... 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 . ...

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• The INTERBALL Tail PROBE orbital elements
• The INTERBALL Auroral PROBE orbital elements collections

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Murchison Radio-astronomy Observatory . ... Parkes radio telescope . ... Mopra radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... For example, modified Newtonian dynamics (MOND) has no relativistic extension, and so makes no firm lensing predictions, but galaxy-galaxy lensing data can be used to empirically constrain the deflection law of a MONDian point-mass. ...

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

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
• List of Tables

MAIN CHARACTERISTICS BASIC MODIFICATIONS TEST RESULTS . ... integrated drop tests in order to verify the strength of DM modified shell and equipment attachment points, functional check of new chairs and DM structure, determination of shock impacts onto the crew to verify landing safety; . ... nominal landing with the main parachute system (MPS) - drop #1 took place on December 24, 1998; . ... reduction of shock g-loads values at landing in accordance with decrease of landing speeds. MAIN | ...

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• S.P. Korolev RSC Energia - International Space Station

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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... Exposure time per pixel (i.e., the integration time which contributes to the counts in each pixel), for the whole observation, or a given group. ... FPKTTIME 2 - group_elapsed_time . ... Group exposure time per pixel . ... Exposure time for the observation: This is the total time during which the FOS accumulated data for the observation and is given in the header keyword EXPTIME. ... The total exposure time for the entire observation (all groups) is given by the keyword EXPTIME in the data header. ...

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• Index of /ftp/observing/completed_observations
• WFC3 Data Handbook

For all keywords that contain a red and a blue value, the blue value comes first. ... The full pathname, but without the trailing "b.fit" and "r.fit", that would be given to the next exposure if the basename argument is not given to the expose command. ccdHeaters=float,float . ... bluelambda2=float [M] . The center wavelength for the given grating: the 1 or 2 indicates the grating bay. The bluelambda and redlambda keywords match one set of these, depending on the position of the turret. ...

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• Agile ICC Version History
• emerg_close

This page was created by the IDL library routine mk_html_help . ... mk_html_help . at the IDL command line prompt. ... to calculate CHIANTI line intensities and continua, to create a synthetic spectrum. ... WRITTEN : Ver.1, 7-Nov-01, Giulio Del Zanna (GDZ) and Peter Young (PRY) MODIFICATION HISTORY: V.2, 7-Nov-01, GDZ . Fixed a small bug (now the spectrum plot is always plotted within the widget), and modified the option to add continua. ... Added extended details in the ascii output spectrum. ...

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• NEAR recorded on 23 January 1998(frame 1)
• FIRPO Help 5
• FIRPO Runs

chandra_acis_ao9.par ; generate an ACIS spectrum for a source using a DEM , ; and optionally rescale the DEM to produce the same ; counts as a ROSAT / PSPC observation ; ;calling sequence ; .run initale ; @chandra_acis_ao9.par ; ;(LL/VK; modified from chandra_acis_ao5.par, Feb04) ;(LL ... density [cm^-3] T_components = [6.9, 7.4] ;log(T[K]) components in the EM EM_components = [5.1d12, 6.1d12] ;Emission Measure [cm^-3] obs_rate = 0.1 ; ROSAT / ...

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• http://hea-www.harvard.edu/PINTofALE/ardb/chandra_acis_ao7.par
• Modifying the SAOtng GUI
• PINTofALE EXAMPLE : Simulation for Chandra ACIS-I

... 30 Mar 2004 Corrected : jo1031.html, jo1031.txt, fjupoout.html ----------- 22 Mar 2004 jo1033.txt, so1012.txt Modified : (Column 'Old Ident' erased) fjupoout.html , fsapoout.html , fjupogal.html, fjupoinn.html, fmapomai.html, fnepomai.html, fnepoout.html , fsapoinn.html, fsapomai.html, furpoinn.html, furpomai.html , furpoout.html ----------- 20 Feb 2004 jo1032.txt Modified : fjupoout.html ----------- 15 Jan ... Line with jo0024 in the file fjupoout.html was corrected. ...

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... 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. ...

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• Geomagnetic Kp Index
• Geomagnetic ap, Ap, Cp, and C9 Indices
• Geomagnetic Indices Kp, ap, Ap, Cp and C9

In 2001, Westerbork observations of the disturbed galaxy named VV-29 (alias Arp-188, UGC-10214) showed that there is second smaller galaxy (named VV-29c) that appears behind the western side of the main body of the distorted galaxy. ... The galaxy was featured as the May 2, 2002 Astronomy Picture of the Day . ... When VV-29 had its 15 minutes of fame in May 2002, it appeared under the name "The Tadpole Galaxy," but based on the images above, we will always think of it as "The CHAINSAW"! ...

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• Designated Observatory Application
• Designated Observatory Registry
• IAU Commission #34 (Interstellar Matter)

New precession formula . ... It gives the precession-nutation matrix as the product of four rotational matrices as NP = R 1 (- ) R 3 (- ) R 1 ( ) R 3 ( ) and the precession one similarly as P = R 1 ( - ) R 3 (- ) R 1 ( ) R 3 ( ) . Here and are the angles to specify the location of the ecliptic pole of date in the given inertial frame, and are the true and mean ecliptic angles of precession, respectively, and and are the true and mean obliquities of the ecliptic, respectively. ...

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• Keywords_102
• Keywords_28

... 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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• CMEs and Space Weather
• Chains and CMEs

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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Home - News - Download - Documentation - Search - FTP . About NEdit . ... Download . Get NEdit . ... nedit man page . ... Mirror Sites . ... Christian Denat . ... Back ] . ... Select word/line/file ( modified ) . ... Project macros ( modified ) ( new ) . ... Find definition ( new ) ( new ) . Find definition dialog ( new ) ( modified ) . ... Trace IF / ELSE / END IF ( modified ) ( new ) . Fold C/C++ ( modified ) ( modified ) . ... Element functions ( modified ) [ Back ] . ...

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• comedi_command_test
• NEdit
• comedi_get_cmd_generic_timed

XmCCD Copyright 2007-2012 John Kielkopf ======================================= Development Log =============== March 9, 2002 Version 1.0.0 * Support for SBIG cameras using the first public SBIG library * Basic panel for operation with ds9 +--------------------------+ May 22, 2002 Version 1.1.0 * Updated to use libudrv 4.35 +--------------------------+ May 24, 2004 Version 1.2.0 * USB support +--------------------------+ March 1, 2005 ...

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• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.1/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/CHANGELOG
• http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.2.2/CHANGELOG

... We demonstrate through numerical simulations that model parameters estimated with our technique are essentially bias-free, even when the average number of counts per bin is 1. ... The IW technique avoids such biases by estimating through successive iterations, where for each iteration, j, , and the best-fit parameters are determined by minimization of . ... In our sample, we find that the minimum values and best-fit parameters converge after about 6 iterations. ...

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• (Re-)Configurable Data File Writing At UKIRT
• NICMOS Calibration Pipeline: Processing Associations of Exposures
• ADASS 2002 Conference Proceedings

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. ...

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• http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom2/d-f/egypt.txt
• http://crydee.sai.msu.ru/ftproot/pub/rec/games/idgames/levels/doom2/a-c/burzum1.txt
• Use of program libraries