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http://xmm.vilspa.esa.es/sas/6.0.0/doc/cxctods9/ChangeLog.
http://xmm.vilspa.esa.es/sas/6.0.0/doc/cxctods9/ChangeLog.
1. Fixing and Freeing Region Markers
Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...
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Ссылки http://hea-www.harvard.edu/RD/saotng/fixregions.html -- 7.3 Кб -- 01.10.2012
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2. http://xmm.vilspa.esa.es/sas/6.5.0/doc/cxctods9/ChangeLog
... SOC-SPR-2454. Version 1.44 - 2003-05-03 (UL) ------------ + brought in line with selectlib-4.65 Version 1.43 - 2003-03-13 (UL) ------------ + some transparent gcc-2.95.3 backward-compatibility changes Version 1.42 - 2003-03-05 (UL) ------------ + closed SPR 2403: How to change the ds9 that xmmselect uses Ds9 constructur (used by xmmselect) now makes use of SAS_IMAGEVIEWER environment variable that can also contain an absolute path the ds9 executable ...
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Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/cxctods9/ChangeLog -- 9.2 Кб -- 04.08.2005
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3. Changing Programs & Resolving Problems
... HST . ... Data . ... Hubble Heritage Project . ... HST Peer Review Process . ... HST Overview . ... Cycle 24 Announcement . ... Program Information . ... Retrieving HST Data . ... Program Change Requests . ... Proceed to the Program Information Page for the program in question, and use the appropriate links on that page. ... Policies for the Telescope Time Review Board (TTRB) : Repeating HST Observations, Changes to Accepted HST Programs, Resolution of Duplications, and Other Program Alterations. ...
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Ссылки http://www.stsci.edu/hst/programs/changing_programs -- 13.3 Кб -- 10.04.2016
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4. http://www.atnf.csiro.au/research/Astro2010/talks/mverdon.pdf
Pulsar radio emission - oscillating model M. Verdon, D. Melrose University of Sydney 10 th June, 2010 Outline Problems understanding pulsar radio emission Magnetosphere model Emission mechanisms Oscillating model Wave modes Time-dependence Coupling What is a pulsar? rotation axis magnetic axis polar cap open field line region closed field line region Emission models Production of ...
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Ссылки http://www.atnf.csiro.au/research/Astro2010/talks/mverdon.pdf -- 553.5 Кб -- 16.06.2010
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5. An IRAF-Independent Interface for Spatial-Region Descriptors
... To move toward open analysis software, we plan to make the PROS regions subsystem available from processes outside of IRAF. We also plan to make the region descriptor parsing system available for purposes beyond the creation of masks, such as an interface to an image display program, accepting a region descriptor and generating commands to display the region on an image. ... Anticipating two kinds of new requirements, we reconsidered the design of the PROS region descriptor processing subsystem. ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/schmidtd.html -- 11.4 Кб -- 03.11.2000
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6. Dynamic HTML in Communicator
... The previous example, Chapter 12, "Expanding Colored Squares Example," illustrates how to expand and contract the clipping region of a layer without changing the wrapping width of the layer. This example illustrates how to capture mouse events so that the user can make a layer's wrapping width wider or narrower by dragging the mouse. ... how to capture mouse events for a layer . how to change the wrapping width of a layer by using the load() function . ... Capturing Events for the Layer . ...
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Ссылки http://crydee.sai.msu.ru/~vab/html.doc/dhtml/dynhtml/layers38.htm -- 11.3 Кб -- 13.08.1997
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7. Common problems
... R.A. = 00h55m04s.86, Decl. = -37 41'43".7 . ... Variable star in NGC 1511 . ... Variable star near Pegasus 2001bn IAUC 8624 BV anon 2001bh 7622 K star ugc11635 2001dh 7482 M star ic5374 1999db 7227 QSO anon 1999dc 7227 AGN anon 1999cx 7210 AGN anon 1999cu 7210 AGN anon 1999bs 7141 cat var ugc11093 1998di 6982 dwarf nova anon 1993U 5818 QSO anon 1993V 5818 QSO anon 1992W 5517 M star mcg 8-23-96 1992X 5517 M star mcg 6-32-24 1991ap 5327 QSO anon 1989Z 5162 var ngc4013 1985J 4059 CV ugc6274 ? ...
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Ссылки http://www.rochesterastronomy.org/snimages/snproblems.html -- 7.3 Кб -- 19.04.2014
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8. The Sun Changes
Astronomy Picture of the Day . ... 13.04.1998 . ... Credit: Learmonth Solar Observatory , IPS , USAF , NOAO Explanation: Our Sun changes every day. ... Dark spots that might appear on the image are usually sunspots , dark magnetic depressions that are slightly cooler than the rest of the Sun's surface. ... Over the next few years the average number of sunspots and plages will increase until "Solar Maximum" occurs in 2001. ... April 1998 . ... 1997 1998 . ... Publications with keywords: Sun - sunspot . ...
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Ссылки http://www.astronet.ru/db/xware/msg/1163501 -- 13.8 Кб -- 01.02.2007
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9. How can six Trojan asteroids reside in Neptune's L4 region without colliding? |
... Young super-Jupiter found wandering without a parent . ... Astronomy for Kids . ... Tune into the Asteroid Day press conference . ... Astronomy 101 . ... How can six Trojan asteroids reside in Neptune's L4 region without colliding? ... The gravity of a planet, its star, and the centrifugal force associated with the planetary orbit nearly balance in five regions near the planetт??s path where an asteroid (or spacecraft) could orbit safely. ... Get instant access to subscriber content on Astronomy.com...
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Ссылки http://www.astronomy.com/magazine/ask-astro/2013/03/trojan-asteroids -- 63.4 Кб -- 10.04.2016
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10. http://www.naic.edu/~phil/lbw/calpolbJump_dec05/calPolBJump_dec05.html
... The cal value for lbw polB changed on 04dec05. ... The Tsys jump in polB occurred with both diode 1 and diode 2 so the problem was after the switch that selects which diode to send to polB. ... The plots show tsys versus date (.ps) ( .pdf ): . ... Top: Tsys polA vs date. ... All tsys measurements switched to diode 2. 23nov05 ( dashed green ): new diodes installed. 23/25nov05 ( dashed purple ): cal values remeasured. 06dec05 ( dashed blue 1405Mhz to get off of the resonance in polA at 1400Mhz. ...
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Ссылки http://www.naic.edu/~phil/lbw/calpolbJump_dec05/calPolBJump_dec05.html -- 7.2 Кб -- 01.03.2006
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11. Circular polarization: change of sign
Next: Scattering properties Up: Polarization properties (transmitted radiation) Previous: Linear polarization: wavelength dependence . Traditionally, the main problem considered in connection with circular interstellar polarization is the meaning of the wavelength where changes the sign . ... This is also demonstrated by Fig. 19 (lower panel) which shows the wavelength dependence of the factors of linear and circular polarization for particles of magnetite as was done by Shapiro ([ 1975 ]). ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node8.html -- 13.2 Кб -- 19.11.2010
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12. http://www.issp.ac.ru/iao/2014/booklet/ia14_booklet_en1_page_B02.pdf
... Great oppositions. ... Proxima Centauri. ... Scientists proved that the problem of preserving the Earth's climate and the annual change of seasons can be solved by a small star, negligible mass, but similar to a main-sequence star, moving in a circular orbit around the Sun. ... Sombrero Galaxy. The Sombrero Galaxy, M104, is known as a holder of one of supermassive black holes. ... Roughly estimate the approximate mass of the supermassive black hole in the center of M104 (answer in solar masses m). ...
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Ссылки http://www.issp.ac.ru/iao/2014/booklet/ia14_booklet_en1_page_B02.pdf -- 257.5 Кб -- 22.10.2014
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13. ASP: Effecting Global Change
The night after the John Glenn program, I pitched the terraforming idea to my students. I asked them if they'd like to terraform Mars as a big class project; I wanted to throw the idea to them and see how they would react. Already I had a vision of splitting the class into several groups and having each group take charge of a portion of the project. ... Following my initial idea on how to conduct the project, I split the class into six groups, each student choosing his or her group. ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/48/change2.html -- 11.3 Кб -- 02.10.2012
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14. http://www.astro.louisville.edu/software/astroimagej/updates/release_notes.html
AstroImageJ Release Notes . ... Daily Build Version db3.2.1 (with ImageJ 1.47i) (Last Updated: 02/04/2016) . Changes . Version 3.2.0 (with ImageJ 1.47i) (Release date: 02/01/2016) . ... Version 3.1.0 (with ImageJ 1.47i) . ... Known Problems . Feature Requests in Roadmap but not in this Version . ... Version 2.0.0 (with ImageJ 1.47a1) . ... Changes in this Version . ... Version 1.1 (with ImageJ 1.45l) . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/updates/release_notes.html -- 220.6 Кб -- 28.03.2016
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15. The Face on Mars
... The Raw Images . Table 1: List of Viking Orbiter Images of the "Face on Mars" . ... Processing the Face Images . ... In July, 1976, Viking Orbiter 1 was acquiring images of the Cydonia region of Mars as part of the search for potential landing sites for Viking Lander 2. ... Using the height field, it is also possible to view the "Face" from different look directions, by mapping the Viking Orbiter image directly on the the topography and then placing the "viewer" at different locations. ... Mars . ...
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Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/face.htm -- 14.9 Кб -- 15.03.1998
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16. The Face on Mars
The Face on Mars . ... The Raw Images . Table 1: List of Viking Orbiter Images of the "Face on Mars" . ... Processing the Face Images . Table 2: Dimensions of Mercator Projected Images of "The Face on Mars" . Map Projected Images . ... Processing the "Face on Mars" Images . ... This page will provide interested persons with both the raw Viking images, transformed to GIF format, and a brief tutorial (with examples) of image processing techniques applied to create "better looking" images. ...
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Ссылки http://www.iki.rssi.ru/solar/eng/face.htm -- 12.7 Кб -- 15.10.1997
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17. Zen: Search for: "count problem"
. Hide Zen home . Pgsql . GiST . GIN . SP-GiST . Tsearch2 . SAI RVO . SAI CAS . SOA . Supernovae . TODO . HomePage . Astronet . Google . Rambler . Yandex . Oddmuse . E-R-E dict . Index . edit . View changes for these pages . count problem . == Почему count(*) медленный ? == Очень кратко: из-за MVCC (многоверсионности). 1K - last updated 2005-04-08 20:32 UTC by megera . 1 pages found. SiteMap Changes HowTo 2016-04-11 2016-04-10 Blog . Administration . Search: . Zen, 2003-2007
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Ссылки http://www.sai.msu.su/~megera/wiki?search=%22count+problem%22 -- 6.1 Кб -- 11.04.2016
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18. 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
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19. Phil Plait's Bad Astronomy: Misconceptions
... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...
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Ссылки http://www.badastronomy.com/bad/misc/badseasons.html -- 24.7 Кб -- 09.04.2016
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20. Guider Image Controller Overview
... Finding Stars . ... Handling Bad Pixels . ... The guide camera image controller can control one or more guide cameras. ... Each time the camera is read, the image is automatically saved to a fits file on a shared disk. ... Cameras that have bad pixels require "bad pixel maps" in order to find stars, centroid or even compute statistics for the image. ... View this image (for instance in NIH Image) and determine an upper and lower cutoff; pixels whose values are outside of this range are considered...
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Ссылки http://www.apo.nmsu.edu/Telescopes/HardwareControllers/GuiderImageOverview.html -- 10.6 Кб -- 22.06.2000
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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