Wave propagation in the warm plasma and the spectrum of the solar radio bursts |
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Authors: | L Mollwo |
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Institution: | (1) Zentralinstitut für solar-terrestrische Physik (HHI) der DAW, Berlin-Adlershof, D.D.R. |
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Abstract: | The frequency bands of noise storms and type I-bursts as well as of type IVdm-bursts are shown to be in accordance with the consequences of a recently proposed mechanism (Mollwo, 1970). An explanation results of the observed spectral minimum near 600 MHz and interpretations are supposed of some features of type III- and of type IVmA-bursts. The magnetic field strength over active regions in two corona levels is deduced, too. The discussion leads to a conception of the corona parameters in the level of type IV-bursts which suggests an origin of these bursts by absolute instability of space charge waves. |
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