Dependence of the flare stream velocity on magnetic field orientation |
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Authors: | M I Pudovkin S A Zaitseva S P Puchenkina |
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Institution: | (1) Radiophysical Research Institute, Gorky, U.S.S.R. |
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Abstract: | The stationary current of diffusely-distributed super-thermal electrons along a weakly inhomogeneous coronal magnetic field is considered as a possible model of the noise storm continuum source in decametric wavelengths. It is shown that the realization of such a streaming leads to a considerably increased level of plasma noise in the diffuse component region and then to enhanced radio emission from this region. |
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