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http://xmm.vilspa.esa.es/sas/5.4.1/doc/evlistcomb/ChangeLog.
http://xmm.vilspa.esa.es/sas/5.4.1/doc/evlistcomb/ChangeLog.
1. http://xmm.vilspa.esa.es/sas/6.0.0/doc/emenergy/ChangeLog
... Version 8.1.1 - 2004-03-12 (JB) ------------- - Parameter rejectbade3e4 was incorrectly called rejecte3e4 in doc. ... Makes use of new OFFSETS extension. ... Use badpixutils_mod. ... Version 2.5 - 27-11-1998 ----------- - Fixed SPR 335 (The function change_case is duplicated in other tasks). ... Version 2.4 - 25-09-1998 ----------- - Changed output format for CCD background map and time series. ... Version 2.0 - 20-07-1998 ----------- - Fixed SPR 334 (Change on/off parameters from integer to boolean...
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Ссылки http://xmm.vilspa.esa.es/sas/6.0.0/doc/emenergy/ChangeLog -- 8.5 Кб -- 12.03.2004
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2. WFPC2 Header Changes due to OPUS 10.0 Update
... WFPC2 Header Changes due to OPUS 10.0 Update . ... Data . ... WFPC2 Home . ... OPUS 10.0 includes a major change for the WFPC2 and FOC science data processing pipelines in OPUS. ... FITS standard TELESCOP keyword is added to all headers. ... The header positions of the DATE, FILETYPE, INSTRUME, and EQUINOX keywords have changed. ... How to identify OPUS 10.0 headers for WFPC2 and FOC: . FLTSWVER and OPUS_VER keywords, which are in the STIS and NICMOS FITS spt headers, are not in WFPC2 or FOC shh. ...
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Ссылки http://www.stsci.edu/hst/wfpc2/analysis/opus_ten.html -- 17.3 Кб -- 10.04.2016
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3. Changing the task context
. The context of a task can be changed using a pop-up menu that can be activated with the sequence ESC S : . The following context parameters can be changed with this menu: . error level: 1-4 . message level: 1-4 . output mode: normal, expert or test . screen output: on or off . log file output: on or off . hide ``hidden'' keywords: on or off To change the context of a running task, its name must be present in the User Command Area. If the UCA is empty, the template context will be changed.
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Ссылки http://www.atnf.csiro.au/computing/software/gipsy/hermes/changecontext.html -- 1.9 Кб -- 17.01.2009
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4. Editing Files and Parameters
... eparam* - edit parameter files . ... Type ``<esc>-?'' within a parameter editor for more details on commands. *tupar* - Edit table headers . Table files (* .tab ) consist of a header including a variety of parameters and the table itself. It is possible to edit the header using tupar and the table with tedit provided you have write-access to the file. ... Works like emacs but uses <ctrl> D to exit. *hedit* - edit image file header . qphedit* - edit .qp file headers . ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node11.html -- 5.8 Кб -- 01.10.2012
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5. Initializing Keywords
Next: Short Help Up: Graphical User Interfaces Previous: Graphical User Interfaces . The parameter area is used to set and display the various parameters used by the context. These parameters may be either defined by the user or defaulted by the context. User defined parameters are set or changed by simply moving the mouse cursor to the relevant field and typing in the value. The corresponding SET/LONG command is sent to MIDAS as soon as the mouse is moved out of the field. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node524.html -- 2.8 Кб -- 23.02.1996
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6. http://www.eso.org/~qc/concept/MEF_QC.pdf
... Scoring Necessary step towards more automated certification Idea: · define key QC1 parameters , check new values against trending for those · evaluate compliance: o if new within defined range, ok o if outside: nok · user may focus on nok ones, while ok is certified automatically in `confidence mode ' Required: · configure set of key parameters per product · configure comparison mode o fixed: ...
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Ссылки http://www.eso.org/~qc/concept/MEF_QC.pdf -- 49.3 Кб -- 07.08.2006
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7. ALTER FULLTEXT PARSER
Full-Text Search in PostgreSQL: A Gentle Introduction . Prev . Fast Backward . Fast Forward . Next . ALTER FULLTEXT PARSER -- change a full-text parser . ALTER FULLTEXT PARSER prsname RENAME TO newprsname ; . ALTER FULLTEXT PARSER changes an existing full-text parser. prsname . The name (optionally schema-qualified) of the parser to rename. newprsname . The new name of the parser. ... CREATE FULLTEXT PARSER . ... DROP FULLTEXT PARSER . ... ALTER FULLTEXT .. ...
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Ссылки http://www.sai.msu.su/~megera/postgres/fts/doc/sql-fts-alterparser.html -- 4.5 Кб -- 13.04.2008
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8. INTERBALL-TAIL KP changes
... New version of magnetic field data (descriptor "itm") is now available with small corrections in offsets and attitude coverage. ... Full set of INTERBALL-TAIL AKR radiointensity KP for AKR instrument is now available (descriptor "ita"). ... KP data availability plots are created. ... Magnetic field data (descriptor "itm") after 1st January, 1998 are recomputed with corrected Bx_GSE offset (this was just 0.5 nT correction). ... CDF files for plasma wave KP are now available (descriptor "itw"). ...
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Ссылки http://www.iki.rssi.ru/apetruko/kppnews.html -- 3.2 Кб -- 27.10.2003
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9. IKI SSC, INTMINS APRIL99
Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...
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Ссылки http://www.iki.rssi.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
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10. http://www.mrao.cam.ac.uk/~eic22/ALMAmemos/memo590/dispersivephase.py
Emily Curtis eic22@mrao.cam.ac.uk Script for working with ATM dispersive phase for Memo 590 import os import string import numpy from atmtools import * System variable parameters ... #Users' output directory dcval = 0.01 #Change in water vapour to compute change in path /mm fmin = 0 #Minimum frequency to compute phase /GHz fmax = 1000 #Maximum frequency to compute ...
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Ссылки http://www.mrao.cam.ac.uk/~eic22/ALMAmemos/memo590/dispersivephase.py -- 7.4 Кб -- 11.11.2009
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11. Echelle for Beginners
Contact Russet McMillan (primary) or your Observing Specialists (secondary) for additional information. Contact Jack Dembicky for web page errors, corrections, ommisions, or additions. This page last updated: July 6, 2004 - JMD . This page last checked: September 14, 2003 - JMD . Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . Taking your Calibration lamps . ... Setting up multiple exposures . ... Stopping an exposure (discarding data) . ...
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Ссылки http://www.apo.nmsu.edu/35m_operations/35m_manual/Instruments/Echelle/Basics_HTML_Pages/Using_Echelle_with_TUI.html -- 4.5 Кб -- 27.10.2004
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12. Where are the tunable parameters of the kernel?
The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Date: Thu, 15 May 1997 08:10:29 GMT . From: < demiguel@robot3.cps.unizar.es > . I need to find the tunable parameters of the linux kernel, bue i cant find them (filesystems, processes, swapping,...) . I would like to know if there is any files such as mtune, or dtune is System V where you can change the main tunable parameters. Thank you everybody!! . Messages . 1. Kernel tunable parameters by Jukka Santala .
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Ссылки http://www.arcetri.astro.it/irlab/doc/library/linux/khg/HyperNews/get/khg/64.html -- 2.6 Кб -- 23.03.2000
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13. 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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14. Arecibo Observatory Narrow S-Band Receiver (2.24-2.42 GHz)
... S-Band Radar (2.24 - 2.42 GHz) . ... Receiver History . Contact Info . ... It is normally left in the higher range, which is the band used by the Arecibo Planetary radar. If you expect to need to adjust it, contact us in advance to make sure that it's working. [back to top] . ... Info . ... To see an up-to-date plot of Tsys, just type tsys on your terminal after logging into Arecibo's computer network. [back to top] . ... The lower filter (2.24-2.34) is not well characterized. [back to top] . ...
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Ссылки http://www.naic.edu/~astro/RXstatus/Sradar/Sradar.shtml -- 12.4 Кб -- 03.02.2013
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15. Backward and Forward compatibility
Very important in the introduction of a new programming language standard is that old programs (at least those who obey the outgoing standard) can be used once again, with the new standard. When we went from Fortran 66 to Fortran 77 the extended DO -loop was removed (the extended DO -loop means that if you do not change any of the DO -loop parameters you can jump out of the loop and then jump in again (this is somewhat contrary to the concept of structured programming). ... 2, June 1993, page 1. ...
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Ссылки http://star.arm.ac.uk/f77to90/a4.html -- 5.4 Кб -- 30.03.1996
[ Сохраненная копия ] Ссылки http://crydee.sai.msu.ru/f90/a4.html -- 5.4 Кб -- 30.03.1996
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[ Сохраненная копия ] Ссылки http://crydee.sai.msu.ru/f90/a4.html -- 5.4 Кб -- 30.03.1996
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16. Linear polarization: wavelength dependence
... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...
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Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node7.html -- 18.9 Кб -- 19.11.2010
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17. http://www.adass.org/adass/proceedings/adass02/reprints/P7-13.pdf
... DIRT uses results from a number of numerical models of astrophysical processes, and has an AWT based user interface. ... This pro ject is an example of refactoring with no impact on user interface, so the existing user community was not affected. ... Rationale for Refactoring DIRT is a powerful tool for searching pre-calculated models to fit observed data. ... Before refactoring, model data was represented within the user interface using Database and Record ob jects. ... Refactoring DIRT 383 Figure...
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Ссылки http://www.adass.org/adass/proceedings/adass02/reprints/P7-13.pdf -- 437.8 Кб -- 11.03.2003
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18. IJEventListener (ImageJ API)
... Class . ... PREV CLASS NEXT CLASS . FRAMES NO FRAMES All Classes . ... FIELD | ... METHOD . DETAIL: FIELD | ... public interface IJEventListener . ... Field Summary . static int . ... Field Detail static final int FOREGROUND_COLOR_CHANGED . ... Constant Field Values . static final int BACKGROUND_COLOR_CHANGED . ... static final int COLOR_PICKER_CLOSED . ... static final int LOG_WINDOW_CLOSED . ... static final int TOOL_CHANGED . ... Method Detail void eventOccurred (int eventID) . ...
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Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/IJEventListener.html -- 12.6 Кб -- 02.12.2010
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19. http://www.astro-soc.odessa.ua/
... Astronomical Observatory, Shevchenko Park, Odessa, 65014, . ... The XVI -th G. Gamow's Odessa Astronomical Summer Соnference-School, 14-20 August, 2016, Odessa, Ukraine . ... The XV -th G. Gamow's Odessa Astronomical Summer Соnference-School, 16-23 August, 2015, Odessa, Ukraine . ... The XIV -th G. Gamow's Odessa Astronomical Summer Соnference-School, 17-23 August, 2014, Odessa, Ukraine . ... The XIII -th G. Gamow's Odessa Astronomical Summer Соnference-School, 19-25 August, 2013, Odessa, Ukraine . ...
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Ссылки http://www.astro-soc.odessa.ua/ -- 16.6 Кб -- 15.03.2016
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20. Example of changing a password with the passwd command
To change your password: passwd Old password: enter your current password New password: enter your new password Retype new password: re-enter your new password . Enter the command passwd and then respond to the prompts by entering your old password followed by your new one. ... The passwords will not appear on the screen as you type, to prevent other people from seeing them. If you make a mistake, the message Mismatch - password unchanged. is displayed and your password remains unchanged. ...
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Ссылки http://comet.sai.msu.ru/UNIXhelp/basics/basic3.1.html -- 2.3 Кб -- 17.01.1997
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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