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2. Cassini VIMS
- ID:
- ivo://padc.obspm.planeto/vims_satellites/q/epn_core
- Title:
- Cassini VIMS
- Short Name:
- VIMS satellites
- Date:
- 04 Feb 2024 04:04:45
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The Visual and Infrared Mapping Spectrometer (VIMS) instrument onboard the Cassini spacecraft observed the system of Saturn, acquiring spectral cubes in the range 0.4-5.2 microns. This service focuses on Saturn satellites, and provides access to calibrated and ancillary data, computed as described here: https://vims.univ-nantes.fr/info/isis-calibration. It also provides direct links to a larger web site with previews.
- ID:
- ivo://padc.obspm.planeto/planets/q/epn_core
- Title:
- Characteristics of Planets
- Short Name:
- Planets
- Date:
- 16 Oct 2023 16:09:45
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- Main characteristics of Solar System planets. Data are included in the table, which includes non-standard EPN-TAP parameters. Data are retrieved from Archinal et al 2018 (IAU report 2015, 2018CeMDA.130...22A) [radii] and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) [masses, heliocentric distances, and rotation periods].
- ID:
- ivo://padc.obspm.planeto/dynastvo/q/epn_core
- Title:
- DynastVO ephemeris service
- Short Name:
- DynAstVO
- Date:
- 07 May 2024 02:02:48
- Publisher:
- Paris Astronomical Data Centre
- Description:
- This database displays calculated orbital parameters for small bodies
- 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.
- 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.
7. IKS
- ID:
- ivo://padc.obspm.planeto/iks/q/epn_core
- Title:
- IKS
- Short Name:
- IKS
- Date:
- 23 Nov 2022 16:32:49
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- Measurements of comet Halley in the spectral channel of IKS on board the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies Node data set (2011 reformatted version) and updated. The data set consists in 101 tables providing the radiance spectrum of comet Halley from various distances, plus two composite spectra. For details and further references, see: Combes M. et al., 1988, The 2.5-12 micron Spectrum of Comet Halley from the IKS-VEGA Experiment, Icarus, 76, 404-436 [1988Icar...76..404C]
- 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
9. 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
11. 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
12. 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.
13. 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> .
- 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
- 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
16. 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, 344â347 (2016). https://doi.org/10.1038/nature17171 ."
17. SOIR
- ID:
- ivo://bira-iasb/soir/soir_q/epn_core
- Title:
- SOIR
- Short Name:
- soir.epn_core
- Date:
- 28 Oct 2023 16:49:38
- Publisher:
- Planetary Atmospheres Research Unit - Royal Belgian Institute for Space Aeronomy
- Description:
- Profiles of species in Venus atmosphere terminator. Data retrieved from calibrated spectra obtained with the SPICAV-SOIR instrument on board the Venus Express spacecraft. These spectra can be checked on the ESA PSA repository. See: A.C. Vandaele et al., Contribution from SOIR/VEX to the updated Venus International Reference Atmosphere (VIRA), Adv. Space Res. (2015), http://dx.doi.org/10.1016/j.asr:2015.08.012.
18. 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).
- ID:
- ivo://padc.obspm.planeto/basecom/q/epn_core
- Title:
- The Nançay Cometary Database
- Short Name:
- basecom.epn_core
- Date:
- 02 May 2024 18:54:10
- Publisher:
- Paris Astronomical Data Centre
- Description:
- Since 1973, the 18-cm lines of the OH radical have been systematically observed in a number of comets with the Nançay radio telescope. This allowed an evaluation of the cometary water production rates and their evolution with time, as well as a study of several physical processes: the excitation mechanisms of the OH radio lines, the expansion of the cometary atmospheres, their anisotropy in relation with non-gravitational forces, the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of 53 cometary apparitions between 1982 and 2009 are now organized in this database.
20. USGS_WMS
- ID:
- ivo://padc.obspm.planeto/usgs_wms/q/epn_core
- Title:
- USGS_WMS
- Short Name:
- usgs_wms.epn_cor
- Date:
- 17 Apr 2024 13:28:42
- Publisher:
- Paris Astronomical Data Centre - Constructor University
- Description:
- Catalogue of USGS Astrogeology WMS Map Layers
21. vcd
- ID:
- ivo://lmd.jussieu/vcd/q/epn_core
- Title:
- vcd
- Date:
- 19 Apr 2024 00:05:16
- Publisher:
- Laboratoire Méteorologie Dynamique
- Description:
- 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.
- ID:
- ivo://padc.obspm.planeto/vvex/q/epn_core
- Title:
- VIRTIS Venus Express nominal mission (demo)
- Short Name:
- VVEx
- Date:
- 01 Feb 2023 16:44:27
- Publisher:
- Paris Astronomical Data Centre - LESIA
- Description:
- IR spectroscopy of Venus
- ID:
- ivo://padc.obspm.planeto/meteor_showers/q/epn_core
- Title:
- VOEvent meteor shower service
- Short Name:
- Meteor Showers
- Date:
- 08 Mar 2023 13:09:31
- Publisher:
- Paris Astronomical Data Centre
- Description:
- The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravity of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82