Published April 1986
| Version v1
Journal article
On the origin of solar s-type radio burst trains
Description
An interpretation of a millisecond structure of meter wavelength solar radio bursts is suggested to be similar to the interpretation of the Iobian's-bursts. The source is supposed to be a weekly anisotrpic plasma with quasi-homogeneous magnetic field where upper-hybrid plasma waves are excited by hot electrons and converted into ordinary and extraordinary waves with refractive index n0,sub(e)<<1 due to scattering by thermal ions. The negative frequency drift is caused by the group delay of electromagnetic waves from the point n0,sub(e)0 till they escape from the source. Quasi-periodic trains of s-bursts arise from the pulsed conversion of plasma waves into ordinary and extraordinary waves
Additional details
Additional titles
- Original title (Russian)
- О происхождении последовательностей с-всплесков в солнечном радиоизлучении
Publishing Information
- Journal Title
- Pis'ma Astron. Zh.
- Journal Volume
- 12
- Journal Issue
- 4
- Series
- Pis'ma Astron. Zh.
- Journal Page Range
- 311-317
- ISSN
- 0320-0108
- CODEN
- PAZHD
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 18003732
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- MHZ RANGE 100-1000; PLASMA; PLASMA WAVES; SHORT WAVE RADIATION; SOLAR ATMOSPHERE; SOLAR RADIO BURSTS; WAVE PROPAGATION
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; MHZ RANGE; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; STELLAR ATMOSPHERES
Optional Information
- Notes
- For English translation see the journal Soviet Astronomy Letters (USA).