This is a Preprint and has not been peer reviewed. This is version 1 of this Preprint.
This is a Preprint and has not been peer reviewed. This is version 1 of this Preprint.
It is shown, using results of direct numerical simulations, laboratory experiments, measurements in the atmospheric boundary layer, in troposphere, in stratosphere, and the satellite infrared radiances data that in many cases the temperature fluctuations in buoyancy driven chaotic and turbulent atmosphere can be well described by the distributed chaos approach based on the Bolgiano-Obukhov phenomenology. A possibility of analogous consideration of the atmospheric dynamics on other planets (Venus, Mars, Jupiter and Saturn) has been briefly discussed using the data obtained with the Phoenix lander and the radio and infrared observations.
https://doi.org/10.31223/X5690C
Oceanography and Atmospheric Sciences and Meteorology, Physical Sciences and Mathematics, Planetary Sciences
atmosphere, temperature, chaos, spectrum, buoyancy
Published: 2021-03-25 17:15
Last Updated: 2021-03-25 17:15
CC BY Attribution 4.0 International
Conflict of interest statement:
None
Data Availability (Reason not available):
The spectral data were taken from the quoted papers.
There are no comments or no comments have been made public for this article.