Physics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77..255f&link_type=abstract
Solar Physics, vol. 77, Apr. 1982, p. 255-261.
Physics
4
Broadband, Decimeter Waves, Radiant Flux Density, Solar Radiation, Type 4 Bursts, Fine Structure, Magnetic Flux, Solar Corona
Scientific paper
The different and constantly changing patterns in type IV decimeter continuum broadband absorptions and emissions is ascribed to a mechanism that affects the propagation of the radiation on its way outwards through the corona. Inferences are drawn that the whole source is affected by a switch-off-and-on mechanism, that the size of the source is at most of the order of the product of the typical time of flux increase or decrease and the speed of light, and that the radiations at the various frequencies change virtually simultaneously. The process involved may be a screening of a large part of the outgoing beam of radiation ducted along a channel of relatively low density. All the broad band features should be discussed in terms of a phenomenology of possible structures of shocks, solitons, and series or trains thereof.
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