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    • 1. Generation from Ground Calibration Data
    ... and spectral information of the zodiacal light emission is taken from literature ... 1) The spatial distribution of the zodiacal light is contained in the ZODIACAL_MAP ... The zodiacal light spectrum (essentially solar) is compiled from literature and ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node965.html -- 8.9 Кб -- 20.09.2011
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    2. http://xmm.vilspa.esa.es/external/xmm_sw_cal/background/files/OMbackg05.pdf
    ... Q LA (Counts/sec. sq.arcsec) BPM16274 Diffuse Galactic Zodiacal Light (Counts/sec. sq.arcsec) Light (Counts/ sec. sq.arcsec) thrp. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/background/files/OMbackg05.pdf -- 149.4 Кб -- 24.04.2006
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    3. http://xmm.vilspa.esa.es/external/xmm_sw_cal/background/files/MSSLbckgd_v6.pdf
    ... 10-6 10 white 0.214 290 Table 3: Results of the DGL background. filter latitude (o ) 90 0 minimum maximum 3 Zodiacal Light Zo diacal light (Bz l ) is due to sunlight scattered by interplanetary dust particles, and is seen at ultraviolet, optical and near ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/background/files/MSSLbckgd_v6.pdf -- 118.6 Кб -- 19.04.2006
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    4. Generation from In-Orbit Data
    ... However on the longterm it will be possible to estimate the diffuse background components (DGL and Zodiacal light). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node962.html -- 3.7 Кб -- 20.09.2011
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    5. Generation from In-Orbit Data
    ... However on the longterm it will be possible to estimate the diffuse background components, namely DGL and zodiacal light (cf. section 4.5.13 ). ...
    [ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/calibration/documentation/CALHB/node966.html -- 3.3 Кб -- 20.09.2011
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    6. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0019-1-0.ps.gz
    ... background count rate in the OM is dominated by the zodiacal light in the optical ... The zodiacal light level depends on space coordinate. ... This is because, for these lters, the zodiacal light level is negligible. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0019-1-0.ps.gz -- 410.9 Кб -- 02.07.2002
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    7. http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0022-1-0.ps.gz
    ... and om zodiacal keep an intensity map, the average spectrum and an estimate of the expected photon 1 XMM­Newton CCF Release XMM­CCF­REL­22 Page: 2 rate for the different filter elements of the diffuse galactic light and the zodiacal light respectively ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-SRN-0022-1-0.ps.gz -- 47.0 Кб -- 03.01.2001
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    8. http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0001-1-0.ps.gz
    ... The zodiacal light appears as a truly diffuse source with G­type spectrum, varying from a magnitude of 23.4 to 21.6 per square arcsec, so the equivalent ranges per pixel are: 23.2 to 21.4 (MOS) and 20.4 to 18.6 (PN). ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/docs/documents/CAL-TN-0001-1-0.ps.gz -- 81.1 Кб -- 08.07.2008
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    9. http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/csim.ps
    ... the X-ray background model. max magn The maximum bound for the magnitude distribution.. ux The 0.25-12 keV X-ray background ux. units The units for the ux (photon s 1 mm 2 or eV s 1 mm 2 ). zodiacal The zodiacal light level. di use The di use light level ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/csim.ps -- 652.6 Кб -- 12.01.2005
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    10. http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/osim.ps
    ... The background is made up of two components, the zodiacal light and the di use galactic background. ...
    [ Текст ]  Ссылки http://xmm.vilspa.esa.es/scisim/release/latest/help/postscript/osim.ps -- 1009.1 Кб -- 12.01.2005
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