... Here, we describe this phenomenon, characterize it with averages and correlation functions, and interpret it as the result of decorrelation of the impulseresponse function of interstellar scattering between the widely-separated antennas. ... The average envelope of correlations of the visibility function show two exponential scales, with characteristic delays of 1 = 4.1 ± 0.3 µs and 2 = 23 ± 3 µs, indicating the presence of two scales of scattering in the interstellar medium. ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/publications/articles/tmp/arx1501.04449.pdf -- 2235.8 Кб -- 16.03.2016 Похожие документы
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Ссылки http://solarwind.cosmos.ru/txt/2011/presentations/Sun/Ishkov/apj_691_2_1222.pdf -- 1208.5 Кб -- 15.04.2011 Похожие документы
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