... CFPL are easy to understand, they take into account all the processes of emission and absorption in line formation, energy exchange between Stokes parameters intensity etc. ...
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Ссылки http://www.uafo.ru/publ/gao/2012GAOconf_289_292_Mozharovsky.pdf -- 269.8 Кб -- 15.01.2013 Похожие документы
... between H and hard X-ray emissions during impulsive solar flares// Solar Phys. 1985 ... Soft X-ray, Microwave, and hard Xray emission from a solar flare: implication for ...
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Ссылки http://www.uafo.ru/publ/uafo/2008UAFO_11_104_111_Kuzmenko.pdf -- 2088.9 Кб -- 01.02.2013 Похожие документы