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Mars Express Data Holdings

 Brief

Mission To Mars

MEXASP_1100 Order Volume 
Data from the Electron Spectrometer (ELS) instrument of the Analyzer          
of Space Plasmas and Energetic Atoms experiment, 3rd edition (ASPERA-3),      
aboard the Mars Express spacecraft.  The ASPERA-3 Principal Investigator      
is Dr. Rickard Lundin, Swedish Institute of Space Physics (IRF), Kiruna,      
Sweden.  The primary source for ASPERA-3 data is the ESA Planetary            
Science Archive (PSA).
MEXASP_1100_EXT1 Order Volume 
Data from the Electron Spectrometer (ELS) instrument of the Analyzer  
of Space Plasmas and Energetic Atoms experiment, 3rd edition (ASPERA- 
3), aboard the Mars Express spacecraft.  The ASPERA-3 Principal       
Investigator is Dr. Rickard Lundin, Swedish Institute of Space        
Physics (IRF), Kiruna, Sweden.  The primary source for ASPERA-3 data  
is the ESA Planetary Science Archive (PSA).
MEXASP_1100_EXT2 Order Volume 
Data from the Electron Spectrometer (ELS) instrument of the Analyzer  
of Space Plasmas and Energetic Atoms experiment, 3rd edition (ASPERA- 
3), aboard the Mars Express spacecraft.  The ASPERA-3 Principal       
Investigator is Dr. Rickard Lundin, Swedish Institute of Space        
Physics (IRF), Kiruna, Sweden.  The primary source for ASPERA-3 data  
is the ESA Planetary Science Archive (PSA).
MEXASP_1200 Order Volume 
Calibrated data from the Electron Spectrometer (ELS) instrument of    
the Analyzer of Space Plasmas and Energetic Atoms experiment, 3rd     
edition (ASPERA-3), aboard the Mars Express spacecraft.  The ASPERA-3 
Principal Investigator is Dr. Rickard Lundin, Swedish Institute of    
Space Physics (IRF), Kiruna, Sweden.  The primary source for ASPERA-3 
data is the ESA Planetary Science Archive (PSA).
MEXASP_3100 Order Volume 
Data from the Neutral Particle Imager (NPI) instrument of the Analyzer        
of Space Plasmas and Energetic Atoms experiment, 3rd edition (ASPERA-3),      
aboard the Mars Express spacecraft.  The ASPERA-3 Principal Investigator      
is Dr. Rickard Lundin, Swedish Institute of Space Physics (IRF), Kiruna,      
Sweden.  The primary source for ASPERA-3 data is the ESA Planetary            
Science Archive (PSA).
MEXASP_3200 Order Volume 
Data from the Neutral Particle Imager (NPI) instrument of the         
Analyzer of Space Plasmas and Energetic Atoms experiment, 3rd edition 
(ASPERA-3), aboard the Mars Express spacecraft.  The ASPERA-3         
Principal Investigator is Dr. Rickard Lundin, Swedish Institute of    
Space Physics (IRF), Kiruna, Sweden.  The primary source for ASPERA-3 
data is the ESA Planetary Science Archive (PSA).
MEXASP_3200_EXT1 Order Volume 
Data from the Neutral Particle Imager (NPI) instrument of the         
Analyzer of Space Plasmas and Energetic Atoms experiment, 3rd edition 
(ASPERA-3), aboard the Mars Express spacecraft.  The ASPERA-3         
Principal Investigator is Dr. Rickard Lundin, Swedish Institute of    
Space Physics (IRF), Kiruna, Sweden.  The primary source for ASPERA-3 
data is the ESA Planetary Science Archive (PSA).
MEXASP_3200_EXT2 Order Volume 
Data from the Neutral Particle Imager (NPI) instrument of the         
Analyzer of Space Plasmas and Energetic Atoms experiment, 3rd edition 
(ASPERA-3), aboard the Mars Express spacecraft.  The ASPERA-3         
Principal Investigator is Dr. Rickard Lundin, Swedish Institute of    
Space Physics (IRF), Kiruna, Sweden.  The primary source for ASPERA-3 
data is the ESA Planetary Science Archive (PSA).
MEXMDE_1001 Order Volume 
All MARSIS Level 1b data, that is, telemetry     
data that have been cleaned, merged, time ordered, and sorted by      
instrument data types and instrument modes.  Data are in              
scientifically useful form, but still uncalibrated.
MEXMDI_1001 Order Volume 
MARSIS data volume containing documentation and all available         
Mars Express Active Ionospheric Sounding (AIS) Science data for       
spacecraft event time (SCET) dates 2004-01-01 (001) up to the most    
recently processed times.
MEXMDS_1001 Order Volume 
All MARSIS Level 2 data, that is,                
subsurface-sounding data that have been uncompressed, calibrated,     
and, except for data acquired using the SS2 mode, range-processed     
after correcting for the distortion of the transmitted signal         
caused by the ionosphere.  Geometric information needed to            
locate observations in space and time is also provided in the         
data set.

Generated: Tue Nov 24 04:39:31 2009

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