๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

A comparison of type III solar radio burst theories using satellite radio observations and particle measurements

โœ Scribed by Larry G. Evans; Joseph Fainberg; R. G. Stone

Publisher
Springer
Year
1971
Tongue
English
Weight
330 KB
Volume
21
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis

The required electron density to excite a type III solar burst can be predicted from different theories, using the low frequency radio observations of the RAE-1 satellite. Electron flux measurements by satellite in the vicinity of 1 AU then give an independent means of comparing these predicted exciter electron densities to the measured density. On this basis, one theory predicts the electron density in closest agreement with the measured values.

๐Ÿ“œ SIMILAR VOLUMES

A comparison of type III metric radio bu
A comparison of type III metric radio bursts and global solar potential field models
โœ Bernard V. Jackson; Randolph H. Levine ๐Ÿ“‚ Article ๐Ÿ“… 1981 ๐Ÿ› Springer ๐ŸŒ English โš– 391 KB

We compare evidence of coronal magnetic fields from polarized metric type III radio bursts with (a) global potential field models, (b) direct averages of the observed photospheric magnetic field, and (c) Ha synoptic charts. The comparison clearly indicates both that the principal aspects of type III