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- W171491557 abstract "Fluctuations of the radio radiation in the type II bursts of May 3, 1973 are analyzed on the basis of data obtained with the Weissenau (FRG) spectrograph in the range of 30--960 MHz and with the polarimeter of the Institute of Terrestrial Magnetism, the Ionosphere, and Radio-Wave Propagation, USSR Academy of Sciences at a frequency of 74 MHz. The characteristic time scale of these fluctuations at 74 MHz decreases during an event from 2--5 to 1--3 sec. It is shown that the origin of the fluctuations is connected with the presence in the corona of heterogeneities of the magnetic field and the electron density. The heterogeneities consist of formations strongly drawn out along the surface of the sun. Their radial dimensions are l/sub parallel/(2--7) x10/sup 8/ cm and they grow with an increase in distance from the sun. The transverse dimensions of the heterogeneities are l/sub perpendicular10/ cm." @default.
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- W171491557 date "1977-01-01" @default.
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- W171491557 title "Fine Structure of the type II solar radio burst of May 3, 1973" @default.
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