Article

 

Modeling the solar irradiance background via numerical simulation Public Deposited

https://scholar.colorado.edu/concern/articles/mg74qm73q
Abstract
  • Various small scale photospheric processes are responsible for spatial and temporal variations of solar emer- gent intensity. The contribution to total irradiance fluctua- tions of such small scale features is the solar irradiance back- ground. Here we examine the statistical properties of irradi- ance background computed via a n-body numerical scheme mimicking photospheric space-time correlations and cal- ibrated by means of IBIS/DST spectro-polarimetric data. Such computed properties are compared with experimen- tal 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 ob- served by new missions such as Kepler.
Creator
Date Issued
  • 2010-01-01
Academic Affiliation
Journal Title
Journal Volume
  • 328
File Extent
  • 39-42
Subject
Dernière modification
  • 2019-12-05
Resource Type
Déclaration de droits
DOI
  • DOI 10.1007/s10509-010-0300-7
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