... The parameter dialog presents you with the parameters that the task will use. ... list parameters . ... In general, the edit field field is preceded by a label , specifying the name of the parameter. ... If that is the case, a pull-down menu is shown next to the edit field of that parameter. Other parameters may have a browse button next to the edit field . Clicking on this button will pop-up a browser , in which you can select the value of this parameter by browsing through your file system. ...

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• Change history

Next: Mass change Up: Evolutionary Scenarios of Binary Previous: Stellar Winds From Normal . As mentioned earlier, the duration of the binary evolutionary stage (say, I+I) is determined by the faster evolving component , where is the time each component spends at the corresponding evolutionary stage. ... Next, we should calculate the mass change for the slower evolving companion, the orbital semi-major axis and the eccentricity. Mass change . Semi-major axis change . ...

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• Mass change
• Dependence on the Scenario Parameters and Initial Distributions
• Semi-major axis change

... 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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• INTERBALL-TAIL KP

... This section is intended to help you decide whether your data were calibrated with optimal calibration reference files and to help you decide whether you need to recalibrate your data. ... The calibration software is completely data-driven, meaning that the calibration steps to be carried out are determined by the values of the calibration switches and the calibration reference files keywords contained in the primary header of the file to be processed. ... To edit the calibration keyword values: . ...

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• STSDAS release notes
• WFPC2 Header Changes due to OPUS 10.0 Update
• Recipe Editor GPI Data Pipeline 1.0 documentation

... Main / . TEMPO2 is a pulsar timing software package. ... TEMPO2 requires a timing model for each pulsar being studied. ... TEMPO2 also requires a file containing the pulse arrival times for the pulsar being studied. ... With a pulsar timing model (e.g., 1539.par) and a set of pulse arrival times (e.g., 1539.simulate), TEMPO2 can be used to calculate and display the pulsar timing residuals. ... f 1539.par 1539.simulate: provides the timing model (1539.par) and the arrival times (1539.simulate) . ...

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• Unified Radio Catalog: results for Version 1.1
• Package: mt
• Changing the task context

... 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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• Parameters
• Changes for release 1.8
• Possible Pitfalls

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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... A number of parameters appear in the parameter area which correspond to the status of the package when the interface is created. These parameters can be changed by typing the new values in the field, or reading them from a previously saved session table. The option in the menu may be used to read a session file. The name of the currently loaded session is indicated in the first text field Session at the top of the parameter area in the Main window. ...

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• Format of the table for atomic parameters (ABSP.TBL).
• Setting, Storing, and Retrieving the CCD Keywords
• Upgrading to 2.2 from 2.0 - Apache HTTP Server

... Apache HTTP Server Version 2.4 . ... Session encryption support . ... session_crypto_module . ... The session will be encrypted with the given key. Different servers can be configured to share sessions by ensuring the same encryption key is used on each server. ... The SessionCryptoPassphrase directive specifies the keys to be used to enable symmetrical encryption on the contents of the session before writing the session, or decrypting the contents of the session after reading the session. ...

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• Upgrading to 2.2 from 2.0 - Apache HTTP Server
• Where are the tunable parameters of the kernel?
• API Changes in Apache HTTP Server 2.4 since 2.2 - Apache HTTP Server

... 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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• POLIMODEL (V2.00) --- November00 --- POLIMODEL (V2.00)
• OYSTER Lab
• Parameters

... 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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• Arecibo Observatory L-Wide Band Receiver
• CIMA Data Taking Modes
• The Mock Spectrometer

Full-Text Search in PostgreSQL: A Gentle Introduction . ... Fast Backward . ... ALTER FULLTEXT DICTIONARY -- change a full-text dictionary . ALTER FULLTEXT DICTIONARY dictname RENAME TO newdictname ; ALTER FULLTEXT DICTIONARY dictname SET OPTION opt_text ; . ALTER FULLTEXT DICTIONARY change an existing full-text dictionary. dictname . The name (optionally schema-qualified) of the dictionary to rename. newdictname . The new name of the dictionary. ... CREATE FULLTEXT DICTIONARY . ...

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• ALTER FULLTEXT PARSER
• ALTER FULLTEXT CONFIGURATION
• LIC plug-in

Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...

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Fortran 90 properties already in CF77 . ... Only the old form (fix form) of the source code is available. ... LOGICAL Default KIND number = 8 INTEGER Default int7 int15 KIND number = 6 1 2 digits = 46 7 15 radix = 2 2 2 range = 13 2 4 huge = 70368744177663 127 32767 bit_size = 46 8 16 INTEGER int31 int46 int64 KIND number = 4 6 8 digits = 31 46 63 radix = 2 2 2 range = 9 13 18 huge = 2147483647 70368744177663 9223372036854775807 bit_size = 32 46 46 REAL half Default,single double KIND ...

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• Backward and Forward compatibility
• Argument association
• XFree86/OS2 project

... 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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• Database of Optical Properties -- Level: subpage
• Circular polarization: change of sign
• AI SPbU library of scattering codes

OptInt PmWiki : Pm Wiki / Available Actions . Default actions . ... Cookbook actions . Page actions are applied to wiki pages, as a query string appended to the URL . ... displays dialog for setting/changing password of the specified page or group of pages, see passwords , see also $EnablePostAttrClearSession if you do not want to have the session cleared after validating change General use of passwords . ... display the specified page (default action if no ?action= is present) . ...

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• OptInt PmWiki : PmWiki / Changes From Pm Wiki 1
• OptInt PmWiki : Available Actions
• OptInt PmWiki : Changes From Pm Wiki 1

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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• Astrophysical Research Consortium - Apache Point Observatory
• Appendix B
• Changes from the Old TCC

. Sitemap . Contact . Search . Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . by . Enric Pall . Big Bear Solar Observatory . A colloquium presented at Armagh Observatory on 2006 February 1st. The slides from this presentation are available in the following formats. HTML in your browser . PDF file - 14MB . Quicktime movie - 9MB . Macromedia Flash - 9.7MB . MS Powerpoint - 12MB . Last Revised: 2009 December 17th .

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• sfit help file
• Armagh Observatory
• Influence of Climate Variables on Tree-Ring Widths of Different Species

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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• ASP: An Ancient Universe - Changes in Stars
• ASP: An Ancient Universe - Changes in the Solar System
• ASP: An Ancient Universe - Changes in the Universe

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

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