๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Polarization Models for Rayleigh Scattering Planetary Atmospheres

โœ Scribed by Esther Buenzli; Hans M. Schmid; Franco Joos


Book ID
106472313
Publisher
Springer Netherlands
Year
2009
Tongue
English
Weight
273 KB
Volume
105
Category
Article
ISSN
1573-0794

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Rayleigh scattering in planetary atmosph
โœ Viik Tรตnu ๐Ÿ“‚ Article ๐Ÿ“… 1989 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 791 KB

The vector equation of radiative transfer is solved both for conservative and non-conservative planetary atmospheres using the method of discrete ordinates. The atmosphere, bounded by a Lambert bottom, is considered plane-parallel: and homogeneous. The scattering in the atmosphere obeys the Rayleigh

Flux and polarization reflected from a n
โœ Tรตnu Viik ๐Ÿ“‚ Article ๐Ÿ“… 1990 ๐Ÿ› Springer Netherlands ๐ŸŒ English โš– 375 KB

Assuming that the Rayleigh-scattering atmosphere of a planet is homogeneous and planeparallel we estimate the influence of non-conservativeness of the atmosphere and the state of polarization of the incident radiation upon the phase curves both for flux and polarization.