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Noctilucent clouds - Simulation studies of their genesis, properties and global influencesA numerical model is presented for testing theories of the physical mechanisms of noctiluminescent clouds. The time-dependent, one-dimensional model describes the formation, evolution, and properties of the clouds as interactive ice crystals, meteoric dust, water vapor, and ionized air. Mesopause temperatures below 140 K are found to be necessary for the formation of the clouds, conditions existing only at high latitudes in the summer. No predominant nucleation particle could be identified for the formation of the clouds, although a time period of up to a day was determined as necessary for materialization, which lasts several days. Several atmospheric and environmental conditions were characterized which enhance the appearance of the noctiluminescent clouds. One conclusion reached is that the numerous launches necessary to build a solar power satellite system would not significantly exacerbate noctiluminescent cloud formation.
Document ID
19830033755
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Turco, R. P.
(R & D Associates Marina del Rey, CA, United States)
Toon, O. B.
(R and D Associates Marina Del Rey, CA, United States)
Whitten, R. C.
(R and D Associates Marina Del Rey, CA, United States)
Keesee, R. G.
(R and D Associates Marina Del Rey, CA, United States)
Hollenbach, D.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 11, 2013
Publication Date
November 1, 1982
Publication Information
Publication: Planetary and Space Science
Volume: 30
Subject Category
Geophysics
Accession Number
83A14973
Funding Number(s)
CONTRACT_GRANT: NAS2-9881
CONTRACT_GRANT: DE-AI01-79ER-10035
Distribution Limits
Public
Copyright
Other

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