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ROSAT Status 116
ROSAT Status Report #116
Feb 6 1995
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= =
= ROSAT NEWS No. 35 --- 1-Feb-1995 =
= =
=-----------------------------------------------------------------------=
= ROSAT Scientific Data Center at the =
= Max-Planck-Institut fuer Extraterrestrische Physik (MPE) =
= Postfach 1603, D-85740 Garching, Germany =
=-----------------------------------------------------------------------=
= e-mail addresses (Uli Zimmermann): =
= rosat_svc@mpe-garching.mpg.de (Internet) or MPE::ROSAT_SVC (SPAN) =
= ROSAT Service Area (including ROSAT Data Archive): =
= ftp rosat_svc.mpe-garching.mpg.de user: anonymous =
= WWW address: http://rosat_svc.mpe-garching.mpg.de/ =
= interactive account (including ROSAT Result Archive): =
= telnet xray.mpe-garching.mpg.de user: xray no password =
=-----------------------------------------------------------------------=
= XUV Center: 29382::GXUVDC or GXUVDC@AIT.PHYSIK.UNI-TUEBINGEN.DE =
= WFC Archive access via telnet/ftp ait.physik.uni-tuebingen.de =
= user: xuv (password: xuv_archive) =
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SATELLITE STATUS/MISSION PLANNING
=================================
An imperfection in the mission planning procedure was identified which
led to the scheduling of 'impossible' observing slots implying a loss
on the order of 5 % of the total and 13 % of the time critical observing
time. This imperfection is related to the constrained mobility of the
satellite which requires sun sensor information for any slew or target
acquisition procedure. While in general the mission planning accounts
for this constraint, and does not foresee any target changes on the
night side of the satellite orbit, there is still one particular case
in which 'impossible' observing slots were scheduled. This case can be
characterized as follows:
1) a target was previously acquired on the day side;
2) it then underwent a temporary earth block after which its observation
was to be continued (with no target changes inbetween);
3) the earth block either ended after the night began or so shortly
before the beginning of the night that no re-acquisition was possible
on the day side.
In such cases observing slots after the end of the earth block
erroneously appeared in the mission timeline, but the targets could not be
acquired, and the slots were not used. This situation affects time-
critical observations more strongly than non-time critical ones for which
the optimized mission planning procedure is likely to avoid earth blocks
anyway.
In the forthcoming mission timeline for the second part of AO5 (beginning
in April 1995) this special case will be treated properly, and we expect
an overall increase in observing efficiency. However, we stress that
these 'impossible' slots are a result of the degraded attitude control
system and will remain unavailable. This is especially important for
time-critical observations which have become more difficult to carry out.
If in the future you will find other observations scheduled at the
time-critical period you asked for in your proposal, it will be because
there were 'impossible' slots for your target which were used otherwise.
EXSAS
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Release 95JAN of the EXSAS software has been tested within the MIDAS
94NOV environment for the UNIX systems on AXP (OSF), HP, IBM, SUN,
SUN Solaris, and DECstations (ULTRIX). The software may be copied from
the ROSAT Service Area. Tests on the VMS and the LINUX systems are
underway.
====================== end of ROSAT NEWS ================================