Published 1977
| Version v1
Journal article
Type III radio bursts in a flaming structure
Description
An interpretation is presented of the burst of 3.7.1974. The slowly drifting, fine structure in this type III burst is evidence of the existence of very fast, spatially extensive processes in the corona. The concept is presented of a rapidly varying, magnetohydrodynamically unstable, flaming structure of the magnetic field and, using this model, the intensities were computed of the magnetic field at certain altitudes and at two moments differing by 1.4 s. (author)
Additional details
Publishing Information
- Journal Title
- Bull. Astron. Inst. Czech.
- Journal Volume
- 28
- Journal Issue
- 2
- Series
- Bull. Astron. Inst. Czech.
- Journal Page Range
- 117-119
INIS
- Country of Publication
- Serbia and Montenegro
- Country of Input or Organization
- Serbia and Montenegro
- INIS RN
- 8345348
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ELECTRON BEAMS; FINE STRUCTURE; MAGNETIC FIELDS; MHZ RANGE 100-1000; OPEN CONFIGURATIONS; SOLAR CORONA; SOLAR RADIO BURSTS
- Descriptors DEC
- BEAMS; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; LEPTON BEAMS; MAGNETIC FIELD CONFIGURATIONS; MHZ RANGE; PARTICLE BEAMS; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY