Published July 1982
| Version v1
Journal article
Do magnetic transients exist in solar flares
Description
Analysis of a spectrum of the 1981 July 26 solar flare indicates that the ''magnetic transients'' recently detected with a videomagnetograph at the Big Bear Solar Observatory more likely represent brightness effects than magnetic phenomena. Direct measurements of the Zeeman splitting in the lambdalambda 5233, 5324, 5447, 5587 Fe I lines show that in this flare the field strength reached 3000 gauss
Additional details
Publishing Information
- Journal Title
- Sov. Astron. Lett. (Engl. Transl.)
- Journal Volume
- 8
- Journal Issue
- 4
- Series
- Sov. Astron. Lett. (Engl. Transl.).
- Journal Page Range
- 270-272
- ISSN
- 0360-0327
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 15015759
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- EMISSION SPECTRA; SOLAR FLARES; SPECTRAL SHIFT; TRANSIENTS; ZEEMAN EFFECT
- Descriptors DEC
- SOLAR ACTIVITY; SPECTRA
Optional Information
- Notes
- Cover-to-cover translation of Pis'ma v Astronomicheskij Zhurnal (USSR).