MAVEN SWIA Calibrated Fine Survey 3D Data Collection
Short Name:
SWIA-FINE-SVY
Date:
15 Dec 2022 19:28:31
Publisher:
Planetary Data System
Description:
SWIA fine survey 3d files with time-ordered fully calibrated ion
distributions in units of differential energy flux derived from the
SWIA Fine distribution Survey telemetry, as well as a header of
ancillary information needed to interpret the data.
MAVEN SWIA Calibrated Onboard Survey Moment Data Collection
Short Name:
SWIA-ONB-SVYMOM
Date:
15 Dec 2022 19:27:50
Publisher:
Planetary Data System
Description:
SWIA onboard moment files with time-ordered ion moments converted to
physical units and coordinates, as computed onboard from Coarse and
Fine ion distributions, as well as a header with ancillary information
needed to interpret the moments.
MAVEN SWIA Calibrated Onboard Survey Spectra Data Collection
Short Name:
SWIA-ONB-SVYSPEC
Date:
15 Dec 2022 19:24:25
Publisher:
Planetary Data System
Description:
SWIA onboard spectra files with time-ordered angle-averaged ion
energy spectra in units of differential energy flux, as computed
onboard from Coarse ion distributions, as well as a header with
ancillary information needed to interpret the spectra.
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.
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> .
UCL Magnetodisc Model for Jupiter and Saturn. The data consists of the
magnetic field in JMAG spherical coordinates. For details and further
references, see: Achilleos N. A., Guio, P. and Arridge, C. S., 2010, A model
of force balance in Saturn's magnetodisc, MNRAS, 401, 2349-2371,
<a href="https://doi.org/10.1111/j.1365-2966.2009.15865.x">doi:10.1111/j.1365-2966.2009.15865.x</a>
MESSENGER EPPS EPS Calibrated High Priority Spectra Data Collection
Short Name:
EPS-HI-SPECTRA
Date:
15 Dec 2022 19:28:46
Publisher:
Planetary Data System
Description:
EPS high energy resolution calibrated spectra similar to the
EPS_HIRES_SPECTRA product, but with the configuration from before the
new FSW6 load on 8/18/2008.
MESSENGER EPPS EPS Calibrated Low Resolution Spectra Data Collection
Short Name:
EPS-LORES-SPEC
Date:
15 Dec 2022 19:28:37
Publisher:
Planetary Data System
Description:
EPS low resolution (energy channel) calibrated ion and electron
energy spectra and rate counters. Replaces EPS_MED_SPECTRA after FSW6
(loaded on 8/18/2008).
