Published 1982 | Version v1
Journal article

June-July 1974 proton-flare region. II

  • 1. Ceskoslovenska Akademie Ved, Ondrejov. Astronomicky Ustav

Description

Studies of changes with time of the background magnetic field areas not only confirm the results obtained in the first part of the paper, dealing with the investigation of the morphological development of the large-scale June-July 1974 proton-flare region related magnetic patterns, but also demonstrate the physical unity of this whole complex evolutionary process and its relation to the cyclic magnetic field generation in the Sun. The fast disintegration of the whole large-scale magnetic field figure and a complete disappearance of its sunspot, flare and green-corona activity follows during three-four rotations after the proton-flare events. For the explanation of this, the mechanisms have to be looked for which either transport magnetic field lines into the upper layers of the solar atmosphere and the interplanetary space, or which dissipate them without observable solar activity. (author)

Part of:
June-July 1974 proton-flare region. I

Additional details

Additional titles

Subtitle (English)
Regularities in the magnetic field area and related sunspot and flare-activity development

Publishing Information

Journal Title
Bull. Astron. Inst. Czech.
Journal Volume
33
Journal Issue
3
Series
Bull. Astron. Inst. Czech.
Journal Page Range
160-173
ISSN
0004-6248

Optional Information

Notes
For Part I see Bull. Astron. Inst. Czech. (1981) v. 32(6) p. 349-359.