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Solar observations by the large pulkovo radio telescope at 3.2-cm wavelength

Published online by Cambridge University Press:  14 August 2015

V. Ikhsanova
V. Ikhsanova*
Affiliation:
Pulkovo Observatory, Leningrad, U.S.S.R.

Extract

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The observations of the sun by the large Pulkovo radio telescope [1] began in 1956 December. In accordance with the antenna dimensions, a fan-beam diagram about one minute of arc in width and one degree in height was expected (at λ = 3.2 cm).

Type
Part II: The Sun
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 171 - 173
Copyright
Copyright © Stanford University Press 1959 

References

1. Khaĭkin, S. E., and Kaĭdanovskiĭ, N. L. Paper 29.Google Scholar
2. Ikhsanova, V. N. Izv. Obs. Pulkovo , 21, 29, 1958.Google Scholar
3. Waldmeier, M. Z. Ap. 31, 304, 1953.Google Scholar
4. Kakinuma, T. Proc. Res. Inst. Atm. Nagoya U. 4, 78, 1956.Google Scholar