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Start Over Subject mars Content Level University
1. 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
2. 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
3. PRETHARSIS
ID:
ivo://geops.ipsl/pretharsis/q/epn_core
Title:
PRETHARSIS
Short Name:
pretharsis.epn_c
Date:
01 May 2024 01:20:23
Publisher:
IPSL/GEOPS
Description:
"The growth of the Tharsis volcanic complex on Mars during Noachian/Hesperian era induced a reorientation of the spin axis of the planet (true polar wander). This service gives access to a map of Mars topography before Tharsis formation (Early Noachian) and a map of Mars topography before true polar wander (Late Noachian/Early Esperian), from the model described in Bouley, S., Baratoux, D., Matsuyama, I. et al. Late Tharsis formation and implications for early Mars. Nature 531, 344–347 (2016). https://doi.org/10.1038/nature17171 ."
4. SPICAM
ID:
ivo://latmos.ipsl/spicam/q/epn_core
Title:
SPICAM
Short Name:
spicam.epn_core
Date:
02 May 2022 14:11:03
Publisher:
Laboratoire Atmosphères, Milieux, Observations Spatiales
Description:
The database contains profiles of atmospheric CO2 density and temperature derived thereof, and ozone concentration profiles, all derived from the first year(s) of SPICAM UV stellar occultation observations (Forget et al. 2009, Lebonnois et al. 2006). The database also includes the full dataset of four Martian years of aerosol extinction profiles from SPICAM UV solar occultations (Määttänen et al. 2013).
5. 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
6. 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.
7. 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> .
8. Planetary Images Database
ID:
ivo://padc.obspm.planeto/bdip/q/epn_core
Title:
Planetary Images Database
Short Name:
BDIP
Date:
23 Nov 2022 15:28:18
Publisher:
Paris Astronomical Data Centre
Description:
Planetary Images Database
9. Planetary Images Database
ID:
ivo://padc.obspm.planeto/bdip/q/observatories
Title:
Planetary Images Database
Short Name:
bdip.observatori
Date:
23 Nov 2022 15:28:18
Publisher:
Paris Astronomical Data Centre
Description:
Observatory names
10. 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