Abstract
This paper presents a short summary of observations of coronal structures at microwaves using an instrument with high spatial resolution and good wavelength coverage. The comparison of the RATAN-600 data with optical observations of coronal loops in the green line and with the Very Large Array maps at 21 cm has shown that the loops represent only a small part of coronal matter, although their role may be of great importance in the physics of the solar corona. Prominence (filament) associated sources, especially “peculiar” ones, are also reviewed.
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© 1994 Springer Science+Business Media Dordrecht
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Korzhavin, A.N., Bogod, V.M., Borovik, V.N., Gelfreikh, G.B., Makarov, V.I. (1994). Coronal Loops and Prominences as Observed With Ratan-600. In: Fleck, B., Noci, G., Poletto, G. (eds) Mass Supply and Flows in the Solar Corona. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0930-7_34
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DOI: https://doi.org/10.1007/978-94-011-0930-7_34
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