Published May 1977
| Version v1
Journal article
The fine structure of prominences. III
Description
Faint, Doppler shifted, emission features are detected in high resolution spectra of limb prominences. Their average line-of-sight velocity is about 3 x 106 cms-1, their average life time is 300 s, and their angular sizes are < approximately 108 cm in our spectrograms. The emission line width of the spectral features increases with increasing line shift. Some implications on the stability of prominences by these structures are discussed briefly. (Auth.)
Additional details
Additional titles
- Subtitle (English)
- Small scale Doppler shifted features
Identifiers
- DOI
- 10.1007/bf00149653;
Publishing Information
- Journal Title
- Solar Physics
- Journal Volume
- 52
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 369-377
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8345314
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Is Lead record
- Yes
- Descriptors DEI
- BRIGHTNESS; DOPPLER EFFECT; EMISSION SPECTRA; FINE STRUCTURE; MAGNETIC FIELDS; SOLAR PROMINENCES; SUN; VELOCITY
- Descriptors DEC
- OPTICAL PROPERTIES; PHYSICAL PROPERTIES; SOLAR ACTIVITY; SPECTRA; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent