... Version 1.34.3 - 2002-11-05 (CB) -------------- Minor ammendment made to perl script for SPR 3016 Version 1.34.2 - 2002-11-05 (CB) ------------- Perl scrip ammended to fix problem identifying engineering-4 data (fixes SPR 3016) Version 1.34.1 - 2002-10-22 (CB) ------------- Configuration file ammended for omdetect version 4.1 (fixes SPR 3001) Version 1.34 - 2002-10-17 (CB) ------------- Uploaded for release track ... Intermediate file names changed so that they aren't overwritten. ...

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• Output Columns modified

... select data groups menu . activate fields (radio buttons) to qualify the query . ... select menu option to record query selections, enter a unique report option name and save option . ... select Visit Data menu from data groups menu . ... select LRP menu from data groups menu . activate LRP name "query" radio button and select LRP 02035A from automatically activated dropdown menu . ... select LRP menu from data groups menu and select LRP 02036A from automatically activated dropdown menu . ...

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• Python: module build_PRD_dataset
• Modifying a USC
• Problem Statement

Last modified: 10 November 1998 . ... Modified: . ... We expect observations will resume on November 16. Any additional changes which must be made in the HALCA schedule will be communicated as quickly as possible. We expect some changes because the HALCA observing efficiency may drop about 25% for the next few months, and because of the rescheduling of some missed observations. This WEB page contains the schedule for HALCA observations from November 16, 1998 to February 28, 1999. ...

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• In-Orbit Checkout/GOT Schedule
• lbaops:tidnotes:fileprep [ATNF VLBI Wiki]
• VLBI Wiki | TidNotes / FilePrep

... 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. ...

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• Rhiannon Zoe Nolan Howell November 2002
• Rhiannon Zoe Nolan Howell 1998 November
• x111 idl routines

... 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 . ...

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• Chains and CMEs

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" . ...

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• Modifying An Acuter Digitial Imager - an Astronomy Net Astrophotography Forum

Next: The Quasi--Newton Method. Up: Outline of the Previous: The Newton--Raphson Method. ... At each iteration, one computes . ... Neglecting the second derivatives matrix , we obtain the ``normal equations'' and the Gauss--Newton direction . This so--called Gauss--Newton method is intended for problems where is small. ... The algorithm implemented here is a modification of that Gauss--Newton method, that allows convergence even for rank deficient Jacobians or for large residuals. ...

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• NVSS radio survey
• Modification of Tables
• MJD --- column label: MJD_OBS

This is a new popup window - close it when you are done . ... 1st image with new camera, canon 450d which was modified for use in astrophotography. Scope wo 80mmfd mount cge my original camera now in the shop for shutter repair, unguided 33x180sec calibrated with deep sky stacker and post processed in Photoshop cs3 captured the evening of November 11th 2010 from the overly lit skies above my observatory 42.36.01n 71.17.53w . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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... 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" . ...

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• INTERNATIONAL SPACE STATION
• S.P.Korolev RSC Energia - LAUNCHERS

... Sun images . ... Active areas . November : 2015 . ... 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 November 09, 2015 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 November 09, 2015 00:31 UT . ...

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• Sunspots and active regions November 10, 2010
• Sunspots and active regions November 01, 2015
• Sunspots and active regions November 10, 2005

HARP-B is a heterodyne focal plane imaging array working at 325 - 375 GHz, built for the JCMT at MRAO in collaboration with the ATC in Edinburgh and the HIA in Canada. ... December 2005 - Harp-B being commissioned at the JCMT. Dec 11TH - First Light! ... November 2005 - Harp-B is installed at the JCMT . Last Modified 11th December 2005 by Jane Buckle . Harp Webpage Administrator at the Cavendish Astrophysics Server. ...

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• Galaxy Evolution: Publications submitted
• Mini-seminars: Michaelmas 2005
• Graca Rocha - Talks

... 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 . ...