June-July 1974 proton-flare region. II
Creators
- 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)
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
INIS
- Country of Publication
- Czech Republic
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 14777744
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Is Lead record
- Yes
- Descriptors DEI
- ENERGETIC SOLAR PARTICLES; MAGNETIC FIELDS; PHOTOSPHERE; PROTONS; SOLAR ACTIVITY; SOLAR CORONA; SOLAR CYCLE; SOLAR FLARES; SUN; SUNSPOTS; TIME DEPENDENCE
- Descriptors DEC
- ATMOSPHERES; BARYONS; CATIONS; CHARGED PARTICLES; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONS; MAIN SEQUENCE STARS; NUCLEONS; RADIATIONS; SOLAR ATMOSPHERE; SOLAR RADIATION; STARS; STELLAR RADIATION
Optional Information
- Notes
- For Part I see Bull. Astron. Inst. Czech. (1981) v. 32(6) p. 349-359.