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1. VSOP Long-Term Schedule
Last modified: 17 February 1998 . Original version 17 February 1998 . Modified: . This WEB page contains the schedule for HALCA observations from March 1 to June 30, 1998. ... Frequency bands with a following '*' are for polarization and will be recorded with 256 Mbit/s. S2 V123a CYG-A C Socr 107 Fr:Apr-17 06:10 - 20:55 VLBA VT835 W49N K Socr 109 Su:Apr-19 08:20 - 18:20 VLBA VT837 1921-293 K Socr 110 Mo:Apr-20 09:30 - 12:30 VLBA Percentage of time 2.8 . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/pub/people/vlbi/vsop/www/longterm_980217.html -- 57.7 Кб -- 27.12.2007
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2. Output Columns modified
XMM-Newton Science Analysis System . ... CORR_RATE - The count rate after the following corrections have been applied; . 1) A further point-spread function correction may be applied, to extrapolate the counts from 12 to 35 pixels (presently only done for UV observations) 2) Correction for dead-time. 3) Correction for the OM sensitivity-degradation. A key-word TDS_CORR is added to the table to record the correction value. ... XMM-Newton SOC/SSC -- 2007-07-09 ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/ommag/node8.html -- 3.6 Кб -- 09.07.2007
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3. FIRPO Help 1
... This is in the cardboard box labelled "new setup", together with other stuff below. ... In the Leinert Schrank there is a box of new (virgin, unconnected) batteries. ... This is to be obtained somewhere (at this time there were two on the first level of the 1.23m building) 7- a multimeter. to be found in Leinert's Schrank. 8- an eyepiece for the photometer, and a barrel with hole to check the alignment of the mount. these are in a small cardboard box, to be found inside the "new setup" box. ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/luna/firpo/firpo_message10.html -- 5.5 Кб -- 28.07.2005
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4. Sunspots and active regions February 09, 2016
... Sun images . ... Active areas . February : 2016 . ... The following regions with sunspots can be now observed on the Sun's surface . Group number . ... Group length (in degrees) . ... Beta . ... Coordinates and other characteristics of active regions are issued for February 09, 2016 00:31 UT The following H-alpha plages without spots can be currently observed on the Sun's surface . ... Coordinates and other characteristics of active regions are issued for February 09, 2016 00:31 UT . ...
[ Сохраненная копия ]  Ссылки http://www.tesis.lebedev.ru/en/active_areas.html?m=2&d=9&y=2016 -- 25.3 Кб -- 11.04.2016
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5. Format Documentation of *.wdc Files
... Denmark: ftp://ftp.dmi.min.dk/pub/Data/WDCC1/indices/kp-ap/ . Germany: ftp://ftp.gfz-potsdam.de/pub/home/obs/kp-ap/ . ... we do not guarantee the correctness of the international sunspot number R; these values are published separately (Brussels, Belgium) The following scientific and format documentation is adapted from ftp://ftp.ngdc.noaa.gov/STP/GEOMAGNETIC_DATA/INDICES/KP_AP/kp_ap.fmt The subscript p means planetary and designates a global magnetic activity index. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/KP_INDEX/wdc_fmt.html -- 8.3 Кб -- 21.12.2007
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6. NVSS radio survey
... The NVSS is being made as a service to the astronomical community, and the principal data products are being released into a directory accessible by anonymous FTP as soon as they are produced and verified. ... The large (4 deg x 4 deg) map cubes and total intensity only images and their associated multisource (u,v) data sets are stored as binary files in FITS format (see Grosbol et al. ... The source catalog derived from the available images is kept in directory CATALOG as CATALOG.FIT. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/doc/NVSS.html -- 7.9 Кб -- 30.09.1998
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7. About modification of the INTERBALL orbital elements
... The accuracy of calculation of both INTERBALL spacecraft (SC) motion has been estimated at the IKI. ... The 30 days measuring intervals were used during the Tail probe (TP) orbital data treatment, and 15 days intervals - during the Auroral probe (AP) orbit determination. ... http://www.iki.rssi.ru/vprokhor/indap.htm for the Auroral probe; . http://www.iki.rssi.ru/vprokhor/indtp.htm for the Tail probe . ... http://www.iki.rssi.ru/vprokhor/ssc.htm , or http://www.iki.rssi.ru/vprokhor/amisan.htm . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/orbmod.htm -- 6.3 Кб -- 26.07.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/orbmod.htm -- 6.3 Кб -- 26.07.1999
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8. http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom/d-f/dmpits.txt
DMPITS.TXT 04-04-94 ~~~~~~~~~~~~~~~~~~~ DMPITS.ZIP CONTAINS THE FOLLOWING FILES: DMPITS.TXT (YOU'RE READING IT) DMPITS.BAT (STARTS PLAY) DMPITS.WAD (MODIFIED DOOM DATA FILE) COPY DMPITS.BAT AND DMPITS.WAD INTO YOUR DOOM DIRECTORY. ... THERE IS NO SKILL LEVEL CHOICE - THEY'RE ALL THE SAME DIFFICULTY. ... I SURE HOPE YOU GIVE IT A FEW TRYS WITHOUT USING THE CHEAT KEYS. ... DON'T GIVE INTO THOSE CHEAT KEYS. ... ACKNOWLEDGEMENTS ~~~~~~~~~~~~~~~~ THANKS TO THE FOLKS AT ID SOFTWARE FOR CREATING DOOM. ...
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom/d-f/dmpits.txt -- 3.4 Кб -- 29.07.1994
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9. 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_ ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PINTofALE/doc/EXAMPLE_Chandra.html -- 11.5 Кб -- 01.10.2012
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10. Investigator Email Change
... Follow the steps described below in order to make a change to an investigator's email address. Navigate to the program information web page for one of the investigator's observing programs and then click on the Investigators link. ... Select Profile Request and then work through the ProPer interface for changing a person's profile. Once you have completed the profile change, ProPer will display this page which shows that a change confirmation email has been sent to the investigator. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ops/investigator-email-change.html -- 3.4 Кб -- 26.02.2014
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11. FORS1 Photometric System Characterization
These observations are aimed at fully charactering FORS1 photometric system (UBVRI zero-points, color-terms and extinction coefficients) for the Tektronix 2048x2048 pixel CCD (24µm px) . To this aim, the two Landolt/Stetson photometric fields SA95 and SA101 will be observed on a number of epochs and at different airmasses during February and March 2007. ... SA101 . ... OBs for SA101 have to be observed during evenigh twilight (exceptions are expected for the second half of March) . ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~fpatat/fors/testphot2/ -- 10.8 Кб -- 12.03.2007
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12. http://lnfm1.sai.msu.ru/neb/nss/SatStar/expl-S.txt
... Byte-by-byte Description of files: star -S1.txt , star -S2.txt, star -S3.txt ------------------------------------------------------------------------------- Bytes Format Units Label Explanations 1- 4 I4 --- YYYY Year of the date 6- 7 I2 --- MM Month of the date 9- 10 I2 d DD Day of the date 13- 14 I2 h h Hour of the day 18- 24 F7,2 d JD* Julian day of the date , JD*=JD-2450000.5 28- 31 F4.1 degrees M-S Apparent distance between ...
[ Сохраненная копия ]  Ссылки http://lnfm1.sai.msu.ru/neb/nss/SatStar/expl-S.txt -- 3.0 Кб -- 17.02.2005
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13. Large_Scale Emitting Chains
... From the chain visibility point of view, it is very recommended to look at the Javascript movies , especially if the frame rate can be not regulated in your MPEG player. ... The non-CH-associated large-scale chains visible on the SOHO/EIT images at three wavelengths of 171, 195 and 284 as well as on the MLSO/HAO He I 10830 spectroheliogram of December 16, 1997. ... The SOHO/EIT movies at 171 and 195 show the chain dynamics on June 1-3, 1998. ... Javascript movie (230 KB), SOHO/EIT, 171 . ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/~ichertok/REALITY/index.htm -- 10.0 Кб -- 25.06.2012
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14. Rini Modified PlЖssl - MPL Eyepieces, care of Paul Rini, AstroGuide Listing
The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . Low cost beginner eyepieces. Send SASE for price list. ... Listed Since October 26, 2004 . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/astroguide/ag393.html -- 12.2 Кб -- 09.04.2016
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15. S.P. Korolev RSC Energia - International Space Station
... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... ISS Russian Segment . Steps of ISS Assembly . ... Five new devices of the total mass of ~42 kg (instead of 6 devices of the total mass of ~101 kg) are installed in the guidance, navigation and control system of the new series vehicle. ... liquid thermostatting of GN OC devices is provided by installation of three cold plates in the vehicle instrument module (IM); . ... 2015 JSC "S.P. Korolev RSC "Energia" . ...
[ Сохраненная копия ]  Ссылки http://www.energia.ru/en/iss/soyuz-tma-m/soyuz-tma-m_01.html -- 25.8 Кб -- 10.04.2016
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16. pulsedPwrIntoAlfa
... 18sep08: bias for 3a/3b changed. Look at p2030 data (polA,polB summed) . 21sep08: bias for all beams changed. ... The wapps in 3 level mode take 100 MHz bw with 64usec sampling and 256 lags. alfa is centred at 1440 Mhz with the 100 Mhz 1390-1490 filter int. The total power was computed and then averaged to .1 seconds. ... Beam 6b is dead and p2030 is adding polA + polB. ... The a2010 data taken on 21sep08 was analyzed to check the stability of all the beams after the bias changes in alfa. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/mbeam/biasChange_sep08.html -- 5.6 Кб -- 22.09.2008
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17. APOD: February 6, 1999 - The First Explorer
... February 6, 1999 . The First Explorer . ... Explorer I carried instrumentation to measure internal and external temperatures, micrometeorite impacts, and an experiment designed by James A. Van Allen to measure the density of electrons and ions in space. The measurements made by Van Allen's experiment led to an unexpected and startling discovery -- an earth-encircling belt of high energy electrons and ions trapped in the magnetosphere now known as the Van Allen Belt . ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap990206.html -- 4.4 Кб -- 02.10.2012
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18. Software Maintenance Manual
... Created: 23 February 2001 . ... SOFTWARE MAINTENANCE MANUAL . ... 9 January 2001 . ... Note: in the final document, the table of contents will be to third level] . The Software Maintenance Manual describes the procedures for installation and maintenance of the software for the Gemini Near-infrared Integral Field Spectrograph (NIFS). ... Section 19.4.3 of the document “Programmatic Requirements for Gemini Instrumentation Development” states the requirements for the Software Maintenance Manual . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/nifs/manuals/man0003.htm -- 139.3 Кб -- 06.09.2001
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19. RSOG Pre-Observation Products
Next: GOCG Pre-Observation Products . Previous: RadioAstron Mission Element Overview . ... Observation Summary File (OSF) . GRT (Ground Radio Telescope) Schedule Files . ... How: The long-term schedulers will produce two files: GSTS-file (General Space Telescope Schedule) to be used by GOCG and LTS-file for all mission elements. ... What: The RSOG will produce schedule files for all GRTs participating in a particular observation, in the format required by each GRT. ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/RadioAstron/documents/rmoh/eng/rsogpre.htm -- 7.2 Кб -- 16.05.2001
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20. Database of Optical Properties -- Level: subpage
This page will contain definitions (and basic references) of the following parameters: . cross-sections C ext , C sca , C abs , C bk ; . efficiencies Q ext , Q sca , Q abs , Q bk ; . ... TE/TM mode definitions for arbitrary shapes. Note that some parameters are defined in a quite different (specific) manner than for spherical scatterers, and some definitions in the book of Mishchenko et al. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/staff/ilin2/DOP-old/2-11.html -- 2.3 Кб -- 19.11.2010
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