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Monte Carlo Calculations of Reflected Intensities for Real Spherical Atmospheres

To calculate the emergent radiation field, a realistic atmospheric model and algorithm must be developed. The radiation field may be characterized by the emergent intensities of scattered light. This is possible only if the algorithm determines these intensities as dependent upon atmospheric and angular parameters.

Identiferoai:union.ndltd.org:unt.edu/info:ark/67531/metadc131064
Date01 1900
CreatorsMontgomery, John A.
ContributorsKattawar, George W., 1937-, Cecil, David R.
PublisherNorth Texas State University
Source SetsUniversity of North Texas
LanguageEnglish
Detected LanguageEnglish
TypeThesis or Dissertation
Formativ, 52 leaves, Text
RightsPublic, Copyright, Copyright is held by the author, unless otherwise noted. All rights reserved., Montgomery, John A.

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