Published 1985
| Version v1
Book
Anticipated scientific return of the Advanced Solar Observatory
Creators
Description
The scientific importance of the Advanced Solar Observatory (ASO) is discussed with emphasis on its soft X-ray, XUV, and EUV facilities. The principal achievement expected from the ASO's SXR/XUV and EUV telescope is a greatly improved resolution of the magnetic structure and activity in the transition region and corona. Observations from these facilities, combined with complementary observations of the photosphere and chromosphere from Solar Optical Telescope and of the higher corona from the Pinhole/Occulter Facility, are expectecd to yield significant advances in all major areas of solar physics concerning the causes and effects of solar magnetic fields. 24 references
Additional details
Publishing Information
- Publisher
- Advanced Solar Observatory.
- Imprint Place
- Carmel, CA (USA)
- Imprint Title
- Conference on soft x-ray XUV, and EUV observations of the solar atmosphere
- Journal Page Range
- p. 23.
Conference
- Title
- Advanced Solar Observation conference on soft X-ray, XUV, and EUV observations of the solar atmosphere.
- Dates
- 21-24 Jan 1985.
- Place
- Carmel, CA (USA).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 19015359
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- EXTREME ULTRAVIOLET RADIATION; MAGNETIC FIELDS; ORBITING SOLAR OBSERVATORIES; SOFT X RADIATION; SOLAR ATMOSPHERE; SOLAR FLARES; SOLAR WIND; SUN; TELESCOPES
- Descriptors DEC
- ATMOSPHERES; ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; MAIN SEQUENCE STARS; RADIATIONS; SATELLITES; SOLAR ACTIVITY; STARS; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR FLARES; STELLAR WINDS; ULTRAVIOLET RADIATION; X RADIATION