The Mg 280‐nm doublet as a monitor of changes in solar ultraviolet irradiance
- 20 July 1986
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 91 (D8) , 8672-8682
- https://doi.org/10.1029/jd091id08p08672
Abstract
No abstract availableKeywords
This publication has 28 references indexed in Scilit:
- The sun as a star - Three-component analysis of chromospheric variability in the calcium K lineThe Astrophysical Journal, 1984
- 18 months of UV irradiance observations from the Solar Mesosphere ExplorerGeophysical Research Letters, 1984
- Interpretation of solar irradiance variations using ground-based observationsThe Astrophysical Journal, 1983
- Solar spectral irradiance, 120 to 190nm, October 13, 1981 ‐ January 3, 1982Geophysical Research Letters, 1982
- Solar luminosity variation. IV - The photospheric lines, 1976-1980The Astrophysical Journal, 1982
- Stellar rotation in lower main-sequence stars measured from time variations in H and K emission-line fluxes. I - Initial resultsThe Astrophysical Journal, 1981
- Solar luminosity variation. III - Calcium K variation from solar minimum to maximum in cycle 21The Astrophysical Journal, 1981
- Photospheric models of solar active regions and the network based on the MG II H and K line wingsThe Astrophysical Journal, 1978
- The MG II H and K lines. II - Comparison with synthesized profiles and CA II KThe Astrophysical Journal, 1976
- Resonance-line transfer with partial redistribution. II - The solar MG II linesThe Astrophysical Journal, 1974