This is a Preprint and has not been peer reviewed. This is version 2 of this Preprint.
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Abstract
It is shown, using results of numerical simulations, atmospheric experiments and observations with natural trace-gases (ozone, carbon dioxide etc.), that the spatio-temporal distributed chaos can provide good quantitative description of the statistical properties of the passive scalar tracers in the atmosphere from the atmospheric surface layer up to the stratosphere. Related properties of the solar radiation transmittance in the atmosphere have been also briefly discussed as well as analogous properties of the tracers in Jupiter's atmosphere.
DOI
https://doi.org/10.31223/X5KW45
Subjects
Physical Sciences and Mathematics
Keywords
atmosphere, chaos, tracers, transmittance
Dates
Published: 2021-05-13 05:34
Last Updated: 2021-07-05 11:42
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License
CC BY Attribution 4.0 International
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Conflict of interest statement:
None
Data Availability (Reason not available):
The spectral data were taken from the quoted papers
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