... GHRS IMAGEs and MAPs are obtained with the focus diodes (see Section on page 80 ) at the ends of the array of main science diodes. ... An IMAGE can only record the light in the 1.74 1.74 arcsec region of the LSA. ... A standard IMAGE will have a pixel spacing of 0.109 arcsec and will cover the entire LSA aperture of 1.74 1.74 arcsec. You may also select pixel spacings of 0.055 or 0.027 arcsec, with proportionately smaller regions of the sky covered in a 16 16 (the default) IMAGE. ...

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• Decadal Survey ASTRO 2010 - Requests for Information responses submitted to the
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The HyperNews Linux KHG Discussion Pages . Forum: Supporting Functions . Keywords: request_irq . Date: Tue, 29 Oct 1996 14:54:25 GMT . From: Robert Wilhelm < robert@physiol.med.tu-muenchen.de > . request_irg() and free_irq() seem to take a new parameter in Linux 2.0.x. What is the magic behind this? . Messages . 1. dev_id seems to be for IRQ sharing by Steven Hunyady .

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. Minsk bibliography on light scattering . Related Internet resources . (under construction) . Here we will give links to such Internet resources as follows: . SCATLIB . contains lists of references to papers devoted to calculations of light scattering by particles of different shapes . and so on. To homepage . © 1990,2001 Victor Babenko (Bibliography compiling) . © 2001 Serge Beletsky (Design & Programming) . E-mail: serge@cyteg.com . Last updated: 2001/10/30

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This module provides the ability to set environment variables based upon attributes of the request. ... The mod_setenvif module allows you to set environment variables according to whether different aspects of the request match regular expressions you specify. ... BrowserMatch . ... Syntax: BrowserMatch regex env-variable [= value ] [ env-variable [= value ]] .. ... Module: mod_setenvif . ... The BrowserMatch directive defines environment variables based on the User-Agent HTTP request header field. ...

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infile,s,a, ./tmp/acis_evt2_filtered.fits ,,, Input file to get meta data from mission ,s,a, ,,, Name of mission instrument ,s,a, ,,, Name of Instrument detector ,s,a, ,,, Name of Detector (- if not required ) filter ,s,a, ,,, Name of Filter (- if not required ) ...

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... The e-mail interface of the CATS is designed like CGI for the call of the basic procedures: select and match from the html-forms and the program is a lexical analyser, distinguishing keywords and parameters from the electronic letter sent to the address `cats@sao.ru'. ... The output of result is forseen in the same formats as in other forms of the access to the CATS. ... out[put] < arg1 arg2... > . ... ra [ < arg1 > ] < arg2 > < arg3 > ... min max [center] . ... window < arg1 arg2 ... > . ...

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... Telescopes, instruments and cameras are keenly affected by local weather and atmospheric conditions. The decision to open any telescope or have access to any instrument or camera is at the sole discretion of the on-duty observing specialist(s) at the time of your requested access. ... Specific parameters exist for access to APO telescopes, instruments, or cameras which protect our highly-sophisticated and sensitive equipment and provide safe work conditions for staff and visitors. ...

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... Since July 1993 all observations collected by the 1.82m telescope at Cima Ekar (Asiago) are systematically archived on DAT cartridges and a listing of collected data, including all parameters of the observations, is maintained in a relational DBMS. ... A user willing to retrieve data from the archive must send the list of requested observations (that must include the keyword `` CODICE '') to the archive maintainer who will forward it to the technical staff at the Asiago Observatory. ...

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• VLT Data Quality Control
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APIRET rc = Dos32Profile ( ULONG func, PID pid , PRFCMD *profcmd, PRFRET *profret); 0 NO ERROR ok 8 NOT_ENOUGH_MEMORY couldn't allocate profile structures 87 INVALID_PARAMETER some parameter not ok 111 BUFFER _OVERFLOW not enough size in return buffer 115 PROTECTION_VIOLATION invalid return buffer data 126 MOD_NOT_FOUND requested module data not available 303 INVALID_PROCID parameter 2 is not a valid PID 328 SYS_INTERNAL ... pid of process to be profiled 0 if kernel profiling . ...

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The Interball-Tail KP archive is final. ... Select a day: . Data available since August 3, 1995) . ... DAY . ... Magnetic field (PRAM) Electron density and mean energy (ELECTRON) Ion density, velocity and temperature (CORALL) Energetic particle fluxes (DOK-2 and SKA-2) H+ and O+ fluxes (PROMICS) AKR intensity (AKR) Antisunward ion flux (VDP) Plasma wave amplitudes (MIF-M/PRAM) PC index (Ground-based) INTERBALL-TAIl orbit . ... Now data in all formats are available for 1995-2000) . GIF plot . ...

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• Trapped Radiation -- History
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... AMPLE (Adaptable Minor Planet Ephemerides) is integrated software package to deal with a number of problems concerning minor planets with the aid of IBM-type personal computer. ... compiling a list of all numbered minor planets which can be seen at certain moment within specified sky region and visualization of their mutual positions; . ... As AMPLE is able to reproduce virtually any table of "the Ephemerides of Minor Planets" , it may be considered as computer version of the EMP. ...

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• (Untitled)
• Conference WPLTN-2012 | Conference page