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Study of Ribbon Separation and Magnetic Reconnection Rates in a Two-Ribbon Flare

✍ Scribed by W. Xie; H. Zhang; H. Wang

Publisher
Springer
Year
2008
Tongue
English
Weight
772 KB
Volume
254
Category
Article
ISSN
0038-0938

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πŸ“œ SIMILAR VOLUMES

A numerical experiment relevant to line-
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✍ T. G. Forbes; E. R. Priest πŸ“‚ Article πŸ“… 1983 πŸ› Springer 🌐 English βš– 953 KB

The nonlinear evolution of a reconnecting magnetic field configuration similar to that occurring just before the onset of'post'-flare loops in two-ribbon flares is determined. The evolution, which is obtained by numerically solving the resistive MHD equations, shows two new features that have not ye

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A great He two-ribbon flare of 12 October, 1981 was observed with the Domeless Solar Telescope at the Hida Observatory and its detailed photometry was made with a two dimensional microdensitometer. The principal results are as follows: (1)The impulsive phase of the flare started with the progressive

Spectrograph, filtergraph and magnetogra
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✍ A. G. Michalitsanos; P. Kupferman πŸ“‚ Article πŸ“… 1974 πŸ› Springer 🌐 English βš– 875 KB

We present high resolution detailed observations of the class 3N two-ribbon flare of 1973, July 29 (McMath 12461), which was associated with the disappearance of a large filament ('disparition brusque'). This flare occurred in a diffuse bipolar magnetic region completely devoid of sunspots, and was