Spatial distribution of XUV emission and density in a loop prominence
- 1 March 1980
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 65 (2) , 347-356
- https://doi.org/10.1007/bf00152798
Abstract
No abstract availableKeywords
This publication has 13 references indexed in Scilit:
- The high-temperature corona associated with a loop prominence systemThe Astrophysical Journal, 1979
- Physical parameters in long-decay coronal enhancementsSolar Physics, 1979
- Electron densities in the solar corona from density-sensitive line ratios in the N I isoelectronic sequenceThe Astrophysical Journal, 1978
- Extreme ultraviolet spectroheliograph ATM experiment S082AApplied Optics, 1977
- Electron impact excitation coefficients for laboratory and astrophysical plasmasJournal of Quantitative Spectroscopy and Radiative Transfer, 1976
- The pressure and energy balance of the cool corona over sunspotsThe Astrophysical Journal, 1976
- The temperature structure and pressure balance of magnetic loops in active regionsSolar Physics, 1975
- The loop prominence of 11 August 1972: A coronal continuum eventSolar Physics, 1974
- On the distribution of material as a function of temperature in the post-flare loop system of 12 August 1970Solar Physics, 1971
- The Ionization Equilibrium of Elements Between Carbon and NickelMonthly Notices of the Royal Astronomical Society, 1969