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Variations in 18-Mc/s solar and cosmic noise

Published online by Cambridge University Press:  14 August 2015

R. Fleischer
R. Fleischer*
Affiliation:
Observatory of Rensselaer Polytechnic Institute Troy, New York, U.S.A.

Extract

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Apparatus for measuring changes in the received intensity of 18–Mc/s cosmic noise has been in operation at the Sampson Station of the Observatory of Rensselaer Polytechnic Institute since 1957 February. It is similar in principle to the equipment of the High Altitude Observatory on which is based the contribution of the Warwicks [1] to this Symposium.

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 208 - 209
Copyright
Copyright © Stanford University Press 1959 

References

1. Warwick, C., and Warwick, J. W. Paper 37.Google Scholar
2. Fleischer, R., and Redlich, R. W. A. J. 62, 243, 1957.CrossRefGoogle Scholar
3. Fleischer, R., and Lichtenstein, P. R. Rensselaer Observatory Publications , Number 1, 1958.Google Scholar