Abstract
X-ray emission from solar coronal loops changes on two different timescales: a) flare loops and transient active region brightenings show a rapid variability, b) quiet region loops are quasi-steady and change only slowly with time. This different time behavior has been analyzed on the basis of Yohkoh SXT observations and we report here on the results from our analysis, mainly focussing on quiet loop variability.
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References
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© 1994 Springer Science+Business Media Dordrecht
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Hiei, E. (1994). Structure and Development of Quiet Loops in the Solar Corona. 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_33
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DOI: https://doi.org/10.1007/978-94-011-0930-7_33
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4401-1
Online ISBN: 978-94-011-0930-7
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