Add to ORKGThe amount of dust in the Martian atmosphere is variable in both space and time. The presence of aerosols in the Mars atmosphere complicates quantitative analysis of Martian surface properties. We have developed a model for Mars surface and atmospheric scattering based on equations in Hillier et al (1991). This formulation was chosen for its speed of computation and because it accounts for the spherical geometry of atmospheric scattering at high mission angles, i.e., near the planetary limb
It is widely believed that the Martian polar layered deposits record climate variations over at leas...
The martian climate has long been thought to have evolved substantially through history from a warm ...
The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state...
We have completed preliminary calculations of the minimum sizes of bolides that would penetrate vari...
Results are presented of one-dimensional radiation convection modeling of the early Mars atmosphere....
The presence of a permanent CO2 polar ice cap on Mars has important consequences for the planet's cl...
We have found that a rather simple thermal model of the Martian surface, in combination with current...
We have found that a rather simple thermal model of the Martian surface, in combination with current...
Our MSATT work has focused on the evolution of CO2 on Mars. We have constructed a model that predict...
At high obliquity, Martian polar ground temperatures could exceed the melting point of ice for consi...
Recent studies have shed light on mesoscale phenomena in the Martian atmosphere, unresolved by globa...
Mars is a small planet with a thin atmosphere of almost pure carbon dioxide. To first order, the Mar...
The long-term variations in the atmospheric pressure and the polar cap temperature of Mars resulting...
The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state...
The long-term variations in the atmospheric pressure and the polar cap temperature of Mars resulting...
It is widely believed that the Martian polar layered deposits record climate variations over at leas...
The martian climate has long been thought to have evolved substantially through history from a warm ...
The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state...
We have completed preliminary calculations of the minimum sizes of bolides that would penetrate vari...
Results are presented of one-dimensional radiation convection modeling of the early Mars atmosphere....
The presence of a permanent CO2 polar ice cap on Mars has important consequences for the planet's cl...
We have found that a rather simple thermal model of the Martian surface, in combination with current...
We have found that a rather simple thermal model of the Martian surface, in combination with current...
Our MSATT work has focused on the evolution of CO2 on Mars. We have constructed a model that predict...
At high obliquity, Martian polar ground temperatures could exceed the melting point of ice for consi...
Recent studies have shed light on mesoscale phenomena in the Martian atmosphere, unresolved by globa...
Mars is a small planet with a thin atmosphere of almost pure carbon dioxide. To first order, the Mar...
The long-term variations in the atmospheric pressure and the polar cap temperature of Mars resulting...
The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state...
The long-term variations in the atmospheric pressure and the polar cap temperature of Mars resulting...
It is widely believed that the Martian polar layered deposits record climate variations over at leas...
The martian climate has long been thought to have evolved substantially through history from a warm ...
The climate of Mars likely evolved from a warmer, wetter early state to the cold, arid current state...