Add to ORKGData assimilation is employed in a novel way for the Mars atmosphere to perform a complete analysis of constituent data over periods of several Mars years
We discuss how objective guidance on selecting the most valuable atmospheric measurements on future ...
The aim of this project is to assimilate, for the first time, ozone measurements into a Mars atmosph...
The prominence of thermal tides in the Martian atmosphere has long been recognized, through classica...
Data assimilation, the combination of observations and numerical models which provide physical const...
A meteorological data assimilation system has been developed recently for analyzing measurements of ...
Water ice clouds have been shown to alter the thermal structure of the Martian atmosphere. Here we d...
Abstract not available. From the introduction: 'The Thermal Emission Spectrometer (TES) aboard Mar...
The wealth of observations now available from multiple spacecraft in orbit around Mars and rovers/la...
The technique of data assimilation gives us an opportunity to further our understanding of important...
Observations of atmospheric ozone on Mars can be used to develop the representation of trace gas tra...
In an effort to continuously improve the capabilities of the Martian atmospheric predictions at LMD,...
Mineral dust is a key component in the atmosphere of Mars, and understanding its properties and beha...
From the introduction: Given the quantity of data expected from current and forthcoming spacecraft m...
The aim of this project is to model the Martian water cycle, including radiatively active water ice ...
Our Global Climate Model (GCM) of the Martian atmosphere is the result of twenty years of ongoing co...
We discuss how objective guidance on selecting the most valuable atmospheric measurements on future ...
The aim of this project is to assimilate, for the first time, ozone measurements into a Mars atmosph...
The prominence of thermal tides in the Martian atmosphere has long been recognized, through classica...
Data assimilation, the combination of observations and numerical models which provide physical const...
A meteorological data assimilation system has been developed recently for analyzing measurements of ...
Water ice clouds have been shown to alter the thermal structure of the Martian atmosphere. Here we d...
Abstract not available. From the introduction: 'The Thermal Emission Spectrometer (TES) aboard Mar...
The wealth of observations now available from multiple spacecraft in orbit around Mars and rovers/la...
The technique of data assimilation gives us an opportunity to further our understanding of important...
Observations of atmospheric ozone on Mars can be used to develop the representation of trace gas tra...
In an effort to continuously improve the capabilities of the Martian atmospheric predictions at LMD,...
Mineral dust is a key component in the atmosphere of Mars, and understanding its properties and beha...
From the introduction: Given the quantity of data expected from current and forthcoming spacecraft m...
The aim of this project is to model the Martian water cycle, including radiatively active water ice ...
Our Global Climate Model (GCM) of the Martian atmosphere is the result of twenty years of ongoing co...
We discuss how objective guidance on selecting the most valuable atmospheric measurements on future ...
The aim of this project is to assimilate, for the first time, ozone measurements into a Mars atmosph...
The prominence of thermal tides in the Martian atmosphere has long been recognized, through classica...