Galileo Energetic Particle Detector Pre-Jupiter Calibrated Bundle            
                                                                             
Galileo EPD Venus Resampled 5.0 Minute Calibrated Data Collection            
                                                                             
PDS3 DATA_SET_ID               = GO-V-EPD-4-SUMM-5.0MIN-V1.0                 
PDS3 DATA_SET_NAME             = GO VEN EPD RESAMPLED SUMMARY 5.0 MIN v1.0   
START_TIME                     = 1990-041T03:10:10                           
STOP_TIME                      = 1990-041T08:35:10                           
PDS3 DATA_SET_RELEASE_DATE     = 1993-11-09                                  
PRODUCER_FULL_NAME             = Christopher R. Brull                        
                                                                             
References:                                                                  
GO-V-PPR-3-RDR-VENUS-V1.0, NASA Planetary Data System.                       
                                                                             
These data were originally archived in the following PDS3 data set:          
GO-V-EPD-4-SUMM-5.0MIN-V1.0 (https://doi.org/10.17189/1519697).              
                                                                             
Collection Overview                                                          
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This collection contains 5 minute averages for the energetic                 
particle detector rate data obtained from the LEMMS telescope during         
the time the detector was operated during the Venus encounter.  The          
data are recorded in 5 minute averages for each of 17 LEMMS                  
channels.  (The CMS telescope was not powered up during the Venus            
encounter.)  All of the data was taken with the telescope                    
perpendicular to the spacecraft spin axis (motor step position = 4).         
The rates reported are in units of counts/sec.  Each entry is averaged       
over a 5 minute time span to reduce the amount of data more condusive        
for browsing.                                                                
                                                                             
NOTE                                                                         
==================                                                           
Data in this collection includes only that data which has                    
valid data flag markers as a result of processing done by the Galileo        
Energetic Particles Detector Archive Processor.  A gap in the data exists    
from ~06:38 to ~07:38.                                                       
                                                                             
Depending on the tools used for EPD data analysis, it is possible to         
encounter the pitch angle of the detector being substituted for the pitch    
angle of the charged particles. For example, in Figure 4 of Williams et al.  
(1998), J. Geophys. Res., 103, 17,523-17,534, the authors show a loss at 0   
deg PA, which if viewed carefully must be at 180 deg PA. It is therefore     
useful to exercise caution with pitch angles in the EPD data, depending on   
how the data are obtained.