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    • 1 | 2 | След.

    1. http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-9.ps.gz
    ... the boresight was scheduled once after every eclipse seasons and once per year after ... Both of the 15 ks total time visits should be split into three 5 ks pointings: pn in ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-9.ps.gz -- 179.2 Кб -- 31.03.2008
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    2. http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-11.ps.gz
    ... the boresight was scheduled once after every eclipse seasons and once per year after ... Both of the 15 ks total time visits should be split into three 5 ks pointings: pn in ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001-2-11.ps.gz -- 118.2 Кб -- 09.01.2009
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    3. http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001.pdf
    ... eclipse) OM photometry (raster) EPIC gain/offset & eff. area RGS wavelength scale RGS eff area (coord), OM photometry, EPIC (parasitically) spectr. capab. & contam. -----------------------------------------------------------------------------o s C n e te ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-PL-0001.pdf -- 194.6 Кб -- 13.07.2015
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    4. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-7.pdf
    ... The situation is different for abnormal conditions like the eclipse seasons or during solar flares. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-7.pdf -- 1722.6 Кб -- 11.08.2008
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    5. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-4.pdf
    ... Abnormal conditions include the eclipse seasons and solar flares (marked by the vertical lines in figures 1-11, 1-12), where the gain at the beginning of an orbit (i.e. during calibration observations) can vary significantly from the gain for the ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-4.pdf -- 1346.2 Кб -- 14.02.2005
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    6. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201403/freyberg-cal-2014.pdf
    ... frame times: 25 MHz oscillator (2014) Total difference of the effective frequency of ... External events like eclipse seasons or RGS switch offs are indicated; dotted ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201403/freyberg-cal-2014.pdf -- 1763.9 Кб -- 24.04.2014
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    7. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-1.pdf
    ... the stepwise degradation after solar flares · · · · · · Refined calculation of the ... ured in-orbit radial profile introduce a systematic error of ~2% of total counts ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-1.pdf -- 1574.9 Кб -- 04.04.2003
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf
    ... Solar flares created a series of jumps in the CTE of the EPIC-MOS cameras prior to the cooling described above, while the EPIC-pn CTE degrades independently of solar flares at a nearly constant rate per year as seen in Fig. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0062-1-0.pdf -- 673.9 Кб -- 10.11.2005
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    9. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-0.pdf
    ... to compensate the stepwise degradation after solar flares Degradation of the MOS ... in-orbit radial profile, introduce a systematic error of ~2% of total counts ... better than 5% in the determination of the total effective area is reached over the ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-0.pdf -- 2175.1 Кб -- 12.08.2002
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    10. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-2.pdf
    ... Abnormal conditions include the eclipse seasons and solar flares (marked by the vertical lines in figures 1-11, 1-12), where the gain at the beginning of an orbit (i.e. during calibration observations) can vary significantly from the gain for the ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0018-2-2.pdf -- 1829.9 Кб -- 12.07.2004
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