Solar EUV, XUV and soft X-ray telescope facilities
Abstract
Facility class, high resolution instrumentation can enable maximum spatial, spectral and temporal resolutions and provide understanding of the complex physical conditions in the outer solar atmosphere and the mechanisms responsible for these conditions. The scientific rationale for facility class instruments operating in the EUV, XUV, and soft X ray spectral ranges are discussed. Possible configurations for these facilities and priorities for their development are considered.
- Publication:
-
Smithsonian Astrophysical Observatory Report
- Pub Date:
- January 1982
- Bibcode:
- 1982sao..rept.....W
- Keywords:
-
- Extreme Ultraviolet Radiation;
- Solar Radiation;
- Spectroheliographs;
- Ultraviolet Telescopes;
- X Ray Telescopes;
- Chromosphere;
- Drawings;
- Mass Flow;
- Solar Flares;
- Solar Magnetic Field;
- Spatial Resolution;
- Astronomy