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|Title:||Microwave & Hard X-ray Emission during Solar Flare of 19 Oct 1981|
|Authors:||Verma, V K|
|Abstract:||Time correlation study of a double ribbon flare, observed on 19 Oct. 1981, in the light of H-, microwave and hard X-ray data is presented. The kinetic energy of electrons required to emit hard X-rays is nearly 104 times that of those electrons which produce microwave emission. arc sec, respectively, and the kinetic energy involved in flare strand separation turns out to be 6.2 1027 erg sec-1.|
|ISSN:||0975-105X (Online); 0367-8393 (Print)|
|Appears in Collections:||IJRSP Vol.13(5) [October 1984]|
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