Modelling meteor layers in the ionospheres of Mars and Venus
Abstract
This presentation will compare MIA-Mars model outputs with observed MaRS electron density profiles. Meteor layer model results will be compared with MaRS meteor layer observations. Additionally MIA-Venus electron density profiles will be compared to VeRa observations as a first step to model meteor layers for the Venusian ionosphere.
- Publication:
-
EPSC-DPS Joint Meeting 2011
- Pub Date:
- October 2011
- Bibcode:
- 2011epsc.conf..743P