Published 1985
| Version v1
Journal article
Application of the ejection distribution number to great chromosphere burst diagnostics
Description
A relation between the ejection distribution number of solar radiation amplitude fluctuations and solar activity has been found. For the quiet Sun the distribution of the ejection number in the solar radioemission amplitudes is close to that in the normal random process. Changes in the ejection distribution number of the solar radioemission amplitude fluctuations take place 1.0-1.5 h before the great chromosphere burst and within it at 755 MHz, and after the burst the number of ejections is reduced to that characteristic for the normal random process
Additional details
Additional titles
- Original title (Russian)
- Применение распределения числа выбросов к диагностике больших хромосферных вспышек
Publishing Information
- Journal Title
- Issled. Solntsa Kranykh Zvezd
- Journal Issue
- no.22
- Series
- Issled. Solntsa Kranykh Zvezd.
- CODEN
- ISKZD
INIS
- Country of Publication
- USSR
- Country of Input or Organization
- USSR
- INIS RN
- 18054029
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- AMPLITUDES; BALMER LINES; CHROMOSPHERE; FLUCTUATIONS; MHZ RANGE 100-1000; SOLAR FLARES; SOLAR RADIO BURSTS; STOCHASTIC PROCESSES
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; FREQUENCY RANGE; MHZ RANGE; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR FLARES; VARIATIONS