Published May 1977 | Version v1
Journal article

The fine structure of prominences. III

  • 1. Oslo Univ. (Norway). Institutt for Teoretisk Astrofysikk

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.)

Part of:
The fine structure of prominences. II

Additional details

Additional titles

Subtitle (English)
Small scale Doppler shifted features

Identifiers

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
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