... occur after Perigee; min 0.5 h to max 56 min (at the end of the eclipse season) · Base-line for eclipse operations being outlined with the MOC: meeting foreseen on 12-06 · Target: keep start of instrument Observations (i.e. close cal obs) at Perigee + 4.5 ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200106/casale_ops_status.pdf -- 90.0 Кб -- 14.05.2014 Похожие документы
... EMOS2 HKPARMINT 0010.CCF 20141106T15:15:00 20141223T20:55:00 HKPARMINT NO 2 Changes During the 2014 winter eclipse season, gaps in ground station coverage around perigee resulted in delays in stabilising to the nominal MOS focal plane (FP) temperature ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0324-1-0.ps.gz -- 221.5 Кб -- 02.02.2015 Похожие документы
... The time dependency prepares for future use, when parameterizations of time dependent misalignments (e.g. due to relaxations after slew and/or perigee passages) become available. ...
... The time dependency prepares for future use, when parameterizations of time dependent misalignments (e.g. due to relaxations after slew and/or perigee passages) become available. ...
ACTIONS · EPIC_10/1 on Munoz. ... EPIC_9/2 on Altieri: to provide new CCFs reflecting the current MOS bad pixels. ... Commitment to maintenance. · new portal for calibration : · Capella cross- calibration with Chandra: GRB021004 killed first effort...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200302/metcalfe_030203_sciops.pdf -- 1334.3 Кб -- 14.05.2014 Похожие документы