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A Quantitative Method to Optimise Magnetic Field Line Fitting of Observed Coronal Loops

โœ Scribed by L. Carcedo; D.S. Brown; A.W. Hood; T. Neukirch; T. Wiegelmann

Book ID
111611905
Publisher
Springer
Year
2003
Tongue
English
Weight
252 KB
Volume
218
Category
Article
ISSN
0038-0938

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Observations of preburst heating and mag
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โœ Robert F. Willson ๐Ÿ“‚ Article ๐Ÿ“… 1984 ๐Ÿ› Springer ๐ŸŒ English โš– 731 KB

The Very Large Array (VLA) has been used at 20 cm wavelength to study the evolution of a burst loop with 4" resolution on timescales as short as 10 s. The VLA observations show that the coronal loop began to heat up and change its structure about 15 rain betbre the eruption of two impulsive bursts.