๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Noise storms and particular photospheric magnetic structures

โœ Scribed by C. Zanelli; P. Zlobec

Publisher
Springer
Year
1977
Tongue
English
Weight
432 KB
Volume
53
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

โœฆ Synopsis

A comparison of flux and polarization of solar radio noise storms with photospheric source position and magnetic field configuration for six year observations is reported. Three independent results pointing to a predominance of 'plus' magnetic structures as regards noise-storm generation are outlined. A rather strong proof towards a cause-effect connection of photospheric magnetic structure development and noise-storm evolution is stressed.

๐Ÿ“œ SIMILAR VOLUMES

Solar noise storms and magnetic sector s
Solar noise storms and magnetic sector structures
โœ R. T. Stewart ๐Ÿ“‚ Article ๐Ÿ“… 1985 ๐Ÿ› Springer ๐ŸŒ English โš– 746 KB

A synoptic study of the occurrence and polarization of 160 MHz noise storms recorded at Culgoora during the current solar cycle shows that the storm sources occur in large unipolar cells extending > 90 ~ in solar longitude and ~< 60 ~ in latitude, with lifetimes of ~ 1 yr. From solar maximum onwards