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1. Taurid Complex
Orbital intersection . ... Structure of Taurid stream . ... Meteoroid swarm and Taurid fireballs . ... The following four diagrams schematically show four different Taurid orbits and the orbits of Earth and Jupiter. ... The Taurid stream contains particles (small, solid grains) at different stages of their precession cycles. ... The study of when a meteor stream can produce a meteor shower is the study of when precession brings orbits to intersection with Earth, or e.g. with Mars . ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~aac/zetataur.html -- 8.7 Кб -- 19.10.2007
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2. Laboratory for Spectroscopy of Molecular Structures
... Laboratory for Spectroscopy of Molecular Structures . ... Optics and spectroscopy of molecular and liquid crystals, fullerenes, superthin molecular films. Optical studies of structure, phase transitions, pretransitional phenomena, structural modifications in external field and under high pressure. ... Methods developed in the laboratory enable to determine in free standing films of different types liquid crystals values of polarization, two-dimensional constants of orientational elasticity. ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/lsms/indexen.html -- 9.6 Кб -- 03.12.2012
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3. The Structure of HTML 3.0 Documents
... Most HTML elements are identified in a document as a start tag, which gives the element name and attributes, followed by the content, followed by the end tag. ... To identify the document as being HTML 3.0, it is recommended that documents start with the prologue: <!doctype HTML public "-//W3O//DTD W3 HTML 3.0//EN"> . ... HTML 3.0 documents formally have the following structure: <HTML> <HEAD> head elements .. ... HTML> . ... The permitted syntax of HTML 3.0 compliant documents is specified by the...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/webdesign/html-3.0/overview.html -- 4.2 Кб -- 19.12.1996
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5. Doug Burke's Perl/S-Lang pages: Structure examples
... Doug's Home Page . ... S-Lang structures are converted to hash references in Perl , as shown below. ... n\n ; print Structure contents:\n ; # you can treat $s as a reference to a hash array in most respects, except: # - the order of the keys in the array matches that of the # original S-Lang structure # while ( my ( $ key , $ value ) = each %{$s} ) { print key $ key \t has a value of $ value \n ; } print \n ; $$s{afield} = 'a changed field value '; print ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~dburke/perl-slang/examples_structs.html -- 9.6 Кб -- 02.10.2012
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6. Magnetic Field Lines
... Magnetic field lines similarly describe the structure of magnetic fields in three dimensions.They are defined as follows. If at any point on such a line we place an ideal compass needle, free to turn in any direction (unlike the usual compass needle, which stays horizontal) then the needle will always point along the field line (drawing below). Field lines converge where the magnetic force is strong , and spread out where it is weak. ... Exploration" home page (index) Glossary . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/EAMAGSPH/wfldline.html -- 5.1 Кб -- 21.12.2007
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7. Structure of FITS files
Next: FITS data-types and Up: FITS Format Previous: FITS Format . A FITS file contains a sequence of logical header/data units (HDU) which all start with a set of header records describing the following data records. The logical record length of a FITS file is always 2880 bytes of 8 bits. Both header and data sections start in a new logical record. ... The basic FITS paper [ 1 ] specified both a logical and physical record length of 2880 bytes. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol1/node108.html -- 4.2 Кб -- 23.02.1996
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8. GRB follow-up team
... Team . ... V.V.Sokolov "The gamma-ray bursts, core-collapse supernovae and global star forming rate at large redshifts" . ... I.V.Sokolov, A.S.Moskvitin, Eda Sonbas, O.V.Verkhodanov, O.P.Zhelenkova "A galaxy cluster in the GRB 021004 field" . ... The monitoring of GRB afterglows and the study of their host galaxies with the SAO RAS 6-m telescope from 1997". ... A.S.Moskvitin, T.A.Fatkhullin, V.V.Sokolov and V.N.Komarova, "Spectral and photometric monitoring of CCSNe at SAO RAS" . ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/grb/conf/conf.html -- 16.2 Кб -- 09.04.2016
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/grb/conf/conf.html -- 16.2 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/grb/conf/conf.html -- 16.2 Кб -- 09.04.2016
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9. CHAMELEON file structure
Next: COBRA file structure Up: Appendices Previous: CONSTRICTOR output file structure Contents . ... SCANDATA TABLE NUMSCAN _ INTEGER SCANID [ NumScan ] _ INTEGER Unique observed STARID [ NumScan ] _CHAR*7 e.g. BSC1948 SCANTIME [ NumScan ] _ DOUBLE [s] from 0UT of date OUTPUTBEAM [ NumOutBeam ] EXTCOLUMN VISSQ [NumSpecChan( beam )][NumBaseline( beam )][ NumScan ] _ REAL VISSQERR [NumSpecChan( beam )][NumBaseline( beam )][ NumScan ] _ ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~chummel/oyster/manual/node255.html -- 10.0 Кб -- 28.04.2015
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10. http://www.mrao.cam.ac.uk/~cjld1/pages/mit3.pdf
Geometric Algebra 3 Dirac Theory and Multiparticle Systems Chris Doran Astrophysics Group Cavendish Laboratory Cambridge, UK Dirac Algebra · Dirac matrix operators are · These act on 4-component Dirac spinors · These spinors satisfy a first-order wave equation MIT3 2003 2 STA Form · Adapt the map for Pauli spinors · Action of the various operators now Imaginary structure still a bivector Dirac equation MIT3 ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~cjld1/pages/mit3.pdf -- 457.9 Кб -- 24.03.2003
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11. Two Story Dome Structure In Progress - an Astronomy Net Domes Forum Message
Domes Forum Message . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Domes and Observatories Discussion | ... Two Story Dome Structure In Progress . ... I am in the middle of planning a two story building with a metal dome on top to get better horizon to horizon viewing. ... www.astronomy.net . ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/domes/messages/31.shtml -- 13.6 Кб -- 09.04.2016
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12. Structure of the Large Magellanic Cloud (LMC)
The near-IR data from 2MASS (Two Micron All Sky Survey) and DENIS (Deep Near-Infrared Southern Sky Survey) are ideally suited for studies of the structure of the LMC, because of the large statistics and insensitivity to dust absorption. ... Wide-angle view of the Large and the Small Magellanic Cloud (SMC) on the sky. ... Another wide-angle view of the LMC (bottom left) and the SMC (top left) on the sky, with part of the luminous band of the Milky Way visible as well (right). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~marel/lmc.html -- 7.8 Кб -- 22.05.2001
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13. Heliophysics, Internal structure and seismology
This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ -- 5.6 Кб -- 21.03.2012
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14. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD5DEC08B-F65B-4888-9A9E-9F931634FB4A%7D
Dust and debris parade in an extremely misshapen ring around the young star, HD 15115. The disk, seen edge-on with NASA's Hubble Space Telescope, is the dense blue line extending from the star to the upper right and lower left of the image. The disk appears thicker at upper right than at lower left, evidence of its lopsided structure. Astronomers think the disk's needle-like look is caused by dust particles following a highly elliptical orbit around the star. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD5DEC08B-F65B-4888-9A9E-9F931634FB4A%7D -- 3.8 Кб -- 10.04.2016
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15. http://www.astro.spbu.ru/staff/ilin2/SOFTWARE/AXITM/readme
Light scattering by axisymmetric particles within a new approach to the T-matrix method The code AXISYM0.FOR realises the new approach to the solution of the light scattering problem suggested by Farafonov (Opt. ... Below them one finds also the description of the input and output parameters, and a list of some used subroutines. The comments given through the code's text allow one to follow its general structure. The file IN contains the input parameter values for a test run. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/ilin2/SOFTWARE/AXITM/readme -- 2.5 Кб -- 19.11.2010
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16. http://www.atnf.csiro.au/research/cena/documents/presentations/bray.pdf
A limit on the ultra-high-energy neutrino flux from Centaurus A Justin Bray For the LUNASKA collaboration Clancy James, Ron Ekers, Chris Phillips, Paul Roberts, John Reynolds, Rebecca McFadden, Ray Protheroe, Jaime Alvarez-MuЯiz, Justin Bray Outline: · Ultra-high-energy (UHE) cosmic rays neutrinos · Detecting UHE neutrinos · The lunar Cherenkov technique · Observations with the ATCA · Observations with Parkes · ASKAP and the future ... Detection Geometry Neutrinos are penetrating.. ...
[ Текст ]  Ссылки http://www.atnf.csiro.au/research/cena/documents/presentations/bray.pdf -- 2515.7 Кб -- 20.07.2009
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17. ION AND ELECTRON ENERGY DETECTOR PAN-2
ION AND ELECTRON ENERGY DETECTOR PAN-2 . ... The energy and angular distributions of charged particles can bring further information on the nature and spatial scales of magnetospheres processes. ... It permits the fast measurements of energy and angular parameters of charged particles in the range 40eV-40keV. ... The sensor unit is an electron electrostatic, axially symmetrical, toroidal analyzer. ... The energy range for both types of charged particles must stepped according to the logarithmic scale. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/projects/warning/pan-2.html -- 6.1 Кб -- 15.02.2000
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18. Naomi McClure-Grffiths
... Now we're getting ready for the Australian SKA Pathfinder ( ASKAP ) and the Square Kilometre Array ( SKA ) itself. I co-lead the Galactic ASKAP survey, GASKAP, and the Polarisation survey, POSSUM. I have roles in SKA science planning, including membership on two SKA Science working groups (HI and The Galaxy), the SKA Science and Engineering Advisory Committee, Australia New Zealand SKA Coordination Committee (ANZSCC) and ANZSCC's Science Advisory Committee. ... Read More . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~naomi/ -- 8.0 Кб -- 09.04.2016
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19. The new concept of formation and development of the Solar system
... part 2 | ... Part 1 . The new concept of formation and development of the Solar system. ... Thus, the initial pulse of the rotation of a protosolar cloud of the solar system was determined as a result of the diversion of a part of the moment of the rotational pulse of the Galaxy. ... Besides this new approach to the pre-solar system as a system of the destroyed vortex structure, we can understand now a number of other peculiarities of the Solar system's structure. ...
[ Сохраненная копия ]  Ссылки http://www.lermus.ru/users/trunaev/part1.htm -- 28.0 Кб -- 04.12.2001
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20. The Arcetri Spectral Code file format
Each emissivity line is structured using the following format: An example from the Ne=10^ 10 file (phot cm 3 s -1 ) is given below: . Fe 2 1550.272 Mn 3.8815e-18 2.2909e-17 6.9024e-17 5.6234e-17 2.2751e-17 ... with the following meaning: . ... 1550.272 : Wavelength ( ) of the transition; . ... 3.8815e-18 : Emissivity in phot cm 3 s -1 for Log T = 4.0 ; . 2.2909e-17 : Emissivity in phot cm 3 s -1 for Log T = 4.1 ; . ... 2.2751e-17 : Emissivity in phot cm 3 s -1 for Log T = 4.4 ; .. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/spettro/line_format.html -- 3.0 Кб -- 11.07.2001
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