๐”– Bobbio Scriptorium
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The stability of sunspot magnetic fields and the origin of solar flares

โœ Scribed by Kunitomo Sakurai

Book ID
107843152
Publisher
Elsevier Science
Year
1971
Tongue
English
Weight
609 KB
Volume
19
Category
Article
ISSN
0032-0633

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๐Ÿ“œ SIMILAR VOLUMES

Motion of sunspot magnetic fields and it
Motion of sunspot magnetic fields and its relation to solar flares
โœ Kunitomo Sakurai ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 323 KB

The magnetic polarity distributions in sunspot groups which produced solar proton flares have been analyzed. It is shown that the fluid motion in sunspot groups and below may be responsible for the origin of inverted or unusual polarity distributions, since rotating motion in these spot groups is of

Stimulated dissipation of magnetic disco
Stimulated dissipation of magnetic discontinuities and the origin of solar flares
โœ E. N. Parker ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 768 KB

It is proposed that the principal cause of the confined solar flare is the dissipation of magnetic energy at the many small-scale pre-existing tangential dscontinuities in the local bipolar magnetic field. The discontinuities are a consequence of the continuous shuffling and intermixing of the footp