Differences in the temporal variations of solar UV flux, 10.7‐cm solar radio flux, sunspot number, and Ca‐K plage data caused by solar rotation and active region evolution
- 1 December 1983
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 88 (A12) , 9883-9888
- https://doi.org/10.1029/ja088ia12p09883
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Solar irradiance variations: 1. Analysis of modeling techniques and intercomparison of ground-based dataJournal of Geophysical Research, 1983
- A three‐component model of the variability of the solar ultraviolet flux: 145–200 nMJournal of Geophysical Research, 1982
- Active‐region evolution and solar rotation variations in solar UV irradiance, total solar irradiance, and soft X raysJournal of Geophysical Research, 1982
- High Spatial Resolution Solar Microwave ObservationsAnnual Review of Astronomy and Astrophysics, 1982
- Solar spectral irradiance, 120 to 190nm, October 13, 1981 ‐ January 3, 1982Geophysical Research Letters, 1982
- The response of ozone to solar activity variations: A reviewSolar Physics, 1981
- Variability of the solar flux in the far ultraviolet 1175–2100 ÅJournal of Geophysical Research, 1980
- The Solar Backscatter Ultraviolet and Total Ozone Mapping Spectrometer (SBUV/TOMS) for NIMBUS GOptical Engineering, 1975
- Space observations of the variability of solar irradiance in the near and far ultravioletJournal of Geophysical Research, 1973
- The quiet and slowly varying components of 9.1 cm radio emission during the solar minimumSolar Physics, 1969