Articles | Volume 28, issue 4
https://doi.org/10.5194/npg-28-627-2021
https://doi.org/10.5194/npg-28-627-2021
Brief communication
 | 
03 Nov 2021
Brief communication |  | 03 Nov 2021

Brief communication: Lower-bound estimates for residence time of energy in the atmospheres of Venus, Mars and Titan

Javier Pelegrina, Carlos Osácar, and Amalio Fernández-Pacheco

Viewed

Total article views: 2,059 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
1,606 421 32 2,059 26 17
  • HTML: 1,606
  • PDF: 421
  • XML: 32
  • Total: 2,059
  • BibTeX: 26
  • EndNote: 17
Views and downloads (calculated since 19 Jan 2021)
Cumulative views and downloads (calculated since 19 Jan 2021)

Viewed (geographical distribution)

Total article views: 2,059 (including HTML, PDF, and XML) Thereof 1,918 with geography defined and 141 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 23 Apr 2024
Download
Short summary
The atmospheres of Venus, Mars and Titan are similar to the atmosphere of Earth. We wanted to find out the value of the residence time of energy in these three atmospheres. We estimated the energy contained in a column of air. From experimental data, we deduced the value of the energy inflow and outflow. From these data, the time of residence of the energy is calculated. This parameter gives a timescale of the response of the planetary atmosphere against global perturbations.