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Solar radio blips and X-ray kernels

✍ Scribed by Benz, A. O.; Fürst, E.; Hirth, W.; Perrenoud, M. R.

Book ID: 109722956
Publisher: Nature Publishing Group
Year: 1981
Tongue: English
Weight: 239 KB
Volume: 291
Category: Article
ISSN: 0028-0836
DOI: 10.1038/291210a0

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A slowly evolving, flaring loop was observed by the UVSP, XRP, and HXIS instruments onboard SMM on June 10, 1980. Simultaneous radio observations from Toyokawa (Japan) are also available. The SMM instruments have an angular resolution ranging from 3 to 30 arc sec by which the loop structure may be d