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21. P/2010 V1-F (Ikeya-Murakami) _ PK10V01f - фрагмент Ф (component F)
Общая Астрономическая Конференция > Практика > Астрономический наблюдательно-информационный портал > Хвостатые гостьи (все о кометах) > P/2010 V1-F (Ikeya-Murakami) _ PK10V01f - фрагмент Ф (component F) периодической кометы P/2015 Y2 (Ikeya-Murakami) = P/2010 V1 (Ikeya-Murakami) = 332P/Ikeya-Murakami .. ... Просмотр полной версии : P/2010 V1-F (Ikeya-Murakami) _ PK10V01f - фрагмент Ф (component F) периодической кометы P/2015 Y2 (Ikeya-Murakami) = P/2010 V1 (Ikeya-Murakami) = 332P/Ikeya-Murakami .. ...
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Ссылки http://www.starlab.ru/archive/index.php/t-28712.html -- 7.4 Кб -- 10.04.2016
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22. PINTofALE EXAMPLE : Simulation for Chandra ACIS-I
... This thread uses PINTofALE to generate a simulated Chandra spectrum. ... define a DEM . ... pset marx .par ExposureTime=50000 OutputDir='sim_ marx ' \ ; GratingType='NONE' DetectorType=' ACIS-I ' SourceFlux=-1 \ ; SpectrumType='FILE' SpectrumFile='spec_ marx .dat' \ ; SourceType='POINT' DitherModel='INTERNAL' ; marx TSTART=2006.46 ; marx2fits sim_ marx / spec_ marx .evt ; dmextract infile= spec_ marx .evt[EVENTS][(x,y)=circle(4018,4141,10)] ; [bin pi=1:1024:1] outfile= spec_ ...
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Ссылки http://hea-www.harvard.edu/PINTofALE/doc/EXAMPLE_Chandra.html -- 11.5 Кб -- 01.10.2012
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23. Basic definitions [Oulu]
spaceweb@oulu.fi - last update: 1 July 1998, 1200 UT (RR) . ... Relates the wave number k to the wave frequency. ... From the equation of motion , m d v /dt = q( v x B ) one can calculate that, in a presence of magnetic field B , a charged particle is accelerated in direction perpendicular to both v (perp) and B . ... The angle a between magnetic field B and velocity vector of a charged particle, v ., i.e., sin a = v(perp) / v(total), where v(perp) refers to the velocity component perpendicular to B . ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/basics.html -- 6.8 Кб -- 21.12.2007
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24. HT-45LU Trinocular Observation Head
... LUMAM . ... HOME . ... MICROSCOPES . ... CAMERAS . ... Home Products Microscopes Lumam HT-45LU Trinocular Observation Head . HT-45LU TRINOCULAR HEAD . ... Every trinocular LUMAM includes three vertical adapters: the VA-V20LU focusing C-mount adapter for attachment of C-mount video/digital cameras, the VA-F20LU photo adapter for 35mm cameras – with adapter rings for cameras that accept T-mount, Pentax or C-mount lenses, and the VA-T1LU telescoping DIN standard eyepiece tube adapter (23.2mm). ...
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Ссылки http://www.lomoplc.com/trinocular_head_ht_45lu.htm -- 10.9 Кб -- 09.04.2016
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25. Fundamentals of Mechanics
.
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Ссылки http://zebu.uoregon.edu/1995/ph161/l4.html -- 4.4 Кб -- 06.10.1997
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26. The Catalogue of Interacting Galaxies by Vorontsov-Velyaminov
... Sternberg Astronomical Institute , Moscow University . ... Present edition unites two parts of Catalogue of interacting galaxies by B.A.Vorontsov-Velyaminov: the first part (Part 1) containing 355 systems was published in 1959 [1] and the second one (Part 2) with 497 objects - in 1976 [2].Thus two published parts of Catalogue include 852 interacting systems. ... All new of them (1162 by number) were taken from the comments to the galaxies in Morphological catalogue by Vorontsov-Velyaminov et al.[ ...
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27. ScrollbarWithLabel (ImageJ API)
... Class . ... java.lang.Object java.awt.Component java.awt.Container java.awt.Panel ij.gui.ScrollbarWithLabel . All Implemented Interfaces: . ... public class ScrollbarWithLabel . ... ScrollbarWithLabel ( StackWindow stackWindow, int value, int visible, int minimum, int maximum, java.lang.String label) . ... void . ... int . ... public ScrollbarWithLabel ( StackWindow stackWindow, int value, int visible, int minimum, int maximum, java.lang.String label) . ... public void setBlockIncrement (int b) . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/gui/ScrollbarWithLabel.html -- 34.0 Кб -- 02.12.2010
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28. Ronbun (Abstract)
... We present the results of an interferometric and single-dish study of G24.78+0.08, a region associated with high-mass star formation. ... We suggest that the embedded stars might be too young to have affected the surrounding molecular cloud significantly on a large scale. ... We assess that the (proto)stellar cluster lies at the center of a molecular clump with diameter of ~2 pc: to a good approximation this may be described as a spherically symmetric clump with density profile of the type n~R^(-1.8...
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Ссылки http://www.arcetri.astro.it/~lt/preprints/ronbun/abstract.html -- 3.0 Кб -- 11.09.2007
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29. Stellar Astronomy
... Subject and Problems of Stellar Astronomy. ... Plane of Galaxy, Methods of Its Location Determination. ... Stars Distances. ... Other Methods of Stars Distances Determination. ... Tangential Velocities, Their Determination by Self-Motions. ... Determination of Solar Apex and Spatial Velocity by Radial and Spatial Velocities of Stars. ... Features of Orientation and Parameters of Peculiar Stellar Velocities Ellipsoid. ... General and Selective Light Absorption in Galaxy. ... Darc Clouds in Galaxy. ...
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Ссылки http://space.univ.kiev.ua/courses/zor_astron_e.html -- 8.0 Кб -- 23.02.2005
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30. RAS ISR' Conclusion on the scientific results received in the orbital complex
... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...
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Ссылки http://www.cosmoworld.ru/mirstation/english/documents/iki_ran_280998.shtml -- 11.0 Кб -- 09.04.2016
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31. IESP-2M Results Page
. An example of ULF electromagnetic fields detection by the IESP-2M instrument. The figure presented is the dynamic spectrogram. E and B components are measured in satellite coordinates. Observations were made in the auroral region. Electromagnetic turbulence, which was observed mostly in electric components, is typical for this phenomenon. Fig.1 .
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Ссылки http://www.iki.rssi.ru/auroral/iesp2m.htm -- 2.0 Кб -- 26.11.1996
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/auroral/iesp2m.htm -- 2.0 Кб -- 26.11.1996
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/auroral/iesp2m.htm -- 2.0 Кб -- 26.11.1996
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32. October-November 2003
... Extreme strong microwave S-component (F10.7 cm) -- enhanced emission in strong magnetic fields of the transition region and low corona; thermal and nonthermal components; . Extreme strong metric-wavelength noise storm -- permanent particle acceleration in strong evolving coronal magnetic fields; . CME/flare-associated events: intense metric emission (type II/IV bursts) and predominated post-eruptive microwave component; . ...
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Ссылки http://www.izmiran.rssi.ru/~ichertok/Radio_Oct03/conclud%20.html -- 2.8 Кб -- 30.06.2004
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33. RadioAstron Monthly Notices
... a) assembling and tuning of printing-circuit boards for the Test-set device and assembling of the Test-set device itself; . ... Engineering models of the On-board Rubidium Frequency Standard (ORFS-SRT) and Space Radio Telescope On-board Heterodyne and Clock Frequencies Synthesizer set (OHCFS-SRT) were packed and delivered to LA to be assembled with the SRT in the Device Container. ... FC Focal Container – hermetic package with the scientific payload; it contains receivers, . ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/archives/2003/month_notic/may.html -- 22.7 Кб -- 03.11.2011
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34. The Laboratory of Astrometry
... Observatory . ... The Laboratory of Astrometry . Dept. for Physics of Stars&Galaxies . ... Astronomical Calendar . ... UkrVO . ... The purpose of research: Creating a stellar catalog to study the structure and kinematics of star systems, including open star clusters and stars with large proper motions; the enhancement ICRF / Hipparcos system to stars dawn to 17 m (V); Search of binary systems of brown dwarfs and determination of their parameters; astrometry of minor bodies of the Solar System. ...
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Ссылки http://www.mao.kiev.ua/index.php/en/observatory/departments/astrometrylab -- 20.7 Кб -- 10.04.2016
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35. Getting Started in Actor Prolog. Analyzing Web Sites.
In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...
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Ссылки http://www.cplire.ru/Lab144/start/e_scan.html -- 13.7 Кб -- 24.09.2007
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36. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
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37. Medium
The space between the planets is far from empty. It contains: electromagnetic radiation (photons); hot plasma (electrons, protons and other ions) a.k.a. the solar wind ; cosmic rays; microscopic dust particles; and magnetic fields (primarily the Sun's). While the Sun 's radiation is obvious, the other components of the interplanetary medium were not discovered until very recently. ... Except near some of the planets, interplanetary space is filled with the Sun's magnetic field. ... Sun .. ...
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Ссылки http://www.sai.msu.su/tnp/medium.html -- 7.8 Кб -- 01.10.2012
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38. http://jet.sao.ru/~goray/v4641/v4641.htm
Taking into account the result by Watanabe P=2.5 days in outburst, I reconstruct old set of photographic observations being partly lost, and add some new observations. ... The periodogram calculated with the method by Lafler and Kinman is shown. ... The last periodogram indicates peaks corresponding following possible periods with the double-wave light curve: 0.4236, 0.4650, 0.5379, 0.6064, 0.7365, 0.871, 1.168, 1.5437, 2.8173, and 6.89 days. ...
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Ссылки http://jet.sao.ru/~goray/v4641/v4641.htm -- 2.3 Кб -- 22.07.2005
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39. COSMIC RAY Observation
Cosmic Ray laboratory of . ... Neutron Monitor (Cosmic Ray Observations) . is situated in Irkutsk (Russia) . ... Height - location above sea level . ... Height: . ... For recording the CR (Cosmic Rays) neutron component at Irkutsk, . neutron monitor NM-64 is used, which is an installation with 18 two-meter proportional counters filled with BF 3 (boron trifluoride gas) in which the B 10 90 per cent of the total boron. ... The neutron monitor is located at 475m above sea level. ...
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Ссылки http://cgm.iszf.irk.ru/irkt/about.htm -- 3.9 Кб -- 10.01.2005
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40. Pulkovo Database of Observations of Visual Double Stars
. Additional settings . Number of observations found: . 17 . ADS number: . 03353 . WDS number: . 04385+2656 . Components: . AB . All (17) . Photo (15) . CCD (2) . Epoch . JD . Separation . e(S) . N(S) . e1(S) . Pos.angle . e(P) . N(P) . e1(P) . N . Orient. Meas.code . Detector . Back . Abbreviations . Main Page .
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Ссылки http://www.puldb.ru/db/ds.php?q=99 -- 5.5 Кб -- 27.02.2014
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