The XUV structure of solar active regions
- 1 January 1982
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 75 (1) , 189-203
- https://doi.org/10.1007/bf00153471
Abstract
No abstract availableKeywords
This publication has 14 references indexed in Scilit:
- Physical properties of individual coronal loops in a solar active region observed in the XUVThe Astrophysical Journal, 1980
- The energy balance and pressure in the solar transition zone for network and active region featuresThe Astrophysical Journal, 1979
- Densities in the quiet sun and polar coronal holes from EUV line ratios involving O III /1666.15 A/The Astrophysical Journal, 1978
- Emission-line spectra of two active regions on the solar limb - 1175-1940 AThe Astrophysical Journal Supplement Series, 1978
- Magnetic loops, downflows, and convection in the solar coronaThe Astrophysical Journal, 1978
- Spectral lines observed in solar flares between 171 and 630 angstromsThe Astrophysical Journal, 1978
- Dynamics of the quiescent solar coronaThe Astrophysical Journal, 1978
- The solar spectrum - Wavelengths and identifications from 160 to 770 angstromsThe Astrophysical Journal, 1976
- The temperature structure and pressure balance of magnetic loops in active regionsSolar Physics, 1975
- The fine structure of the solar atmosphere in the far ultravioletSolar Physics, 1974