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Bursts of microwave radio emission associated with solar flares

Published online by Cambridge University Press:  14 August 2015

G. B. Gelfreich ,
V. N. Ikhsanova ,
N. L. Kaĭdanovskiĭ ,
N. S. Soboleva ,
G. M. Timofeeva  and
V. N. Umetskiĭ
G. B. Gelfreich
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
V. N. Ikhsanova
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
N. L. Kaĭdanovskiĭ
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
N. S. Soboleva
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
G. M. Timofeeva
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.
V. N. Umetskiĭ
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.

Extract

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Bursts of solar radio emission which coincide in time with solar flares are occasionally observed over the whole frequency range up to 35,000 Mc/s. The purpose of this paper is to describe briefly some bursts observed at Pulkovo at wavelength λ = 3.2 cm.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 218 - 221
Copyright
Copyright © Stanford University Press 1959 

References

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