๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Inferences of plasma parameters from coronal hole observations

โœ Scribed by Shadia Rifai Habbal


Publisher
Springer Netherlands
Year
1996
Tongue
English
Weight
632 KB
Volume
243
Category
Article
ISSN
0004-640X

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Coronal magnetic field patterns inferred
โœ M. F. Lantos-Jarry ๐Ÿ“‚ Article ๐Ÿ“… 1970 ๐Ÿ› Springer ๐ŸŒ English โš– 316 KB

A noise storm center clearly associated to an active center has been followed from January 2 to January 8, 1969. The study of the mean distribution of continuum and of type 1 bursts has shown a global and systematic displacement interpreted in terms of the coronal magnetic structure. This structure

Meterwave observations of a coronal hole
โœ Z. Wang; E. J. Schmahl; M. R. Kundu ๐Ÿ“‚ Article ๐Ÿ“… 1987 ๐Ÿ› Springer ๐ŸŒ English โš– 518 KB
Observation of a coronal hole at 85 GHz
โœ M. R. Kundu; Sou-Yang Liu ๐Ÿ“‚ Article ๐Ÿ“… 1976 ๐Ÿ› Springer ๐ŸŒ English โš– 253 KB

A coronal hole was observed at 85 GHz(3.5 mm-h) on November 24, 1970, when a spectacular coronal hole was observed in soft X-rays by AS&E. The miUimeter counterpart of the hole is much weaker and less widespread than in X-rays. The brightness temperature inside the hole was in most places about 100-