... few remaining hot pixels are the ones due to the micrometeoroid impacts, although much less hoter, than before , both in terms of PHA (energy) and recurrence frequency, (for instance, the MOS1 rev 325 meteoroid defects which are all located in CCD 6 & 7 ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0149-1-3.ps.gz -- 89.7 Кб -- 11.12.2003 Похожие документы
... alpha line onto RGS defect · Meteor shower avoidance : Perseids (Revs.490 and 491) and Leonids (Revs.538 and 540) avoidance probable meteoroid impact occurred on Rev.490 few-frame flash seen on MOS2: no lasting effects seen in the following days the ...
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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
... Data Systems Division 9 Research & Scientific Support Department Page 9 XMMNewton OPERATIONS All instruments essentially stable MSG LEOP took out Revs. 1105 to 1110 Rev.1147 HotBird and SpainSat support We're probably due another (micro)meteoroid ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200605/LMetcalfe.pdf -- 2728.8 Кб -- 14.05.2014 Похожие документы
... 1985, "Collisional balance. of the meteoritic complex", Icarus 62, 244-272 N. Divine, 1993, Five populations of interplanetary meteoroids, J. Geophys Res., ...
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Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf -- 673.9 Кб -- 10.11.2005 Похожие документы