... an especially great enhancement of the backgroundmicrowave emission (the so-called ... The microwavebackground S-component was strongly enhanced as Violent solar events ...
... Thus, the presence of dark stripes is related to the absorption of the backgroundmicrowave emission rather than to the absence of light stripes (in the emission). ...
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Ссылки http://www.izmiran.rssi.ru/~gchernov/SolSys5_08ChernovLO.pdf -- 1272.2 Кб -- 03.08.2008 Похожие документы
... Thus the presence of dark stripes is connected not with the absence of bright stripes (in emission), but with an absorption of backgroundmicrowave emission. ...
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Ссылки http://www.izmiran.rssi.ru/~gchernov/Chernov_AA437_1047_05.pdf -- 2303.3 Кб -- 27.12.2005 Похожие документы
... They showed that the circular polarization of the SSP is usually opposite in sign to the associated microwave bursts. ... the SSP emission in the ordinary sense, because the background burst appeared mostly due to gyrosinchrotron emission of ...
... eruption of a large CME against the background of several active regions and other ... completely missing from the RD image (the region will have the background intensity ...
... and absorption stripes against the continuum background of the solar type IV radio ... of the fine structure in the microwave range have recently been revealed with the ... The origin of fibers against the ZS background also was not considered. ...
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Ссылки http://www.izmiran.rssi.ru/~gchernov/PlasPhys4_05ChernovLO.pdf -- 981.9 Кб -- 09.03.2005 Похожие документы
... The blobs consisting the microwave chains are characterized by the angular sizes of 30-60 arcseconds and the brightness temperature of about (11-13)x10^{3} K (at 17 GHz the brightness temperature of the undisturbed background Sun is (10.3-10.8)x10^{3} K). ...
... and absorption bands seen against the background of the type IV radio continuum ... Emission and absorption bands against the background of the type IV continuum are ...
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Ссылки http://www.izmiran.rssi.ru/~gchernov/chernovAstRep40(4)96.pdf -- 892.0 Кб -- 28.10.2002 Похожие документы