Published January 1989
| Version v1
Journal article
Flare processes in the quiet prominence
Creators
- 1. Moskovskij Gosudarstvennyj Univ., Moscow (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''
- 2. Kievskij Gosudarstvennyj Univ., Kiev (Ukrainian SSR). Astronomicheskaya Observatoriya
Description
A new method is proposed for the determination of the limits of electron concentration variations in plasma along the line of sight from pre-continuum of Balmer series. It is shown that at one and the same prominence thre exist volumes giving a considerable contribution to the prominence emission measure and differing in electron concentration by more than two orders of magnitude (1010<ne ≤2x1012 cm-3). The characteristic value of ne for the volumes responcible for hydrogen lines emissions is about 5x1010 cm-3. The conclusion has been drawn that at small volumes of a quiet prominence there occurs a powerful (flare-like) energy release manifested in a Balmer pre-continuum
Additional details
Additional titles
- Original title (Russian)
- Вспышечные процессы в спокойном протуберанце
Publishing Information
- Journal Title
- Pis'ma v Astronomicheskij Zhurnal
- Journal Volume
- 15
- Journal Issue
- 1
- Series
- Pis'ma Astron. Zh.
- Journal Page Range
- 82-88
- ISSN
- 0320-0108
- CODEN
- PAZHD
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 20054347
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- BALMER LINES; ELECTRON DENSITY; EMISSION SPECTRA; SOLAR PROMINENCES; SOLAR RADIATION
- Descriptors DEC
- RADIATIONS; SOLAR ACTIVITY; SPECTRA; STELLAR RADIATION