Published 1988
| Version v1
Book
Two eruptive prominences and a CME on February 9, 1982
Description
Two H-alpha eruptive prominences located at N10W90 and S14W90, respectively, were observed simultaneously on February 9, 1982. A CME corresponding to the northern one was observed by satellite. No CME was seen for the much larger southern prominence which was associated with an intense radio burst. A comparison of the two eruptive prominences shows that the shape of an eruptive prominence and its change with time could be an important factor in its association with a CME. 9 references
Additional details
Additional titles
- Augmented title (English)
- Coronal Mass Ejection
Publishing Information
- Publisher
- National Solar Observatory.
- Imprint Place
- Sunspot, NM (USA)
- Imprint Title
- Solar and stellar coronal structure and dynamics; Proceedings of the Ninth Sacramento Peak Summer Symposium, Sunspot, NM, Aug. 17-21, 1987
- Journal Page Range
- p. 547-556.
Conference
- Title
- solar and stellar coronal structure and dynamics.
- Acronym
- 9. Sacramento peak summer symposium
- Dates
- 17-21 Aug 1987.
- Place
- Sunspot, NM (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 20039127
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- MAGNETIC FIELD CONFIGURATIONS; MASS TRANSFER; MORPHOLOGICAL CHANGES; SOLAR CORONA; SOLAR PROMINENCES; SOLAR RADIO BURSTS; TIME DEPENDENCE
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; RADIATIONS; RADIOWAVE RADIATION; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE