You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

... The ut1.dat file contains the corrections made to UT1R -TAI time which is used by the Tempo and Tempo2. ... The corrections are published monthly by the International Earth Rotation Service (IERS) in several IERS bulletins . ... This is done by downloading the eopc04_IAU2000.62-now from http://hpiers.obspm.fr/iers/eop/eopc04_05/ to $TEMPO2/earth directory. ... This produces a file ut1.tmp in the /iers directory . cd to $TEMPO2/clock/ and check that the local version of ut1.dat is up to date. ...

... This package contains a PERL script which takes a set of image mode OM ODF files in a single directory and processes them in a pipeline to produce OM image mode pipeline products see Section 9 . ... Through reading the SAS summary file, the perl scrip first produces a list of the filters for the OM data. ... It first checks to see if the exposure is a full-frame low resolution mode, and if so it runs omcomb to combine the four separate image segments into a single full-frame image. ...

Data Processing . S2 or VLBA tapes containing the astronomical data recorded at tracking stations and ground radio telescopes must be sent to correlation center chosen by the principal investigator (PI). ... There are four correlators, which will be able to process RadioAstron data: DRAO S2-correlators in Canada, NRAO VLBA-correlator in USA, and Mitaka correlator in Japan. ... Data and Phase Links . Ground Support of the RadioAstron . ... Progress of the RadioAstron Project in Pictures . ...

Processing Data Sets Based on Time History ========================================== Description: Use the time history of an instrument's observing program and calibration state as an additional factor in reprocessing data. ... NICMOS data are subject to persistence, in which detector pixels that collect a large number of counts in one exposure continue to 'glow' with a count rate that decays gradually with time, producing afterimages in subsequent images. ...

... We have defined a set of rules for classifying SUSI exposures according to the exposure type (BIAS, FF, SCI) and a set of rules for classifying them according to the optical path. ... The MIDAS session shown in Table creates these rules and applies them to our set of SUSI exposures (Table ). The result of the classification process is illustrated in Table . ... The table must contain the following columns: . ... Table: Classification Table for SUSI exposures (susi_rule.tbl) . ...