Is the ?superhot? hard x-ray component in solar flares consistent with a thermal source?
- 1 January 1989
- journal article
- research article
- Published by Springer Nature in Solar Physics
- Vol. 122 (2) , 313-317
- https://doi.org/10.1007/bf00912998
Abstract
No abstract availableKeywords
This publication has 2 references indexed in Scilit:
- Analytic limits on the forms of spectra possible from optically thin collisional bremsstrahlung source modelsThe Astrophysical Journal, 1988
- A new component of hard X-rays in solar flaresThe Astrophysical Journal, 1981