This dataset is used for figures in the paper "Seasonal and dust related variations of the dayside thermospheric and ionospheric compositions of Mars observed by MAVEN/NGIMS." The dataset contains neutral and ion number densities measured by MAVEN/NGIMS and estimated ion number densities under the photochemical equilibrium (PCE). The electron temperature measured by MAVEN/LPW and the photoionization rates estimated by the EUVAC solar flux model (Richards et al., 1994), which are used for estimation of ion number densities under the PCE, are included in the dataset. Detailed information can be found in the readme files in each directory
We investigate the production and loss rates of in the photochemical equilibrium region of the Mart...
We compare here models of the thermosphere/ionosphere of Mars at low and high solar activities, and ...
These data were obtained from the magnetometer (MAG), Neutral Gas and Ion Mass Spectrometer (NGIMS),...
The following data set contains valid photoionization frequencies and electron impact ionization fre...
[1] We use a simple photochemical model of Mars ’ ionosphere to investigate the changes in calculate...
Datasets used in the analysis of Mars Atmosphere and Volatile EvoutioN (MAVEN)'s observations of H– ...
International audienceModel studies of the ionosphere of Mars under daytime conditions reveal that f...
International audiencePrior to the arrival of the Mars Atmosphere and Volatile EvolutioN (MAVEN) spa...
We report the results of the observations of the ionosphere of Mars by the Neutral Gas and Ion Mass ...
International audienceWe report seasonal and dust-related variations in neutral and ion species (CO2...
The thermosphere of Mars begins at the homopause (115-130 km) and reaches the exobase (200 km), whic...
These data were primarily obtained from the Neutral Gas and Ion Mass Spectrometer (NGIMS), Solar Win...
International audienceWe present comparisons of planetary pickup ions at Mars with MAVEN (Mars Atmos...
We investigate the production and loss rates of in the photochemical equilibrium region of the Mart...
We compare here models of the thermosphere/ionosphere of Mars at low and high solar activities, and ...
These data were obtained from the magnetometer (MAG), Neutral Gas and Ion Mass Spectrometer (NGIMS),...
The following data set contains valid photoionization frequencies and electron impact ionization fre...
[1] We use a simple photochemical model of Mars ’ ionosphere to investigate the changes in calculate...
Datasets used in the analysis of Mars Atmosphere and Volatile EvoutioN (MAVEN)'s observations of H– ...
International audienceModel studies of the ionosphere of Mars under daytime conditions reveal that f...
International audiencePrior to the arrival of the Mars Atmosphere and Volatile EvolutioN (MAVEN) spa...
We report the results of the observations of the ionosphere of Mars by the Neutral Gas and Ion Mass ...
International audienceWe report seasonal and dust-related variations in neutral and ion species (CO2...
The thermosphere of Mars begins at the homopause (115-130 km) and reaches the exobase (200 km), whic...
These data were primarily obtained from the Neutral Gas and Ion Mass Spectrometer (NGIMS), Solar Win...
International audienceWe present comparisons of planetary pickup ions at Mars with MAVEN (Mars Atmos...
We investigate the production and loss rates of in the photochemical equilibrium region of the Mart...
We compare here models of the thermosphere/ionosphere of Mars at low and high solar activities, and ...
These data were obtained from the magnetometer (MAG), Neutral Gas and Ion Mass Spectrometer (NGIMS),...