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On the possibility of observing radio emission from flare stars

Published online by Cambridge University Press:  14 August 2015

E. Schatzman
E. Schatzman*
Affiliation:
Institut d'Astrophysique and Faculté des Sciences de Paris, France

Extract

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Strong radio emissions are associated with solar flares. It seems worth while, therefore, to examine whether radio emission associated with flares and eruptions in nonstable stars could be observed. The first problem in this respect is establishing the threshold of sensitivity necessary to receive anything during an eruption or a flare; the second one is naturally fixing the duration of the radio emission, which can be much shorter in a given wavelength than the optical emission.

Type
Part VI: Mechanisms of Solar and Cosmic Emission
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 552 - 553
Copyright
Copyright © Stanford University Press 1959 

References

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