... Future seminars . P a s t seminars . Seminar council . Ultra-High Energy Cosmic Rays: status of the problem " . ... There are several puzzles Ultra-High Energy Cosmic Ray (UHECR) experimental data. ... Situation with Grezen-Zatsepin-Kuzmin cutoff (break in UHECR proton spectrum due to interaction with CMBR) is experimentally unclear. In this talk I'll review existing UHECR experiments and present their results, future experiments and their possibilities. ...

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• Институт космических исследований РАН (ИКИ РАН)
• Multipoint correlations of the solar wind parameters observed by several

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Peremennye Zvezdy", . ... V435 Cas, GSC 4011-01257, . ... V435 Cas was discovered as a variable star by Hoffmeister (1967). ... Six more times of minima were published by Rosino, Bianchini di Martino (1976); despite that, the period of V435 Cas could not be determined. ... These observations are available via the OMC Data Server (Gutierrez et al., ... Rosino, Bianchini, di Martino, 1976 . ... INTEGRAL/OMC data Times of minima of V435 Cas . ... A POSS-II red image centered on V435 Cas. ...

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... В четверг, 14 апреля 2016 г., состоится семинар кафедры астрофизики. Повестка дня . ... Начало в 11 час.15 мин. Ауд. ... В четверг, 31 марта 2016 г., состоится семинар кафедры астрофизики . ... В четверг, 24 марта 2016 г. , состоится семинар кафедры. ... В четверг, 17 марта 2016 г. , состоится заседание кафедры. ... ОСП НИИ ПММ Национального исследовательского Томского государственного университета) . ... Copyright 2016 Астрономия в Санкт-Петербургском университете . ...

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• The Stellar Content and Distance to the Nearby Blue Compact Dwarf Galaxy
• Linear polarization: wavelength dependence
• Wavelength dependence

Solar Eruptive Event of 4 November 2001 observed with the SPIRIT Telescope on Board the CORONAS-F Satellite . ... Based on the data of the SPIRIT telescope on board the CORONAS-F satellite in three EUV channels 175, 284, 304 , we have analyzed large-scale manifestations of the post-eruptive so-lar activity followed one of the most considerable and geoeffective coronal mass ejection (CME) in the 23rd cycle which occurred on 4 November 2001. ... Posteruptive arcade on the CORONAS-F/SPIRIT movies at . ...

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• Soft X-ray Class of Far-Side Flares
• Space weather and ecology

... Tonight's Sky . ... Observing . ... Sky this Month . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Open cluster NGC 2818, spiral galaxy NGC 2964, and spiral galaxy NGC 2976 . ... Astronomy for Kids . ... Sky Guide . ... Observing springtime deep-sky objects with a large telescope . ... University of Hawaii at Manoa's Institute for Astronomy, Honolulu . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email...

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• Max Planck Institute for Astronomy, Heidelberg, Germany | Astronomy.com
• Planetary Science Institute, Tucson, Arizona | Astronomy.com
• Max Planck Institute for Gravitational Physics, Hannover, Germany |

... Photometric standard stars will be interspersed between science stars. ... INSTRUMENT: SurveyCam FILTERS: VRI COMMENTS: Here is the status of nights so far for this project: program nts backup nts total wipeouts 2014-JUL/AUG/SEP 2 3 12 2014-OCT/NOV/DEC 2 1 4 2015-JAN/FEB/MAR - - - 2015-APR/MAY/JUN 4 7 3 2015-JUL/AUG/SEP - - - 2015-OCT/NOV/DEC 3 2 2 2016-JAN/FEB/MAR 2 5 - TOTAL 13 18 21 program nts = used for primary photometric program backup nts = used for backup ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS03.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_oct2015/AS09.html
• ARCSAT Proposal Coverpage

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... The results of radio observations of GRB 080319B in the spectral range of 8.45 GHz are presented. ... Key words: Gamma­rays ­ bursts: observations ­ radio: individual: GRB 080319B 1 Intro duction Gamma­ray bursts (GRBs) are the most luminous explosions currently known in the Universe. ... Smooth angular scanning was used not only in GRB 080319B observations, but to specify the primary standard source radio flux density as well (Kharinov et al., ...

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• Galaxy sector, archive 2008
• Ratan-600 schedule archive
• The GLORIA Project makes available to internet users 13 robotic telescopes in

... About ATNF overview . ... Australia Telescope Steering Committee . ... LMC H II Region Luminosities versus . Observed Ionizing Stars . ... These values are compared to the observed H II region luminosities, yielding an estimate for the mean fraction of H-ionizing photons that escape the local nebulae in this sample. We formally estimate that, overall, 0-51% of the ionizing radiation escapes the local H II regions and is available to ionize the warm, ionized medium in the LMC. ...

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• A page of useful links
• The observed distribution
• Source size measurement from observed quasar microlensing

... About: Dr. Antonov was born in Ryazan in 1950; graduated in Solis State Physics from the Faculty of General and Applied Physics of Moscow Institute of Physics and Technology in 1973; got a PhD degree in 1977 and the degree of Doctor of Sciences from the Institute of Solid State Physics RAS in 1985. ... 1973 – 1975 Probational Researcher, ISSP RAS, Chernogolovka . ... 2003 – present Head of the Laboratory of High-Pressure Physics, ISSP RAS, Chernogolovka . ... LHPP ISSP RAS © 2004 All rights reserved...

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• XI International Astronomy Olympiad
• Igor V.Kukushkin

... 13th European VLBI Network Symposium . and Users Meeting . on September 20-23, 2016. ... 13th European VLBI Network Symposium and Users Meeting on September 20-23, 2016. ... Year book "Ephemerides of Minor Planets for 2016" on-line . ...

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• Keywords_120

... The low energy plasma composition spectrometer AMEI-2 is built to be able to find in the low energy range of the phase space (E, q, j) and separate the fluxes of the major ion species in the magnetotail - H+, He++, He+ and O+, and analyse their energy and angular distributions. ... Electrostatic angular scanning in one direction and the use of the spin of the satellite to sample the other angle give the ability to measure 2-D distributions for each ion specie several times per spin. ...

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• Space Research Institute (IKI) Seminar
• DA Retrieval Service
• Spacecraft Observing the Sun and the Heavens above

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Research results on fast active processes General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Distribution of the recorded spikes in duration . ...

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THE PARAMETERS INVOLVED IN HAPKE'S MODEL FOR ESTIMATION OF THE COMPOSITION OF THE EJECTA LUNAR TERRAINS. ... In the previous papers we were estimated the surface roughness of the ejecta lunar terrains by means comparison of the local phase function and the average integrated lunar indicatrix. ... The Hapke's theoretical model of the lunar surface reflection. ... For THE PARAMETERS INVOLVED IN HAPKE'S MODEL: S.G. Pugacheva, V.V. Shevchenko a low-albedo lunar surface parameter Bo = 1. ...

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• http://selena.sai.msu.ru/Shev/Publications/ms38/ms084.pdf
• http://selena.sai.msu.ru/Ber/Publications/ms40/88_Yamashita%20et_al.pdf
• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf

... 77, 1995 R. A. Shaw, H. E. Payne, and J. J. E. Hayes, eds. Simulation of HST PSFs using Tiny Tim J. Krist Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218 Abstract. ... The most recent ver­ sion, V4.0, includes new mirror zonal error maps and revised aberrations, significantly improving the PSF models. ... Introduction Tiny Tim is a stand­alone program for simulating HST PSFs as viewed with the on­board imaging cameras (WF/PC­1, WFPC2, FOC, COSTAR/FOC). ...

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• Simulation of HST PSFs using Tiny Tim
• Electronic Submission of HST Phase I Observing Proposals
• A Distributed System for ``Phase II'' Proposal Preparation

... Frequency of wobble same as frequency of forcing mechanism (t) + i 2 (t) · Helmholtz Centre Potsdam ­ GFZ · Consistent estimates of AAM , OAM , HAM computed at GFZ · AAM computed from European Centre for Medium-Range Weather Forecasts · OAM computed from Ocean Model for Circulation and Tides (OMCT) · HAM computed from Land-Surface Discharge Model (LSDM) · Ocean and hydrology Sensitivity to Excitation Model GFZ ECMWF AAM OMCT OAM LSDM HAM 1962­2010 1971­2010 1981­2010 1991­2010 2001­2010! ...

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• http://www.gao.spb.ru/english/publ-s/viii-rfs/p099.pdf
• Pulkovo NEO Page: Estimation of Accuracy of the Observations

Reports from around the world indicate that this year's annual Perseid meteor shower was the best display since the 1990s. The accuracy of the calculations by Jeremie Vaubaillon (Institute of Celestial Mechanics, Paris and California Institute of Technology) a frequent collaborator with Armagh astronomers, and the American astronomer Thomas van Flandern regarding the times of peak activity and numbers of meteors observed, were confirmed by observations. ... See also: Perseid 2009 Videos . ...

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• Solar Eclipse Observed Armagh Observatory
• Broadening of Si VIII lines observed in the Solar polar coronal holes
• Armagh Observatory

... The TRACE images may be used without restrictions in publications of any kind. ... These two images, taken on 18 November 2000 at 15:54UT and 16:11UT, respectively, show such an event: the red circle in the image to the left shows a region where many loops are cooling, with bright loop tops (the intensity scales with the square root of the image to reduce the dynamic range). ... See also a collection of images related to the Sun, other cool stars, and solar-terrestrial effects . ... Images | ...

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• New Moons of Uranus
• CHIANTI atomic database
• Cannibal Stars Cause Giant Explosions in Fornax Cluster Galaxy (ESO Press

... Science Users Information > Science and Technical Meetings > Conferences 2010 > The Origin and Fate of the Sun: Evolution of Solar-mass Stars Observed with High Angular Resolution . ... Observing Facilities . ... Observing with ESO Telescopes . ... The goal of this workshop is to review recent results on solar-mass stars obtained with infrared and millimeter interferometers, and to discuss their importance for our understanding of stellar evolution from star formation to stellar end products. ...

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• ESO - LISA Conferences
• ESO - Swedish Heterodyne Facility Instrument Science Verification
• Curriculum Vitae