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Variations of Flaring Kernel Sizes in Various Parts of the H⍺Line Profile

✍ Scribed by K. Radziszewski, P. Rudawy

Book ID: 120777779
Publisher: Springer
Year: 2012
Tongue: English
Weight: 464 KB
Volume: 284
Category: Article
ISSN: 0038-0938
DOI: 10.1007/s11207-012-0192-5

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## Abstract Large solar telescopes built at places with a quite excellent seeing, equipped with a sophisticated optics and control system are too expensive and unique to be used currently in hunting of sudden and short‐lasting activity events, e.g. flares and eruptive prominences. For a systematic