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Start Over Subject mars Content Level University Content Level Research
1. GEM-Mars GCM profiles
ID:
ivo://bira-iasb/gem_mars/q/epn_core
Title:
GEM-Mars GCM profiles
Short Name:
gem_mars.epn_cor
Date:
28 Oct 2023 16:50:48
Publisher:
Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
Description:
Profiles of pressure, temperature and species of the Martian atmosphere simulated with the GEM-Mars general circulation model. See for the main model descritpion Neary, L., et al. 2018. The GEM-Mars general circulation model for Mars: Description and evaluation. Icarus 300, 458-476. https://doi.org/10.1016/j.icarus.2017.09.028. See for the chemistry description Dearden, F. et al., 2019, Mars atmospheric chemistry simulations with the GEM-Mars general circulation model, Icarus, 326, 197-224, https://doi.org/10.1016/j.icarus.2019.02.030.
2. HST observations of planets and satellites
ID:
ivo://padc.obspm.planeto/hst_planeto/q/epn_core
Title:
HST observations of planets and satellites
Short Name:
HST Planeto
Date:
07 May 2024 03:01:53
Publisher:
Paris Astronomical Data Centre - LESIA
Description:
HST observations of planets, dwarf planets, and satellites, extracted from the CADC database catalogue (with daily updates). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period.
3. L3 Omega Cubes - Mars Express
ID:
ivo://idoc/psup/omega_cubes/q/epn_core
Title:
L3 Omega Cubes - Mars Express
Date:
12 Mar 2021 16:07:42
Publisher:
IDOC
Description:
Mars Express - Omega Cubes
4. Mars atmospheric profiles - From NOMAD/TGO
ID:
ivo://bira-iasb/nomad/q/epn_core
Title:
Mars atmospheric profiles - From NOMAD/TGO
Short Name:
nomad.epn_core
Date:
28 Oct 2023 16:48:34
Publisher:
Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
Description:
Profiles of pressure, temperature and species of the Martian atmosphere derived from measurements of the NOMAD instrument on board ESA's Trace Gas Orbiter. See paper https://doi.org/10.1007/s11214-018-0517-2
5. Mars Craters
ID:
ivo://padc.obspm.planeto/mars_craters/q/epn_core
Title:
Mars Craters
Short Name:
mars_craters.epn
Date:
17 Apr 2024 13:17:11
Publisher:
Paris Astronomical Data Centre - Constructor University
Description:
The Mars Crater Catalog by S.J. Robbins was generated from THEMIS Daytime IR and Viking MDIM 2.1 global mosaics of Mars. Craters were selected using 5 points along the rim. The table is statistically complete to the diameter of ~1.0 km. The table contains morphologic and morphometric data for craters with diameter larger than 3 km. The Prometheus basin has been excluded from the Catalog due to technical issues. Reference: "A New Global Database of Mars Impact Craters ≥1 km: (1) Database Creation, Properties, and Parameters", S.J. Robbins and B.M. Hynek, Journal of Geophysical Research - Planets, v.117. (2012) DOI: 10.1029/2011JE003966
6. Mars Craters Lagain
ID:
ivo://padc.obspm.planeto/mars_craters_lagain/q/epn_core
Title:
Mars Craters Lagain
Short Name:
mars_craters_lag
Date:
17 Apr 2024 13:07:37
Publisher:
Paris Astronomical Data Centre - Constructor University
Description:
A catalogue of Mars craters by Lagain et al. (2020), extending the previous catalogue from Robbins and Hynek (2012, DOI:10.1029/2011JE003966). 185 craters were added by Lagain, the object IDs are compatible with the previous work. Reference: "Impact cratering rate consistency test from ages of layered ejecta on Mars", Lagain et al., Planetary and Space Science, v.180. (2020) DOI: 10.1016/j.pss.2019.104755
7. mars_dust
ID:
ivo://lmd.jussieu/mars_dust/q/epn_core
Title:
mars_dust
Date:
19 Apr 2024 00:00:02
Publisher:
Laboratoire Méteorologie Dynamique
Description:
Mars_dust provides a multiannual climatology of Martian airborne dust as measured by various space missions. The retrieved column dust optical depth is mapped for each Martian year and formatted as cubes with time in the 3rd dimension. Two versions are available: irregularly gridded maps, and regular maps produced by kriging. These latter maps are used as column-integrated dust scenarios in the Mars Climate Database (MCD v5). The detailed description of the methodology and dataset can be found in: Montabone et al (2015) Icarus 251, pp. 65-95https://doi.org/10.1016/j.icarus.2014.12.034 ; Montabone et al (2020) JGR-Planets https://doi.org/10.1029/2019JE006111
8. mcd
ID:
ivo://lmd.jussieu/mcd/q/epn_core
Title:
mcd
Date:
28 Jan 2022 00:57:05
Publisher:
Laboratoire Méteorologie Dynamique
Description:
The database contains some outputs of the MCD for all the scenarios available, at different positions of latitude and longitude. These MCD outputs are provided as Votables containing profiles of temperatures, pressures, density and abundances of O2 and O3 for altitudes between 0 and 249.5 km from the surface.
9. MCD
ID:
ivo://lmd.jussieu/mcd/q/collection
Title:
MCD
Date:
26 Aug 2021 09:44:39
Publisher:
Laboratoire Méteorologie Dynamique
Description:
MCD is a database of atmospheric statistics compiled from Global Climate Model (GCM) numerical simulation of Martian atmosphere (<a href=http://www-mars.lmd.jussieu.fr>http://www-mars.lmd.jussieu.fr</a>). The GCM computes in 3D the atmospheric circulation and climate taking into account radiative transfer through the gaseous atmospheres and the dust and ice aerosols, includes a representation of the CO2 ice condensation and sublimation on the ground and in the atmosphere, simulates the water cycle (with modelling of cloud microphysics), the dust multisize particle transport, the atmospheric composition controlled by the photochemistry and the local non-condensible gas enrichment and depletion induced by CO2 condensation and sublimation, and has been extended into the thermosphere and to model ionospheric processes (due to chemistry). The database extends up to exobase (the top of the thermosphere, roughly at 300km in altitude); in addition to statistics on temperature, wind, pressure, radiative fluxes, it provides data such as atmospheric composition (including dust water vapor and ice content) and make use of 'dust and Extreme Ultra Violet (EUV) scenarios' to represent the variation of dust in the atmosphere and solar EUV conditions. User Manual of the service : <a href=http://vo.lmd.jussieu.fr:8080/MCD_VESPA_service_user_manual.pdf>User Manual of the service </a> .
10. Omega mineral maps - Mars Express
ID:
ivo://idoc/psup/omega_maps/q/epn_core
Title:
Omega mineral maps - Mars Express
Date:
12 Mar 2021 16:07:35
Publisher:
IDOC
Description:
Mars Express - Omega Mineral Maps