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    • Пред. | 1 | 2

    11. http://www.mrao.cam.ac.uk/projects/OAS/oi_data/DataExStd_rel3_nov02_letter.pdf
    ... These estimates should include the effect of the earth's atmosphere, but not the spectrum of the target (the effect of the target spectrum should be taken into account as part of any model-fitting/mapping process, i.e. the target spectrum is part of the ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/DataExStd_rel3_nov02_letter.pdf -- 45.2 Кб -- 11.01.2008
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    12. http://www.mrao.cam.ac.uk/projects/OAS/oi_data/OIFITS_PASP.pdf
    ... These estimates should include the effect of the Earth's atmosphere, but not the spectrum of the target (the effect of the target spectrum should be taken TABLE 6 OI_VIS (Revision 1) Label OI_REVN .. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/oi_data/OIFITS_PASP.pdf -- 70.0 Кб -- 11.01.2008
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    13. http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie4838-162-letter.ps
    ... For ground-based long-baseline optical and infrared interferometers, the Earth's atmosphere introduces random path-length uctuations of many tens of microns with a timescale as short as a few milliseconds. ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie4838-162-letter.ps -- 1693.2 Кб -- 20.02.2013
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    14. http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.OldDocs/INT-403-ENG-0006.pdf
    ... 11 For a V=16 star with a flat electromagnetic spectrum in the visible region, we could approximate the number of photons (F1) reaching the earth's atmosphere as: F1 = 2 ( m1 - m2 ) / 5 F 100 Where F2 = 9480 photons cm-2 s-1 nm-1, m1=16 and m2=0 ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.OldDocs/INT-403-ENG-0006.pdf -- 377.3 Кб -- 28.04.2010
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    15. http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf
    ... However, the presence of the Earth's atmosphere affects this argument. ... In particular, the Earth's atmosphere perturbs the differential paths to the array ... Aberrations introduced by the Earth's atmosphere will reduce the fringe contrast by ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.Requirements/INT-402-MIS-0000.pdf -- 1989.2 Кб -- 25.06.2007
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    16. http://www.mrao.cam.ac.uk/~jsy1001/thesis.pdf
    ... be seen by conventional optical and infrared tel bulence in the Earth's atmosphere ... flux at the top of the Earth's atmosphere from a star with an apparent magnitude of ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~jsy1001/thesis.pdf -- 2354.4 Кб -- 20.07.1999
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    17. http://www.mrao.cam.ac.uk/~bn204/publications/2009/ALMAMemo590.pdf
    ... focuses on the dispersive part of the wet path delay introduced by the atmosphere ... of the physical parameters of the atmosphere and what constraints can be placed on ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2009/ALMAMemo590.pdf -- 908.6 Кб -- 10.08.2012
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    18. http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2009/ALMAMemo587.pdf
    ... three-parameter model of the atmosphere; using the absolute measurements from the ... fluctuation of the properties of the Earth's troposphere along the lines of sight of ...
    [ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2009/ALMAMemo587.pdf -- 1202.6 Кб -- 25.11.2009
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    Пред. | 1 | 2

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