A Boundary-Layer Model for Mars: Comparison with Viking Lander and Entry Data
- 1 June 1993
- journal article
- Published by American Meteorological Society in Journal of the Atmospheric Sciences
- Vol. 50 (11) , 1544-1559
- https://doi.org/10.1175/1520-0469(1993)050<1544:ablmfm>2.0.co;2
Abstract
A one-dimensional boundary-layer model for Mars is described, and its results are compared with Viking data. The model equations are similar to Earth boundary-layer models in that they include contributions from Coriolis, pressure gradient, and frictional forces for momentum; and radiation, sensible heat flux convergence, and advection for heat. Turbulent fluxes are computed from the level-2 second-order closure theory of Mellor and Yamada with similarity relations employed for boundary conditions. The pressure gradient force can be specified or computed from a simple slope model. Radiative heating is due to the absorption of solar and infrared radiation by CO2 gas and suspended dust particles. Ground temperatures are computed by solving a surface heat budget using an accurate treatment of conduction into the Martian soil. The data used for comparison were obtained by the Viking 1 and 2 landers for early northern summer. At each site, these data include a single profile of wind and temperature be... Abstract A one-dimensional boundary-layer model for Mars is described, and its results are compared with Viking data. The model equations are similar to Earth boundary-layer models in that they include contributions from Coriolis, pressure gradient, and frictional forces for momentum; and radiation, sensible heat flux convergence, and advection for heat. Turbulent fluxes are computed from the level-2 second-order closure theory of Mellor and Yamada with similarity relations employed for boundary conditions. The pressure gradient force can be specified or computed from a simple slope model. Radiative heating is due to the absorption of solar and infrared radiation by CO2 gas and suspended dust particles. Ground temperatures are computed by solving a surface heat budget using an accurate treatment of conduction into the Martian soil. The data used for comparison were obtained by the Viking 1 and 2 landers for early northern summer. At each site, these data include a single profile of wind and temperature be...Keywords
This publication has 0 references indexed in Scilit: