A measurement of the quiet network contribution to solar irradiance variation
- 1 March 2001
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 28 (5) , 883-886
- https://doi.org/10.1029/2000gl012072
Abstract
No abstract availableKeywords
This publication has 28 references indexed in Scilit:
- Extension of the F10.7 Index to 1905 using Mt. Wilson Ca K SpectroheliogramsGeophysical Research Letters, 1998
- What Determines the Relative Areas of Spots and Faculae on Sun‐like Stars?The Astrophysical Journal, 1998
- An Active Sun Throughout the Maunder MinimumSolar Physics, 1998
- The Behavior of solar magnetic plages measured from Mt. Wilson observations between 1915–1984Geophysical Research Letters, 1996
- Stellar Luminosity Variations and Global WarmingScience, 1994
- Do changes in the photospheric magnetic network cause the 11 year variation of total solar irradiance?The Astrophysical Journal, 1991
- Length of the Solar Cycle: An Indicator of Solar Activity Closely Associated with ClimateScience, 1991
- Evidence for long-term brightness changes of solar-type starsNature, 1990
- Magnetic modulation of solar luminosity by photospheric activityThe Astrophysical Journal, 1988
- High-resolution telescope and spectrograph observations of the quiet solar chromosphere and transition zoneThe Astrophysical Journal, 1984