Ozone, water vapour and argon are minor constituents in the Martian atmosphere, observations of which can be of use in constraining atmospheric dynamical and physical processes. This is especially true in the win-ter season of each hemisphere, when the bulk of the main constituent in the atmosphere (CO2) condenses in the polar regions shifting the balance of atmospheric composition to a more trace gas rich air mass. Current Mars Global Circulation Models (MGCMs) [5, 7, 9] are able to represent the photochemistry occuring in the atmosphere, with constraints being imposed by comparisons with observations. However, a long term comparison using data assimilation provides a more robust constraint on the model. We aim to provide a technique for t...
Data assimilation is employed in a novel way for the Mars atmosphere to perform a complete analysis ...
The wealth of atmospheric data from the Mars Global Sur-veyor (MGS) mission affords us an unpreceden...
Isotopic ratios in atmospheric CO2 are shaped by various processes throughout Mars' history, and can...
This work aims to set up a framework for assimilation of trace gas species into a Martian Global Cir...
The aim of this project is to assimilate, for the first time, ozone measurements into a Mars atmosph...
Observations of atmospheric ozone on Mars can be used to develop the representation of trace gas tra...
The wealth of observations now available from multiple spacecraft in orbit around Mars and rovers/la...
Data assimilation, the combination of observations and numerical models which provide physical const...
From the introduction: Given the quantity of data expected from current and forthcoming spacecraft m...
Our understanding of methane on Mars is insufficient to explain the spatial and temporal variabilit...
Dust-bourne heterogeneous reactions have been modelled using the UK Mars Global Circulation Model (M...
A meteorological data assimilation scheme for the martian atmosphere has been implemented and tested...
The Nadir and Occultation for Mars Discovery (NOMAD) and Atmospheric Chemistry Suite (ACS) instrumen...
Several teams have recently reported the detection of methane in the Martian atmosphere [1-3]. Altho...
The Martian atmosphere is composed primarily (>95%) of CO2 and N2 gas, with CO, O2, CH4, and inert g...
Data assimilation is employed in a novel way for the Mars atmosphere to perform a complete analysis ...
The wealth of atmospheric data from the Mars Global Sur-veyor (MGS) mission affords us an unpreceden...
Isotopic ratios in atmospheric CO2 are shaped by various processes throughout Mars' history, and can...
This work aims to set up a framework for assimilation of trace gas species into a Martian Global Cir...
The aim of this project is to assimilate, for the first time, ozone measurements into a Mars atmosph...
Observations of atmospheric ozone on Mars can be used to develop the representation of trace gas tra...
The wealth of observations now available from multiple spacecraft in orbit around Mars and rovers/la...
Data assimilation, the combination of observations and numerical models which provide physical const...
From the introduction: Given the quantity of data expected from current and forthcoming spacecraft m...
Our understanding of methane on Mars is insufficient to explain the spatial and temporal variabilit...
Dust-bourne heterogeneous reactions have been modelled using the UK Mars Global Circulation Model (M...
A meteorological data assimilation scheme for the martian atmosphere has been implemented and tested...
The Nadir and Occultation for Mars Discovery (NOMAD) and Atmospheric Chemistry Suite (ACS) instrumen...
Several teams have recently reported the detection of methane in the Martian atmosphere [1-3]. Altho...
The Martian atmosphere is composed primarily (>95%) of CO2 and N2 gas, with CO, O2, CH4, and inert g...
Data assimilation is employed in a novel way for the Mars atmosphere to perform a complete analysis ...
The wealth of atmospheric data from the Mars Global Sur-veyor (MGS) mission affords us an unpreceden...
Isotopic ratios in atmospheric CO2 are shaped by various processes throughout Mars' history, and can...