spicam.epn_core: Resource Record Summary

Resource Record Summary

Specialized Resource (CatalogResource):
SPICAM

Short name: spicam.epn_core IVOA Identifier: ivo://latmos.ipsl/spicam/q/epn_corePublisher: Laboratoire Atmosphères, Milieux, Observations Spatiales More Info: http://vo.projet.latmos.ipsl.fr/tableinfo/spicam.epn_core VO Compliance: Level 2: This is a VO-compliant resource.	Status: active Registered: 2018 Apr 17 16:28:28Z
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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).

More About this Resource

About the Resource Providers

This section describes who is responsible for this resource

Publisher: Laboratoire Atmosphères, Milieux, Observations Spatiales

Creator: Azria Chloé; Rostaing Alexandre; Zi Yin Contributor: Anni Määttänen ; Francois Forget ; Sebastien Lebonnois

Contact Information:

X Anni Määttänen
Email: anni.maattanen at latmos.ipsl.fr
Address: LATMOS
Tour 45
couloir 45-46
3rd and 4th floors
Boite 102 / 4 Place Jussieu
75005 Paris
FRANCE

Status of This Resource

This section provides some status information: the resource version, availability, and relevant dates.

Version: n/a
Availability: This is an active resource.

Relevant dates for this Resource:

Updated: 2022 May 02 14:08:31Z

This resource was registered on: 2018 Apr 17 16:28:28Z
This resource description was last updated on: 2022 May 02 14:11:03Z

What This Resource is About

This section describes what the resource is, what it contains, and how it might be relevant.

Resource Class: CatalogResource

Resource type keywords: none provided	Subject keywords: mars solar-system-astronomy planetary-science planetary-atmospheres atmospheric-composition planetary-climates stellar-occultation atmospheric-variability carbon-dioxide Associated observatories/telescopes/instruments: facility: European Mars Express instrument: SPICAM
Intended audience or use: General: This resource provides information appropriate for all users. University: This resource provides information appropriate for use in university education. Research: This resource provides information appropriate for supporting scientific research.
More Info: http://vo.projet.latmos.ipsl.fr/tableinfo/spicam.epn_core	Literature Reference: #Määttänen et al. (2013), A complete climatology of the aerosol vertical distribution on Mars from MEx/SPICAM UV solar occultations, Icarus, 223, doi:10.1016/j.icarus.2012.12.001 #Lebonnois et al. (2006), Vertical distribution of ozone on Mars as measured by SPICAM/Mars Express using stellar occultations, J. Geophys. Res., 111, E09S05, doi:10.1029/2005JE002643 #Forget et al. (2009), Density and temperatures of the upper Martian atmosphere measured by stellar occultations with Mars Express SPICAM, J. Geophys. Res., 114, E01004, doi:10.1029/2008JE003086
Related Resources: Other Related Resources LATMOS DaCHS server TAP service(IsServedBy) ivo://latmos.ipsl/tap [Res. ID]

	Data Coverage Information
	This section describes the data's coverage over the sky, frequency, and time. Wavebands covered: Infrared UV

Available Service Interfaces

	Table Access Protocol - Auxiliary ServiceXX
	This is a standard IVOA service that takes as input an ADQL or PQL query and returns tabular data. VO Compliance: Level 2: This is a VO-compliant resource. Available endpoints for the standard interface: http://vo.projet.latmos.ipsl.fr/tapX(version 1.1 compatible)