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Reconstructed and measured total solar irradiance: Is there a secular trend between 1978 and 2003?

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Author(s)
T. Wenzler
S. K. Solanki
N. A. Krivova
Contributor(s)
The Pennsylvania State University CiteSeerX Archives

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URI
http://hdl.handle.net/20.500.12424/1018333
Online Access
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.246.7309
http://arxiv.org/pdf/0909.2975v1.pdf
Abstract
Total solar irradiance reconstructed between 1978 and 2003 using solar surface magnetic field distributions is compared with three composites of total solar irradiance measurements. A good correspondence is found with the total solar irradiance composite from PMOD/WRC, with no bias between the three cycles. The agreement with the other composites (the ACRIM composite, mainly based on the Active Cavity Radiometer Irradiance Monitors I, II & III, and the IRMB composite from the Institut Royal Meteorologique Belgique) is significantly poorer. In particular, a secular increase in the irradiance exhibited by these composites is not present in the reconstructions. Hence any secular trend in total solar irradiance between 1978 and 2003 is not due to magnetic fields at the solar surface. 1.
Date
2012-11-22
Type
text
Identifier
oai:CiteSeerX.psu:10.1.1.246.7309
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.246.7309
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Metadata may be used without restrictions as long as the oai identifier remains attached to it.
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