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1. Climate Change Research at Armagh
... Kieran Hickey of Armagh Observatory has been testing the link between increased temperatures in North-West Europe and the frequency of storms, as shown in the historical records of climate at Armagh and elsewhere. This is part of an on-going research project at Armagh into the nature of climate change in North-West Europe using long-term meteorological records. ... Some years have significantly more winter storms than others, possibly as a result of the North Atlantic Climate "Seesaw". ...
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Ссылки http://star.arm.ac.uk/press/Climate-Change-Research.html -- 4.4 Кб -- 15.06.2001
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2. lbaops:cdiskohints [ATNF VLBI Wiki]
... You are here: start €Ё lbaops €Ё cdiskohints . ... Check you have write permission to the data disk, e.g: > ls -l /data drwxr-xr-x 2 root root 4096 2006-05-17 04:01 firewire drwxr-xr-x 5 vlbi vlbi 4096 2008-03-28 10:30 internal dтАФтАФтАФ 2 root root 4096 2005-10-28 16:47 removable drwxr-xr-x 5 vlbi vlbi 4096 2008-03-28 21:52 xraid0 drwxr-xr-x 5 vlbi vlbi 4096 2008-03-30 10:15 xraid1 drwxr-xr-x 5 root root 4096 2008-03-30 22:07 xraid2 drwxr-xr-x 5 root root 4096 2008-03-30 22:52 xraid3 . ...
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Ссылки http://www.atnf.csiro.au/vlbi/dokuwiki/doku.php/lbaops/cdiskohints -- 16.2 Кб -- 10.04.2016
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3. East Siberian Center for the Earth's Ionosphere Research. Problems of the IS
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... A most promising problem is to investigate the interaction of two VHF powerful radiowave beams in the ionosphere, whose difference frequency is equal to the plasma frequency in some ionospheric area (that is, the difference frequency is taken in the range 1-8 MHz). ... Two-frequency interaction effects are based on radiowave non-linear mixing, which is rather complicated when describing and modelling the experiment. ...
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Ссылки http://rp.iszf.irk.ru/esceir/isr/theoren.htm -- 5.2 Кб -- 04.06.2001
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4. RESEARCH PROBLEMS of the LRS
... The main research task of the LRS was an investigation of interstellar medium of our Galaxy using its line emission in radio domain with the help of the gratest RATAN-600 Radio Telescope. ... The complex investigation of the Interstellar Clouds structure on the different scales and with the different radio lines for understanding of structure, dynamics and evolution of interstar gas and its interaction with other galactic constituents and the conditions for star formation. ...
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Ссылки http://mavr.sao.ru/hq/lrs/lrssao1.html -- 6.0 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lrs/lrssao1.html -- 6.0 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrs/lrssao1.html -- 6.0 Кб -- 09.04.2016
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lrs/lrssao1.html -- 6.0 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrs/lrssao1.html -- 6.0 Кб -- 09.04.2016
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5. Supernovae
... Supernovae physics (from Wikipedia ): A supernova is a stellar explosion that creates an extremely luminous object that is initially made of plasma ionized form of matter. ... The explosion expels much or all of a star's material at a velocity of up to a tenth the speed of light, driving a shock wave into the surrounding interstellar gas. ... Working on a time series of images in the Large Magellanic Cloud he detected a flaring star, possibly a supernova located in a distant galaxy behind the LMC. ...
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Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/sn/sn.html -- 8.2 Кб -- 02.10.2012
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6. http://www.naic.edu/~phil/obsproblems/lbw1400ripple04/lbw1400ripple.html
There has been ripple in the lband wide bandpass near 1400 Mhz during the a1861 run of may04 and during the a1914 run in aug04. ... The first two sbc were polA, polB at 25Mhz while the last two sbc were polA,polB at 12.5 Mhz. When they observed above 1370 Mhz, the 1320 hipass and 1370 hipass wave guide filters were installed. ... Project a1914 used the 1st two sbc for polA and polB at 25 Mhz. ... Fig 1. (on/off-1) degK vs frequency with offsets for plotting. ... The bumps at 1381 Mhz are gps L3. ...
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Ссылки http://www.naic.edu/~phil/obsproblems/lbw1400ripple04/lbw1400ripple.html -- 4.9 Кб -- 03.08.2004
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7. INTERNATIONAL SPACE STATION
... In the experiment the following physical phenomena are proposed to be demonstrated in microgravity: . ... a series of the experiment sessions with Letauschaya Tarelka device); . ... Faza device; . ... check for the following onboard the ISS RS: a capability to demonstrate the action of physical laws of dynamics of reactive and gyroscopic forces on ellipsoid (Letauschaya Tarelka device) rotating in the unsupported medium in microgravity, with video record of its behavior in the station module; . ...
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Ссылки http://www.energia.ru/eng/iss/researches/education-27.html -- 14.2 Кб -- 02.10.2012
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8. Рекорды и рекордсмены / Азбука астрономии
... Главная Астрономия Фотографии Рекорды Форум Гостевая книга . Азбука . ... Обмен кнопками/баннерами в самом . ... Азбука звездного неба / Рекорды и рекордсмены . ... Самая большая планета . Самая маленькая планета . Самая яркая планета . ... Планета с самым большим количеством лун . Самая большая луна . ... Самая большая группа солнечных пятн . ... Самая большая звезда . ... Самая яркая звезда . Звезда с самой большой светимостью . ... Звезда с самым большим собственным движением . ...
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Ссылки http://www.astro-azbuka.info/records -- 34.5 Кб -- 09.04.2016
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9. Welcom to CONPAS workshop
... Dr. Ravil Nazirov is the head of the workshop, and Andrew Ananjev is the secretary of the workshop. ... The workshop is used to be held in the last decade of the month, preferably on Tuesdays. ... The next session will take place October 29, 1996 . ... There is "CONPAS" mailing list which you can join to discuss issues of problem solving and to be automatically notified of important dates and decisions with respect to the coming sessions. ... Secretary of the Workshop: Andrew Ananjev . ...
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Ссылки http://www.iki.rssi.ru/CONPAS/Welcome.html -- 3.2 Кб -- 13.10.1997
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10. Space Research Institute (IKI) Seminar
... Future seminars . P a s t seminars . ... Stochastic Particle Acceleration and the Problem of Background Plasma Overheating " . D.O. Chernyshov and V.A. Dogiel (P.N.Lebedev Institute of Physics) . ... It was concluded also from these investigations that it is problematic to produce emitting electrons from a background plasma by stochastic (Fermi) acceleration because the energy supplied by external sources in the form of Fermi acceleration is quickly absorbed by background plasma. ...
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Ссылки http://www.iki.rssi.ru/galeev/abs_eng/e120517.htm -- 26.7 Кб -- 18.04.2012
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/galeev/abs_eng/e120517.htm -- 26.7 Кб -- 18.04.2012
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11. Application of the Linear Quadtree to Astronomical Databases
... Quadtrees have a wide range of applications, from graphics to image processing to spatial information systems. ... With the advent of the Guide Star Catalog and other large astronomical source lists, an efficient method of storing and accessing such spatial data is necessary. ... We also discuss how the linear quadtree can aid in the correlation of source positions from different astronomical catalogs and how it can be applied to relational databases. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/barrettp.html -- 12.6 Кб -- 03.11.2000
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12. South Pole Lunar Eclipse
... Credit: Robert Schwarz (South Pole Station) Explanation: The Moon was up continuously for 14 days in August -- when viewed from the South Pole . But during the total lunar eclipse on August 28, it circled only about 10 degrees above the horizon . ... Publications with keywords: south pole - total lunar eclipse - Antarctica . Publications with words: south pole - total lunar eclipse - Antarctica . ... A Total Lunar Eclipse Over North Carolina . ... Landing At The Martian South Pole . ...
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Ссылки http://www.astronet.ru/db/xware/msg/apod/2007-09-07 -- 14.1 Кб -- 07.09.2007
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13. The AstroStat Slog Blog Archive Change Point Problem
... Archives . ... X-ray summer school is on going. ... Recently I went to JSM 2007 and tried to attend talks about (bayesian) change point problems, which frequently appears in time series models, often found in economics. ... Tags: ARCH , Bayesian Block , challenges , change point problem , GARCH , light curves , summer school , X-ray . ... I received another type of changing point problem, defining a peak precisely, from a x-ray school student, who tried bayesian block but said it didn?t work. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2007/change-point-problem/index.html -- 24.5 Кб -- 01.03.2014
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14. Труды Ширмина Г.И.
... научных трудов Ширмина Г.И. ћ Luk'yanov, L. G.; Shirmin, G. I.(2007). Sundman surfaces and Hill stability in the three-body problem. Astronomy Letters, Volume 33, Issue 8, pp.550-561 . ... Astronomy Letters, vol. 29, p. 635-639 . ... Astronomy Letters, vol. 29, p. 274-277 (2003) . ... Astronomy Letters, Volume 28, Issue 6, June 2000, pp. ... Problems of celestial mechanics and stellar dynamics, p. 49 - 53 . ... Lagrangian points in the problem of the search for extraterrestrial civilizations. ...
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Ссылки http://lnfm1.sai.msu.ru/neb/rw/shirm-p.htm -- 13.6 Кб -- 02.04.2012
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15. Astrophysical Research Consortium - Apache Point Observatory
... The ARC echelle spectrograph records the entire visible and near-IR spectrum in one exposure on a 2048 x 2048 SITe CCD chip with 24 micron pixels, with a resolution of 30,000. (2.5 pixels) . ... CCD is a SITe TK2048E back illuminated CCD . CCD is a 2048 x 2048 pixel array . ... Field of View: Available slits (Observing Specialist installable): 1.6" x 1.6" , 1.6" x 3.2" (default), 1.6" x 4.7", 0.9" x 0.9" (pinhole) . ... 31.6 grooves/mm, blaze angle b = 63.5 deg (nominal), or tan b = 2 . ...
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Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Echelle/Echelle_quick_info.html -- 26.3 Кб -- 01.10.2007
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16. Rivi: Magnetic Stars
... Be Stars . ... Magnetic Stars . ... Magnetic fields in stars are common. ... The earliest star known to have a magnetic field is the O-star 1 Ori C, one of trapezium stars in the central cluster of the Orion nebula of spectral type O6. ... The non-existence of more rapidly rotating magnetic stars was thought to be an immediate consequence of the magnetic field: The field would help the star to get rid of angular momentum by forcing the wind into co-rotation, and so to brake down the star. ...
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Ссылки http://www.eso.org/~triviniu/magnetics.php -- 14.1 Кб -- 01.10.2012
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17. http://www.mccme.ru/albio/slides/panteleev.pdf
... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...
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Ссылки http://www.mccme.ru/albio/slides/panteleev.pdf -- 2897.4 Кб -- 09.10.2008
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18. History
... In addition, IZMIRAN comprises the St.Petersburg branch and magnetic ionospheric observatory in Kaliningrad. The history of IZMIRAN is largely that of investigating magnetic storms and sub-storms on the Earth surface, in circum-terrestrial and interplanetary space, initially by means of a network of ground stations of the Soviet Union (1930s - 1940s) and the nonmagnetic skunner "Zarja", then through the extensive use of magnetic measurements on artificial Earth satellites and automatic stations. ...
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Ссылки http://www.izmiran.rssi.ru/info/history -- 12.0 Кб -- 09.04.2016
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19. Institutes of Chernogolovka
... Institutes of Chernogolovka . The largest of all the scientific institutions of the center is the Institute of Chemical Physics in Chernogolovka , where fundamental problems of chemical physics are studied: kinetics and mechanisms of chemical and biological processes; processes of combustion, explosion, and polymerization; and mechanisms of elementary reactions involving high energy particles. ... Developments and Technologies . ...
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Ссылки http://www.issp.ac.ru/univer/inst-s.html -- 10.5 Кб -- 11.04.2001
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20. NEAR recorded on 23 January 1998(frame 1)
Main Sections LabIR main page . ... On January 23, 1998 the space probe NEAR was on its way to its closest approach to Earth. ... However, we were able to record a series of images of the space probe shortly before the sunglint event, and we have assembled them into a movie. At the TIRGO observatory, an observation of the space probe NEAR was organized for the night of January 22-23, 1998. ... We show here a preliminary movie (MPEG format, 412kb) made from 74 frames, each lasting 5 seconds. ...
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Ссылки http://www.arcetri.astro.it/irlab/luna/news/near/near2.php -- 10.2 Кб -- 04.02.2013
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