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- ID:
- ivo://cdpp/illu67p
- Title:
- Illumination maps of 67P
- Short Name:
- ILLU67P
- Date:
- 02 Nov 2020 14:04:37
- Publisher:
- Centre de Données de la Physique des Plasmas(CDPP)
- Description:
- Illumination by the Sun of each face of the comet 67P/Churyumov-Gerasimenko based on the shape model CSHP_DV_130_01_LORES_OBJ.OBJ. The service provides the cosine between the normal of each face (in the same order as the faces defined in the shape model) and the Sun direction; both numerical values and images of the illumination are available. Each map is defined for a given position of the Sun in the frame of 67P (67P/C-G_CK). Longitude 0 is at the center of each map. The code is developed by A. Beth, Imperial College London, UK and the service is provided by CDPP (http://cdpp.eu). Acknowlegment: The illumination models have been developed at the Department of Physics at Imperial College London (UK) under the financial support of STFC grant of UK ST/N000692/1 and ESA contract 4000119035/16/ES/JD (Rosetta RPC-PIU). We would also like to warmly thank Bernhard Geiger (ESA) for his support in validating the 2D-illumination maps.
- ID:
- ivo://koa.ipac/KOA
- Title:
- Keck Observatory Archive
- Short Name:
- KOA
- Date:
- 16 Nov 2021 20:00:00
- Publisher:
- Keck Observatory Archive
- Description:
- The archive node for scientific data sets from the Keck Observatory Archive.
- ID:
- ivo://koa.ipac
- Title:
- Keck Observatory Archive
- Short Name:
- KOA
- Date:
- 26 Oct 2021
- Publisher:
- Keck Observatory Archive
- Description:
- The archive node for scientific data sets from the Keck Observatory Archive (KOA).
- ID:
- ivo://cdpp/transplanet
- Title:
- Magnetosphere Ionosphere coupling simulation runs
- Short Name:
- PSWS Transplanet
- Date:
- 02 Nov 2020 14:05:09
- Publisher:
- CDPP
- Description:
- A Transplanet model of magnetosphere-ionosphere coupling at Earth, Mars, and Jupiter
16. 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
- 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
18. 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
19. 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.
20. 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> .
