Evaluation of Solar Indices Used in Semi-Empirical Proxy Models

Details Evaluation of Solar Indices Used in Semi-Empirical Proxy Models Evaluation of Solar Indices Used in Semi-Empirical Proxy Models

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsh33c..01p&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SH33C-01

Physics

1650 Solar Variability (7537), 7524 Magnetic Fields, 7529 Photosphere, 7536 Solar Activity Cycle (2162), 7538 Solar Irradiance

Scientific paper

Space observations of total solar and UV irradiances have been conducted for about three decades. These are important for both understanding the physical mechanisms and causal relationships in the sun and also for their terrestrial climatic impacts. However, to establish their true role in climate change, irradiance time series covering a century, or longer time scales, are needed. Accordingly, considerable efforts have been put forward to constract semi-empirical proxy models for climate studies which necessarily depend on long-term solar indices to identify solar changes. In this paper, we compare various solar indices used for irradiance reconstructions and we will devote special attention how well they match the observed irradiance data over the last three solar cycles.

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