Modeling the solar irradiance background via numerical simulation

Details Modeling the solar irradiance background via numerical simulation Modeling the solar irradiance background via numerical simulation

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.328...39v&link_type=abstract

Astrophysics and Space Science, Volume 328, Issue 1-2, pp. 39-42

Astronomy and Astrophysics

Astrophysics

Solar Irradiance Background

Scientific paper

Various small scale photospheric processes are responsible for spatial and temporal variations of solar emergent intensity. The contribution to total irradiance fluctuations of such small scale features is the solar irradiance background. Here we examine the statistical properties of irradiance background computed via a n-body numerical scheme mimicking photospheric space-time correlations and calibrated by means of IBIS/DST spectro-polarimetric data. Such computed properties are compared with experimental results derived from the analysis of a VIRGO/SPM data. A future application of the model here presented could be the interpretation of stellar irradiance power spectra observed by new missions such as Kepler.

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