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http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/folk/c/chandlers_wife.
http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/folk/c/chandlers_wife.
1. http://www.stsci.edu/stsci/meetings/planets/abs/prog3.html
... Kepler is a mission designed to detect and characterize Earth-sized planets around solar-like stars. The sizes of the planets are determined from the decrease in light from a star that occurs during planetary transits, and the orbital period is determined from the repeatability of the transits. ... These goals are accomplished by continuously and simultaneously monitoring a single field of 140,000 stars for evidence of brightness changes caused by transits of Earth-sized or larger planets. ...
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Ссылки http://www.stsci.edu/stsci/meetings/planets/abs/prog3.html -- 5.3 Кб -- 22.10.1996
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2. Research - The high-velocity clouds of M31
... Research . ... The major problem in HVC research is the unknown distance towards most of the HVCs. ... Thilker et al. (2004) used the Green Bank Telescope (GBT) to map an area of $7^{\circ} \times 7^{\circ}$ around M31 in H i . They discovered a population of HVCs located within a projected distance of about $50~\mathrm{kpc}$ from M31. ... 2004). ... The remaining HVCs around M31 are isolated in position and velocity and may represent primordial, dark-matter-dominated clouds. ...
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Ссылки http://www.atnf.csiro.au/people/Tobias.Westmeier/research_m31.php -- 8.9 Кб -- 10.04.2016
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3. http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/magnetic.pdf
Magnetic Fields around Radio Galaxies Robert Laing (ESO) Laing et al. ... 2008) Negligible depolarization and 2 rotation Almost all Faraday effects must be due to foreground material How to fit depolarization caused by foreground Faraday rotation Complex polarization Rotation measure Integrate over a beam Observed RM for 0 2 rotation and depolarization Faraday rotation and depolarization 5.5 arcsec FWHM Faraday effects at high resolution FWHM = 1.5 ...
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Ссылки http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/magnetic.pdf -- 810.2 Кб -- 07.04.2009
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4. http://zebu.uoregon.edu/51peg.html
... More on 51 Peg: . The discovery of a Jupiter--mass planet in orbit around the solar--type star 51Peg has been reported by Michel Mayor and Didier Queloz (Geneva Observatory) on October 6th at the 9th Cambridge workshop on "cool stars, stellar systems, and the sun" held at Florence (Italy). ... Recall that the measurements of radial velocity only yield v sin i which in turn gives us M sin i. For most values of i, sin i will be greater than 0.5 and this gives a mass estimate of 0.5 Jupiter masses. ...
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Ссылки http://zebu.uoregon.edu/51peg.html -- 18.2 Кб -- 31.07.2000
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5. A Technique for Determining Proper Motions from Schmidt Plate Scans at ST ScI
... Keywords: Proper Motions, Schmidt Plates, Astrometry, Guide Star Catalog, Palomar Sky Survey . In this paper we describe a program of determining proper motions from digitized scans of 1950's-era Palomar Sky Survey (POSS) Schmidt Plates and 1980's-era Palomar Oschin Schmidt `Quick V' plates that were taken for the Hubble Space Telescope ( HST ) Guide Star Catalogue. ... Arrows indicate the magnitude and direction of the proper motion for the stars. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/williamsonr.html -- 10.9 Кб -- 03.11.2000
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6. antichnoste
Aristarch is Copernic of Classic World. ... First Aristarch determined the fact for how many times the Sun was father then the Moon and then he compared the Sun and the Moon with the Earth. ... Only the Moon rotates around the Earth. ... Gipparch suggested that the Sun turned around the Earth steady and in circumference but the Earth is displaced according its centre. ... The orbit point in which the Sun is nearer to the Earth Gipparch called perigee and the most remote one he called apogee . ...
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Ссылки http://www.space.vsi.ru/antichnoste.htm -- 6.6 Кб -- 14.10.2000
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7. http://www.naic.edu/vscience/schedule/tpfiles/O'NeiltagA1267tp.ps
Proposal Identi cation No.: A1267 Date Received: 1999-Jan-28 09:39:33 Technical Page Proposal Type: Regular General Category: Astronomy Sub-Category: Spectroscopy Observation Category: Extragalactic Total Time Requested: 30 Hours Proposal Title: Determining the Galaxy Density Around Known LSB and HSB Galaxies in the Nearby Universe ABSTRACT: That the small-scale environment a galaxy signi cantly a ects its evolution has been well established, but the details of this process are not well known. ...
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Ссылки http://www.naic.edu/vscience/schedule/tpfiles/O'NeiltagA1267tp.ps -- 96.9 Кб -- 15.10.2002
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8. E-P transitions for different orbits
Next: The Scenario Machine: Operational Up: Evolution of Magnetic Rotators Previous: Ejector-propeller hysteresis . ... The length of this segment is determined by the eccentricity. ... In this case no hysteresis occurs and transitions E -- P and the reverse take place in symmetrical points of the orbit. ... Here EP means a mixed state of the rotator at which it is in the ejector state during one part of the orbit, and in the propeller state during the rest of the orbital cycle. ...
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Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node32.html -- 10.3 Кб -- 26.02.1997
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9. Journal "Peremennye Zvezdy"
Swift Launches . ... Credit Copyright: NASA Explanation: Where do gamma ray bursts occur? To help find out, NASA launched the Swift satellite on Saturday, as pictured above . What Swift is designed to do better than any previous satellite is to quickly locate these enigmatic explosions in both sky position and distance. Once a gamma ray burst (GRB) is located, Swift itself will rotate to face it head-on and determine its distance directly. ... NASA Official: Jay Norris. ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1201258 -- 7.9 Кб -- 22.11.2004
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10. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0047-1-0.ps.gz
XMM Newton CCF Release Note XMM CCF REL47 EPIC Filter Transmission D Lumb November 16, 2000 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS flag EMOS1 FILTRANSX 0007 2000 01 01T00:00:00 FILTER THICK , THIN , MEDIUM , EBINS NO EMOS2 FILTRANSX 0007 2000 01 01T00:00:00 FILTER THICK ,THIN , MEDIUM , EBINS NO EPN FILTRANSX 0010 2000 01 01T00:00:00 FILTER THICK ,THIN , ... Therefore some reiteration on all 3 data sets will be necssary. ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0047-1-0.ps.gz -- 101.0 Кб -- 03.01.2001
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11. Using the less pager
. less has better features than more and can be customised to suit your particular needs. Many of its commands are the same as those of the text editor vi . To display a file use the command: less filename . This will display the first screenful of the file. A prompt with the filename is given in the bottom left-hand corner of the screen. You can now move around the file using the less commands. Summary of less commands . Customising the less pager .
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Ссылки http://comet.sai.msu.ru/UNIXhelp/tasks/display1.3.html -- 2.3 Кб -- 17.01.1997
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12. http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/m/misc/mustang_sally
Mustang Sally The Commitments , Wilson Pickett, Buddy Guy, et al key of C C7 verse1 Mustang Sally , guess you better slow that Mustang down F7 C7 Mustang Sally , guess you better slow that Mustang down G G F# F7 You been runnin' all over town C7 I guess you gotta put your flat feet off the ground C7 chorus All you wanna do is ride around Sally ( ride ...
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Ссылки http://crydee.sai.msu.ru/ftproot/pub/rec/music/lyrics/cs-uwp/m/misc/mustang_sally -- 2.8 Кб -- 27.03.1994
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13. K-band Arcetri Obscured Supernova Search - Detection technique
Detection technique . We are using ISIS , the optimal image subtraction method developed by C. Alard & R.H. Lupton, to search for SNe in our images. ... The second image shows the same subtraction, but after the convolution of the best image with ISIS: . ... For this reason, we are suggested to search for nuclear SNe with NICMOS on HST, to exploit its stable PSF, sensitivity and angular resolution to detect from space nuclear obscured SNe which might have been missed by ground-based surveys. ...
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Ссылки http://www.arcetri.astro.it/science/SNe/ISIS.html -- 4.5 Кб -- 02.10.2008
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14. Select a circle around the central point source
Next: A box, to include Up: To produce a region Previous: To produce a region . select cursor and circle . When in the image window, the mouse now has a box shape with an arrow at the upper left corner. The mouse buttons act as follows: . LEFT - to move the center of the circle at the position of the arrow point. ... RIGHT - idle. center the circle at the point source by positioning the arrow point and clicking on the LEFT mouse button. A circle will appear at the arrow position. ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node62.html -- 5.9 Кб -- 01.10.2012
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15. http://www.mso.anu.edu.au/seminars/abstracts/20150210-1100.html
... Right now, the world needs 10,000 additional radiotherapy machines to meet demand. ... The imaging and tracking (source finding) techniques being pioneered for Nano-X form part of an inter-disciplinary research program being developed through a CAASTRO collaboration currently involving Medical Physics and Astrophysics at Sydney and Curtin Universities, together with the Nelune Comprehensive Cancer Centre at Prince of Wales Hospital. ...
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Ссылки http://www.mso.anu.edu.au/seminars/abstracts/20150210-1100.html -- 5.1 Кб -- 10.04.2016
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16. The Sparkle Plug-In: The Sparkle Dialog Box
... There are number of features that can be set by the user in the Sparkle Dialog box. ... The Sparkle plug-in computes the luminosity (level of whiteness) of each pixel in the image (the user can see this when the progress window labeled Generating luminosity array... is displayed). ... The threshold value is currently a slider/text field pair which have a precision of .0001. ... Like the Threshold value, the Flare Intensity has both a slider and a text input field for specifying its value. ...
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Ссылки http://www.sai.msu.su/~megera/gimp/mjhammel/gdp/plug-ins/sparkle-3.html -- 7.9 Кб -- 22.12.2007
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17. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAB5B977A-8A0E-494A-BA35-D9DE7E45A228%7D
. Light echoes around a neutron star have allowed a precise distance to be determined to it. These light echoes are produced when a burst of X-rays bounces off of clouds. X-ray: NASA/CXC/Univ. of Wisconsin-Madison/S.Heinz et al; Optical: DSS
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAB5B977A-8A0E-494A-BA35-D9DE7E45A228%7D -- 3.2 Кб -- 10.04.2016
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18. default
. First Observer's Trailer Installation: June 17, 2002 . Unit R-8108 arrived around noon; driver determined to install the first trailer near the walkway instead of first placing the other trailer to the side of the storage uni. Note the damage in the upper right corner of the roof - missing shingles. Tight fit; the driver was confident there would be enough room to move in the other trailer. Note: the doors and windows are in the wrong location.
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Ссылки http://www.apo.nmsu.edu/Telescopes/ARCprogress/052002trailinstall/061702install1/default.htm -- 3.4 Кб -- 18.06.2002
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19. A Statistical Study of the Relationship between the Solar Cycle Length and
... We have determined the correlation coefficient between tree-ring index values and the sunspot cycle length for 69 tree-ring data sets from around the world of greater than 594 years duration. ... Similar matrices, formed from the same data, but randomly scrambled, provide a control against which we can draw conclusions about the influence of the solar cycle length on climate with a reasonable degree of confidence. ...
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Ссылки http://star.arm.ac.uk/~ambn/abstract288.html -- 2.5 Кб -- 07.05.1998
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20. Galileo Crosses Boundary Into Jupiter's Environment
NASA's Galileo spacecraft radioed confirmation late this week that it has entered Jupiter's environment, crossing over the boundary from interplanetary space into the giant magnetic cocoon around Jupiter called the magnetosphere. ... On Thursday, December 7, Galileo's previously deployed atmospheric probe will plunge into Jupiter's cloud tops at 5:56 p.m. EST and descend into the giant planet on a parachute. ... Jupiter's magnetosphere is like a giant bubble around the planet. ...
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Ссылки http://www.iki.rssi.ru/solar/eng/galpr.htm -- 5.8 Кб -- 15.10.1997
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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