Published 1988
| Version v1
Book
Rotation of the green corona as derived from CI (1964-1986)
Creators
Description
The rotation and other short-term periodicities of the green corona as derived from the coronal index during cycles 20 and 21 are studied. The rotation rate of the solar corona increased by 4.5 percent in cycle 21. Two equally significant rotation rates were observed more frequently in cycle 21. 24 references
Additional details
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. 400-405.
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
- 20039118
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ANGULAR VELOCITY; ELECTROMAGNETIC RADIATION; FOURIER TRANSFORMATION; MAGNETIC FIELDS; ROTATION; SOLAR ATMOSPHERE; SOLAR CORONA; SOLAR CYCLE
- Descriptors DEC
- ATMOSPHERES; INTEGRAL TRANSFORMATIONS; RADIATIONS; STELLAR ATMOSPHERES; STELLAR CORONAE; TRANSFORMATIONS; VELOCITY