Collection Information
IDENTIFIER urn:nasa:pds:maven.euv.derived:occultations::3.1
NAME MAVEN EUV Derived Occultations Data Collection
TYPE Data
DESCRIPTION MAVEN EUV derived. These are the L4 atmospheric number density (in cm-3) and temperature (in K) measured at the tangent point of the MAVEN-Sun line and Mars atmosphere.
MAVEN EUV derived. These are the L4 atmospheric number density (in cm-3) and temperature (in K) measured at the tangent point of the MAVEN-Sun line and Mars atmosphere.
SEARCH/ACCESS DATA MAVEN EUV Derived Occultations Data Collection Online
MAVEN EUV Derived Data Online
   
Citation
DIGITAL OBJECT IDENTIFIER (DOI) 10.17189/we7s-6v50
AUTHORS Thiemann, Edward ; Eparvier, Francis; Jones, Nicholas; Borelli, Rita
EDITORS
PUBLICATION YEAR 2026
DESCRIPTION MAVEN EUV derived. These are the L4 atmospheric number density (in cm-3) and temperature (in K) measured at the tangent point of the MAVEN-Sun line and Mars atmosphere.
   
Context
START DATE TIME 2014-11-17T12:20:21.000Z
STOP DATE TIME 2025-12-02T05:10:34.375Z
LOCAL MEAN SOLAR TIME
LOCAL TRUE SOLAR TIME
SOLAR LONGITUDE
PRIMARY RESULT PURPOSE Science
PRIMARY RESULT PROCESSING LEVEL Derived
PRIMARY RESULT DESCRIPTION
PRIMARY RESULT WAVELENGTH RANGE
PRIMARY RESULT DOMAIN Atmosphere
PRIMARY RESULT DISCIPLINE NAME Atmospheres
INVESTIGATION Mars Atmosphere and Volatile EvolutioN
OBSERVING SYSTEM
OBSERVING SYSTEM COMPONENT Mars Atmosphere and Volatile Evolution (MAVEN)
Extreme Ultraviolet Monitor
TARGET Mars
REFERENCES