Occultation of a noise storm source during the partial solar eclipse of May 20, 1966-Reference-Cited by-同舟云学术

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Occultation of a noise storm source during the partial solar eclipse of May 20, 1966

Published:1967-06 Issue:3-4 Volume:1 Page:474-477
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Letfus V.,Tlamicha A.,Valníček B.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00151371.pdf

Reference6 articles.

1. Christiansen, W. N., Yabsley, D. E., and Mills, B. Y.: 1949, Austr. Journ. Sci. Res. A2, 506.

2. Covington, A. E.: 1947, Nature 159, 405.

3. Daene, H.: 1966, private communication.

4. Fokker, A. D.: 1966, private communication.

5. Gelfreich, G., Korol'kov, D., Rishkov, N., and Soboleva, N.: 1959, Paris Symposium on Radioastronomy (ed. by R. N. Bracewell). Stanford University Press, Stanford, Calif., p. 125.

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The First Low-frequency Radio Observations of the Solar Corona on ≈200 km Long Interferometer Baseline;The Astrophysical Journal;2018-03-01

2. RADIO OBSERVATIONS OF THE SOLAR CORONA DURING AN ECLIPSE;The Astrophysical Journal;2011-03-09

3. Observation of the solar eclipse 1966 May 20 in the region between 3.2 cm to 2.7 m wavelength;Astronomische Nachrichten;2007-07-10

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