DaCHS Server for LMD Home

The IPSL laboratories set up, at federal level, common services and major scientific projects to serve its scientificstrategy.

Please check out our site help. Data on this site can also be queried through TAP and an ADQL form.

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DaCHS Server for LMD TAP service
The DaCHS Server for LMD's TAP end point. The Table Access Protocol (TAP) lets you execute queries against our database tables, inspect various metadata, and upload your own data. It is thus the VO's premier way to access public data holdings. Tables exposed through this endpoint include: epn_core from the mars_dust schema, epn_core from the mcd schema, columns, groups, key_columns, keys, schemas, tables from the tap_schema schema, epn_core from the vcd schema.

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mars_dust
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
mcd
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.

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vcd
The database contains some outputs of the VCD for the scenarios : {1) Standard cloud albedo Scenario, solar EUV average conditions ; 2) Standard cloud albedo Scenario, solar EUV minimum conditions ; 3) Standard cloud albedo Scenario, solar EUV maximum conditions ; 4) Low cloud albedo Scenario, solar EUV average conditions ; 5) High cloud albedo Scenario, solar EUV average conditions available}, at different positions of latitude and longitude. These VCD outputs are provided as Votables containing profiles of temperatures, pressures, density and abundances of main species for altitudes between 0 and 349.5 km from the surface.

Atmospheric composition

Atmospheric variability

Carbon dioxide

mcd

Catalogs

DaCHS Server for LMD TAP service

Mars

Planetary atmospheres

Planetary climates

Planetary science

Solar system astronomy

Venus

vcd

Virtual observatories

DaCHS Server for LMD TAP service

Water vapor

mcd