The numerical model utilized in this study is
a reconstructed one
from the two-dimensional numerical model developed by
Nakajima (1994)
to calculate convection in the Martian atmosphere.
The Nakajima's original model is designed to calculate
cumulus convection in the terrestrial atmosphere.
The source code of the present model can be seen in
Nakajika and Odaka (2000).
The detailed expressions of model equations
are shown in appendix A,
and their finite differenced forms
are shown in appendix B.
