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Coronal Structures Observed at Meter Wavelengths

Published online by Cambridge University Press:  30 March 2016

P. Lantos
Affiliation:
Observatoire de Meudon, 92190 Meudon, France
C.E. Alissandrakis
Affiliation:
University of Athens, Athens (621)Greece

Abstract

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Two dimensional maps obtained with the Nançay Radioheliograph at 169 MHz from 1980 are used to describe and identify the features of the quiet sun at meter wavelengths.

Type
Joint Commission Meetings
Copyright
Copyright © Reidel 1986

References

References:

Alissandrakis, C. E., Lantos, P., NicoLaïdis, E., 1985, Solar Physics, 97, 267.Google Scholar
Axisa, F., Avignon, Y., Martres, M.J., Pick, M., Simon, P. 1971, Solar Physics, 19, 112.Google Scholar
Dulk, G.A., Sheridan, K.V., 1974, Solar Physics, 36, 191.Google Scholar
Kerdraon, A., Mercier, C., 1983, Astron. Astrophys. 127, 132.Google Scholar
Pye, P., Evans, K.D., Hutcheon, R.J., Gerassimenko, M., Davis, J.M., Krieger, A.S., Vesecky, J.F., 1978, Astron. Astrophys. 65, 123.Google Scholar
Radioheliograph Group, 1983, Solar Physics, 88, 383.Google Scholar