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Rapid fluctuations in the position, size, and brightness of intense solar metre-wave radio sources

✍ Scribed by R. A. Duncan


Publisher
Springer
Year
1985
Tongue
English
Weight
836 KB
Volume
97
Category
Article
ISSN
0038-0938

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✦ Synopsis


A comparison of quiescent type I solar radio sources with concurrent intense impulsive type III, V, and type II sources shows that whereas the type I sources are usually small and stable the type III, V, and II sources are usually large and unstable. We conclude that the large size and variability of the type III, V, and II radio sources cannot be attributed to instrumental error or ionospheric refraction but must instead reflect the size and variability of the coronal structures on which they arise.