... This means that objects like Venus and Mars are good sources for such measurements, but that Jupiter is somewhat less so because of limb darkening. ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/publications/2006/OOFP1.pdf -- 270.3 Кб -- 25.11.2009 Похожие документы
... variations siuppplas ets atypothesis thatwe t hreserecresefollosuesawilaut tes piuivalielnts. for planets withgure> 4R Fitghe elatforr 8d<riRed b10Rumming i ns of jupiter s ze ortn the h i c ofciro-pumvwing l tho r hi q leup, distribution-with CB njecti ...
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Ссылки http://www.mrao.cam.ac.uk/wp-content/uploads/2014/04/DArmstrong.pdf -- 1314.9 Кб -- 22.04.2014 Похожие документы
... Astrophys. 334, pp. L5L8, June 1998. 8. M. Mayor and D. Queloz, "A Jupiter-Mass Companion to a Solar-Type Star," Nature 378, pp. 355+, Nov. 1995.. ...
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Ссылки http://www.mrao.cam.ac.uk/projects/OAS/publications/fulltext/spie4838-16-letter.pdf -- 129.8 Кб -- 20.02.2013 Похожие документы
... study of Solar System bodies, the Atacama Large Millimeter/submillimeter Array (ALMA; Hills et al. 2010) will be able to map the shape and surface temperature distributions of hundreds of main belt asteroids and Jupiter Trojans (Busch 2009; Lovell 2008 ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/publications/2015/1503.02650v2.pdf -- 291.9 Кб -- 04.03.2016 Похожие документы
... As mentioned for BOOMERANG, calibration is diфcult at the pole (e.g. Jupiter is always near the horizon) but the DASI team report a nal calibration uncertainty of approximately 3.5%. ...
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Ссылки http://www.mrao.cam.ac.uk/~anthony/capetown_paper/lasenby.ps -- 1071.4 Кб -- 01.05.2002 Похожие документы