A dataset provided by the European Space Agency

Name MEX-M-SPI-2-UVRDR-CLEANED-EXT2
Mission MARS-EXPRESS
URL ftp://npsa01.esac.esa.int/pub/mirror/MARS-EXPRESS/SPICAM/MEX-M-SPI-2-UVRDR-CLEANED-EXT2-V1.0
DOI https://doi.org/10.5270/esa-w1aut8m
Abstract The Mars Express SPICAM level 1A UV dataset contains measurements from the ultra violet SPICAM spectrometer collected during MARS phase with some corrections and processing
Description SPICAM MARS CLEANED UV RDR Data Set Overview The SPICAM MARS CLEANED UV RDR (level 1A) dataset provides data corrected from the dark charge and the electronic noise. It is also cleaned from erroneous data, cosmic rays damage and saturation. Data are stored in the /DATA directory, divided into mission phases subdirectories (MARS/MOCP or MARS/MTP...). An easily viewed version of each record of the SPICAM MARS CLEANED UV RDR data set is shown in [MEXSPI_1001/BROWSE]
Instrument SPICAM
Temporal Coverage 2007-08-27T12:57:49Z/2009-12-13T12:00:00Z
Version V1.0
Mission Description Mission Overview Mars Express was the first flexible mission of the revised long-term ESA Science Programme Horizons 2000 and was launched to the planet Mars from Baikonur (Kazakhstan) on June 2nd 2003. A Soyuz-Fregat launcher injected the Mars Express total mass of about 1200 kg into Mars transfer orbit. Details about the mission launch sequence and profile can be obtained from the Mission Plan (MEX-MMT-RP-0221) and from the Consolidated Report on Mission Analysis (CREMA)(MEX-ESC-RP- 5500). The mission consisted of (i) a 3-axis stabilized orbiter with a fixed high-gain antenna and body-mounted instruments, and (ii) a lander named BEAGLE-2, and was dedicated to the orbital and in-situ study of the interior, subsurface, surface and atmosphere of the planet. After ejection of a small lander on 18 December 2003 and Mars orbit insertion (MOI) on 25 December 2003, the orbiter experiments began the acquisition of scientific data from Mars and its environment in a polar elliptical orbit. The nominal mission lifetime for the orbiter was 687 days following Mars orbit insertion, starting after a 5 months cruise. The nominal science phase was extended (tbc) for another Martian year in order to complement earlier observations and allow data relay communications for various potential Mars landers up to 2008, provided that the spacecraft resources permit it. The Mars Express spacecraft represented the core of the mission, being scientifically justified on its own by investigations such as high- resolution imaging and mineralogical mapping of the surface, radar sounding of the subsurface structure down to the permafrost, precise determination of the atmospheric circulation and composition, and study of the interaction of the atmosphere with the interplanetary medium. The broad scientific objectives of the orbiter payload are briefly listed thereafter and are given more extensively in the experiment publications con...
Creator Contact FRANCK MONTMESSIN
Date Published 2014-05-25
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2014-05-25, MEX-M-SPI-2-UVRDR-CLEANED-EXT2, V1.0. https://doi.org/10.5270/esa-w1aut8m