Phase relations between total solar irradiance and the Mg II index
- 1 January 2016
- journal article
- Published by Elsevier BV in Advances in Space Research
- Vol. 57 (1), 408-417
- https://doi.org/10.1016/j.asr.2015.10.020
Abstract
No abstract availableFunding Information
- 973 Program
- National Natural Science Foundation of China (11573065, 11273057, 11221063)
- Chinese Academy of Sciences
This publication has 40 references indexed in Scilit:
- Modeling Total Solar Irradiance with San Fernando Observatory Ground-Based Photometry: Comparison with ACRIM, PMOD, and RMIB CompositesSolar Physics, 2013
- Solar irradiance variability: a six-year comparison between SORCE observations and the SATIRE modelAstronomy & Astrophysics, 2011
- Solar EUV Spectrum Calculated for Quiet Sun ConditionsSolar Physics, 2011
- Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year CycleSpace Science Reviews, 2009
- Reconstruction of the solar UV irradiance back to 1974Advances in Space Research, 2005
- Solar Cycle 23: An Anomalous Cycle?The Astrophysical Journal, 2004
- Estimates of solar variability using the solar backscatter ultraviolet (SBUV) 2 Mg II index from the NOAA 9 satellitePublished by American Geophysical Union (AGU) ,1992
- The solar UV Mg II core-to-wing ratio from the NOAA9 satellite during the rise of solar cycle 22Advances in Space Research, 1988
- Variations of Solar Irradiance Due to Magnetic ActivityAnnual Review of Astronomy and Astrophysics, 1987
- The Mg 280‐nm doublet as a monitor of changes in solar ultraviolet irradianceJournal of Geophysical Research: Atmospheres, 1986