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The orientation of magnetic fields in quiescent prominences

โœ Scribed by E. Tandberg-Hanssen; Ulrich Anzer

Publisher
Springer
Year
1970
Tongue
English
Weight
322 KB
Volume
15
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

We have measured the longitudinal component, Bll, of the magnetic field in quiescent prominences and obtained a relationship between BII and 0, where 0 is the angle between the long axis of the prominence and the north-s0uth direction on the sun. From this relationship we deduce a distribution function for the magnetic field vector in quiescent prominences in terms of the angle c~ between the field and the long axis of the prominence. The mean angle, &, for our data is small, ~ 15 ~ indicating that the magnetic field traverses quiescent prominences under a small, but finite angle.

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