Observational evidence of continual heating in X-ray emitting coronal loops
- 1 March 1978
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 57 (1) , 103-110
- https://doi.org/10.1007/bf00152047
Abstract
No abstract availableKeywords
This publication has 6 references indexed in Scilit:
- Physics of an active region loop systemSolar Physics, 1977
- Influence of magnetic field structure on the conduction cooling of flare loopsSolar Physics, 1976
- A Discussion on the physics of the solar atmosphere - The structure and energy balance of solar active regionsPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1976
- The interpretation of simultaneous soft X-ray spectroscopic and imaging observations of an active regionSolar Physics, 1975
- The analysis of XUV emission linesSolar Physics, 1975
- Radiation from a High-Temperature Low-Density Plasma: the X-Ray Spectrum of the Solar CoronaThe Astrophysical Journal, 1971