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Показаны документы, содержащие фрагменты текста из документа
http://www.izmiran.rssi.ru/services/saf/archive/en/2011/obzor20110801.en.txt.

1. http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160321.en.txt
Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 14 - 20.03.2016, Forecast on 21 - 28.03.2016, Carrington Rotations 2174, 2175 (18,17.02; 16,50.03.2016) SUNSPOT-FORMING ACTIVITY OF THE SUN WAS ON THE AVERAGE, AND THE LAST THREE DAYS - ON THE LOW LEVEL. ... FLARE ACTIVITY WAS AT THE LOW LEVEL 15, 16 AND 20.03, AND AT THE VERY LOW -ON OTHER DAYS. ... ACCORDING TO THE CENTER IN BOULDER 14-15.03 WAS REGISTERED. ... ACCORDING TO THE CENTER IN BOULDER AND 6-h. SUBSTORM (G0) TO IZMIRAN DATA. ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/services/saf/archive/en/2016/obzor20160321.en.txt -- 6.3 Кб -- 21.03.2016
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2. Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and
The Special Astrophysical Observatory of the Russian Academy of Sciences will organize a traditional International conference ?Physics and Evolution of Magnetic and Related stars? during the period from August 25 to August 31, 2014. ... evolution of CP and related stars, . ... interplay of pulsations and magnetism in B, A, and F stars, . ... chemical abundance patterns of CP and related stars, . magnetic white dwarfs, . ... Laboratory for the Stellar Magnetism Study of SAO of RAS . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/lizm/conferences/2014/en/index.html -- 5.0 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/lizm/conferences/2014/en/index.html -- 5.0 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/lizm/conferences/2014/en/index.html -- 5.0 Кб -- 10.04.2016
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3. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . This year's annual Geminid meteor shower is active during the period December 7 - 17, with the peak of activity occurring during the night of December 13th/14th. The Geminid shower is currently one of the best of the major annual meteor displays, usually having a high number of relatively bright, medium-speed (130,000 km per hour) shooting stars. ... Last Revised: 2009 December 7th . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/2009/Geminids09.html -- 6.8 Кб -- 07.12.2009
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4. APO Home Page
... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/ -- 13.9 Кб -- 11.02.2016
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5. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Flights Chronology . ... Acquiring new scientific information about the role of the right and the left heart in adaptation of the blood circulation system to long-term space flight conditions. ... Investigation of relations between hemodynamic and energetic characteristics of the heart in different phases of a long-term space flight. ... Data carrier "Cardiovector - Data". ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/en/iss/researches/human/11.html -- 26.8 Кб -- 10.04.2016
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6. ESO - I see unexpected boxy emission-like features in my REDL spectra - where
... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > I see unexpected boxy emission-like features in my REDL spectra - where do they come from? ... Observing with ESO Telescopes . ... ESO-MIDAS . ... ESO Data . ... The pipeline by default interpolates across the bad columns in the REDL CCD when it creates the master bias, but does not so when it processes the science data. This inconsistency can create boxy emission-like features as seen in the figure below. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/sci/data-processing/faq/i-see-boxy-emission-like-features-in-my-redl-spectra-where-do-they-come-from.html -- 23.1 Кб -- 10.04.2016
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7. http://www.stsci.edu/documents/dhb/webvol2/c17_hsperror.fm10.html
... HSP photometric accuracies are strongly dependent on the observational setup and observing conditions, such as spacecraft jitter. Absolute photometry can be done only with a one sigma limiting accuracy of approximately 5%, but relative photometry is possible with an accuracy of 1-2%. Estimated HSP Calibration Accuracies . Absolute Timing . ... Relative Timing . ... 1991 through summer 1993 monotonic decrease, . ... Absolute photometry . ... 5% (one sigma) . ... Relative photometry . ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/webvol2/c17_hsperror.fm10.html -- 4.8 Кб -- 10.02.1998
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8. Archive of International Virtual Observatory Discussions Majordomo List
... About ATNF overview . ... Australia Telescope Steering Committee . ... Staff list | Student list | ... Email discussion lists . ... Murchison Radio-astronomy Observatory . ... Australia Telescope Online Archive (ATOA) . ... Virtual Radio Interferometer . ... Subject : International Virtual Observatory Alliance (IVOA)- . Interoperability Meeting, Pune, September 2004 . ... in Virtual Observatory (VO) related activities. ... as a part of the activities of the Virtual Observatory-India (VO-I) . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/lists/ivo/2004/06/0051.html -- 33.2 Кб -- 10.04.2016
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9. http://www.wdcb.ru/stp/data/solar.act/sunspot/sunspot.txt
RELATIVE SUNSPOT NUMBERS Description of Data from SGD Explanation of Data Reports: Relative Sunspot Numbers -- The relative sunspot number is an index of the activity of the entire visible disk of the Sun. ... The provisional daily Zurich relative sunspot numbers, Rz, were based upon observations made at Zurich and its two branch stations in Arosa and Locarno and communicated by M. Waldmeier of the Swiss Federal Observatory. ... This indicates the uncertainty above and below the predicted number. ...
[ Сохраненная копия ]  Ссылки http://www.wdcb.ru/stp/data/solar.act/sunspot/sunspot.txt -- 5.2 Кб -- 18.01.2010
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10. http://www.naic.edu/vscience/schedule/2014Spring/BradfordtagA2850.pdf
... Proposal Type: General Category: Observation Category: Time Requested this semester: Hours Next Semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time: Expected Data Storage: Prop osal Title: ABSTRACT: Regular Astronomy Extragalactic 22 10 3 hours less than 100 GB The Baryonic Content of Extremely Low Mass Galaxies We propose continued HI observations of low mass galaxies to better quantify the galaxy mass function. ...
[ Текст ]  Ссылки http://www.naic.edu/vscience/schedule/2014Spring/BradfordtagA2850.pdf -- 56.6 Кб -- 06.09.2013
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11. Geomagnetic Indices Kp, ap, Ap, Cp and C9
This service contributes to the International Service of Geomagnetic Indices (ISGI) of the IAGA . ... The Kp numbers of the previous month are available in tabular format . ... There are available also historical and current Kp and derived indices per anonoymos FTP (see below). ... U.S.A. FTP server: ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/ . monthly update) . ... contains the monthly Kp / ap tables in a simple text format readable for both humans and computers (*.tab). ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/index.html -- 13.1 Кб -- 14.10.2001
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12. Period Criteria
... Actual stars are expected to be more complicated than these simulations. ... The spot may be entirely visible most of the time (one would observe a prolonged flux minimum low), and then part of it may disappear over the horizon briefly and then return (slow rise and then fall back to constant level). ... With the set of observations taken here, I have information available from several comparison stars and color information. ... The period found must be consistent with the data from any given night....
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~swolk/thesis/period/node9.html -- 7.2 Кб -- 02.10.2012
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13. SSAU international relations
... Pre-university education . ... SSAU History . ... International relations . ... Thus, in different years the University entered into agreements with the universities of China (Harbin Politechnical Institute, Beijing Aerospace University , Beijing Politechnical University , North-West Politechnical University , Bradley University (USA), Sofia Technical University (Bulgaria), Stuttgart Technical University (Germany), Berlin Technical University (Germany), Carlow Technical ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/english/international/ -- 27.3 Кб -- 10.04.2015
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14. Pulkovo Observatory
. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.
[ Сохраненная копия ]  Ссылки http://www.gao.spb.ru/ -- 4.5 Кб -- 06.04.2009
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15. http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf
... A star was observed at different zenith distances during one night at the Engelgardt's Astronomical Observatory in the program of atmospheric extinction study at blue. ... The determination of the star's brightness was performed with the method of photon counting. ... Variable star. ... The brightness of the variable star was measured occasionally during the other nights, and moments of maximal values of brightness (15.59m) were received on nights 2­5, the 2nd table. ... JD 2452805. ...
[ Текст ]  Ссылки http://www.issp.ac.ru/iao/2015/booklet/b10_ia15_p_en_a.pdf -- 173.2 Кб -- 03.12.2015
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16. Radioastrophysical Observatory ISTP RAS SB
RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . 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 Publication SSRT - Siberian Solar Radio Telescope . ...
[ Сохраненная копия ]  Ссылки http://ssrt.iszf.irk.ru/rad11en.shtml -- 17.2 Кб -- 27.02.2014
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17. Science Innovations
. Сайт временно не работает.
[ Сохраненная копия ]  Ссылки http://www.sai.crimea.ua/ -- 1.9 Кб -- 17.05.2015
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18. XWare > APOD
... Henrietta Leavitt Calibrates the Stars . ... X Ray Moon . ... This x-ray image of the Moon was made by the orbiting ROSAT (R ntgensatellit) Observatory in 1990. ... SOHO, the space-based SOlar and Heliospheric Observatory, has become by far the reigning champion facility for discovering comets, its total having recently reached 200. ... Full Throttle For Deep Space 1 . ... The bright stars above are well known as heart of the Trapezium, an open cluster of stars in the center of the Orion Nebula. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/apod.html?page=89&d=2003-01 -- 15.3 Кб -- 12.04.2016
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19. http://www.sao.ru/cats/~satr/RFSymp/abs/08_Doroshenko.ps
CONTINUUM AND BROAD EMISSION LINE VARIABILITY OF SEYFERT GALAXIES V.T. Doroshenko 1,2 , S.G. Sergeev 2 , V.I. Pronik 2 1 Crimean Lab. of the Sternberg Astronomical Institute, Moscow University, Russia 2 Scientific­Research Institute, Crimean Astrophysical Observatory, Ukraine; p/o Nauchny, 98409, Crimea, Ukraine vdorosh@sai.crimea.ua We focused on the observed properties of some Seyfert galaxies without detailed discussion of underlying physical mechanisms. ...
[ Текст ]  Ссылки http://www.sao.ru/cats/~satr/RFSymp/abs/08_Doroshenko.ps -- 89.8 Кб -- 09.10.2006
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20. The culmination of the solar eclipse coincided with the strongest magnetic
... The storm began quite unexpectedly. The strongest geomagnetic storm for the last seven months began on Earth almost precisely at the same time as the solar eclipse reached its maximal stage, the culmination of which occurred at GMT 02:35 (06:35 Moscow time). ... Oscillations of such amplitude in the magnetic field have not been observed since October, 11th of last year, which is more than seven months ago. ... We can only add that the magnetic storm lasted approximately 9 hours. ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/info/tesis_20090723_en.php -- 11.2 Кб -- 01.10.2012
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