Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh23b..01p&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SH23B-01
Physics
7524 Magnetic Fields, 7529 Photosphere, 7536 Solar Activity Cycle (2162), 7537 Solar And Stellar Variability, 7538 Solar Irradiance
Scientific paper
After nearly three decades of total solar irradiance monitoring there is still uncertainty about long-term trends, even whether there is a significant solar cycle dependence. The curret proxy data used in irradiance modeling are summarized and their limitations considered. The recent data obtained during solar cycle 23 provides an enlarged database and additional short-term irradiance variations associated with active region developments. New data about large-scale solar features reveal solar cycle variations and dramatic changes during episodes of extreme activity. These observations suggest potential mechanisms for irradiance variation independent of, or in addition to, sunspots and faculae.
McIntosh Patrick
Pap Judit M.
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