Solar flux model in 30-1300nm wavelength range Virtual Observatory Resource

Authors

1. Killen R.
2. Shemansky D.
3. Mouawad N.

Published by

CDS

Abstract

Solar photon scattering probabilities (g values) have been calculated for discrete transitions in 12 species, in a format designed primarily to allow analysis of spacecraft observations from MESSENGER and BepiColombo at Mercury. The results support observations using the MESSENGER Ultraviolet and Visible Spectrometer spectrograph experiment operating over the spectral range 1150-6000{AA} and the BepiColombo spectrograph in the range 550-3150{AA}. Significant radial velocity dependence is shown for most of the emission lines, a critical factor for interpretation of the observed spectra. The g values have general application for solar system emission sources dominated by scattering of the solar flux.

Keywords

1. the-sun
2. spectroscopy
3. ultraviolet-astronomy
4. solar-system-planets

Bibliographic source Bibcode

2009ApJS..181..351K

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/181/351

IVOA Identifier IVOID

ivo://CDS.VizieR/J/ApJS/181/351

Document Object Identifer DOI

doi:10.26093/cds/vizier.21810351

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/181/351
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/181/351
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/181/351

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).