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Occultations of the Crab Nebula by the Solar Corona in June 1957 and 1958

OB Slee
12(2) pp.134 - 156


14 articles found in Crossref database.

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Turbulent Proton Heating Rate in the Solar Wind from 5–45 R ⊙
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Low-Frequency Radio Observations of the Angular Broadening of the Crab Nebula Due to a Coronal Mass Ejection
Ramesh R., Kathiravan C., Sastry Ch. V.
The Astrophysical Journal. 2001 548(2). p.L229
An Anisotropic Density Turbulence Model from the Sun to 1 au Derived from Radio Observations
Kontar Eduard P., Emslie A. Gordon, Clarkson Daniel L., Chen Xingyao, Chrysaphi Nicolina, Azzollini Francesco, Jeffrey Natasha L. S., Gordovskyy Mykola
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Scintillation studies of cosmic source angular structure (Review)
Zhuk I. N.
Radiophysics and Quantum Electronics. 1980 23(8). p.597
Radio synthesis imaging of anisotropic angular broadening in the solar wind
Anantharamaiah K. R., Gothoskar Pradeep, Cornwell T. J.
Journal of Astrophysics and Astronomy. 1994 15(4). p.387
Properties of solar wind turbulence deduced by radio astronomical measurements
Hollweg Joseph V., Harrington J. V.
Journal of Geophysical Research. 1968 73(23). p.7221
80 MHz Observations of the Coronal Broadening of the Crab Nebula
Harries J. R., Blesing R. G., Dennison P. A.
Publications of the Astronomical Society of Australia. 1970 1(7). p.319
Scattering of radiowaves from cosmic sources in the solar corona
Baselyan L. L., Sinitsin V. G.
Solar Physics. 1971 17(1). p.129
The Interplanetary Medium (1972)
Vitkevich V. V.
Solar-Terrestrial Physics/1970 (1972)
Vitkevich V. V.
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