+G7IV 231322.9 +460851 TW And * SA EA 8.98 2.06 0.15 V 4.1228 v 130 020 F0V+K0 000318.2 +325045 UU And SA EA 11.20 3.00 0.20 V 1.4863 v 170 000 A8IV/V 004345.1 +305620 WW And * SA EA 10.92 0.67 0.16 V 23.2852 050 000 000 A0:+G5-K0III 234453.5 +454112 WX And SA * EA 12.10 1.70 V 3.0011 d 120 030 F5IV
... We show that broadband energy spectra of GRS 1915+105 during all these spectral states can be adequately presented by two bulk motion Comptonization (BMC) components: a hard component (BMC1, photon index 1 = 1.73.0) with turnover at high energies and soft thermal component (BMC2, 2 = 2.74.2) with characteristic color temperature 1 keV, and the redskewed iron-line (LAOR) component. We also present observable correlations between the index and the normalization of the disk "seed" component. ...
... Programmable minimum/maximum temperature alarm · Indoor/outdoor temperature and humidity in up to 3 remote locations (additional sensors required) · Barometric pressure in imperial or metric units · Altitude adjustment for pressure compensation · 24 hour barometric pressure history chart · Comfort level indicators (Dry, Humid and Comfort) 5 FRONT A B C G H D E F I REAR J K L 6 A. WEATHER FORECAST/ PRESSURE window B ... Press and hold ALARM button until the temperature digits flashing...
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Ссылки http://www.meade.com/manuals/weatherstations/TE636W_Instruction_Manual_031111.pdf -- 837.2 Кб -- 07.11.2011 Похожие документы
R And SiO maser. S And SN (NGC 224). W And SiO maser. Z And Outbursts, average cycle 8400d. Porb = 758.8d, it reveals Z And itself in photometry during the low state. A quasi-period, P1, Z And about 656d is present during the outbursts. The beat period Z And between Porb and P1, about 5500d, is also found in the Z And photometric data. RS And H2O maser. RT And Min II = 9.28. P varies, current elements are given. RU And P varies strongly. RX And Porb = 0.209893d. RY And OH, H2O maser. SS And P2 = 650d, P3 =