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
- Language
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Articles
La vignette | Titre | Date de téléchargement | Visibilité | actes |
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modelingTheSolarIrradianceBackgroundViaNumericalSimulation.pdf | 2019-12-05 | Public | Télécharger |