The Sun as an X‐Ray Star. IV. The Contribution of Different Regions of the Corona to Its X‐Ray Spectrum
Open Access
- 10 October 2001
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 560 (1) , 499-513
- https://doi.org/10.1086/322333
Abstract
No abstract availableThis publication has 10 references indexed in Scilit:
- The Sun as an X‐Ray Star. III. FlaresThe Astrophysical Journal, 2001
- On Stellar Coronae and Solar Active RegionsThe Astrophysical Journal, 2000
- The Sun as an X‐Ray Star. II. Using theYohkoh/Soft X‐Ray Telescope–derived Solar Emission Measure versus Temperature to Interpret Stellar X‐Ray ObservationsThe Astrophysical Journal, 2000
- The Sun as an X‐Ray Star. I. Deriving the Emission Measure Distribution versus Temperature of the Whole Solar Corona from theYohkoh/Soft X‐Ray Telescope DataThe Astrophysical Journal, 2000
- The X-Ray View of the Low-Mass Stars in the Solar NeighborhoodThe Astrophysical Journal, 1995
- Temperature structure of active regions deduced from the helium-like sulphur linesSolar Physics, 1995
- The Soft X-ray Telescope for the SOLAR-A missionSolar Physics, 1991
- Einstein Observatory coronal temperatures of late-type starsThe Astrophysical Journal, 1990
- Interstellar photoelectric absorption cross sections, 0.03-10 keVThe Astrophysical Journal, 1983
- Closed coronal structures. III - Comparison of static models with X-ray, EUV, and radio observationsThe Astrophysical Journal, 1981