Galileo Energetic Particle Detector Pre-Jupiter Calibrated Bundle - Errata      
                                                                                
This document describes known errors or deficiencies in the                     
Galileo Energetic Particle Detector Pre-Jupiter Raw Bundle.                     
                                                                                
This bundle was produced for the Planetary Data System (PDS) at the             
Planetary Plasma Interactions (PPI) node.                                       
                                                                                
For questions or problems regarding this bundle, please contact the PDS/PPI     
operator:                                                                       
                                                                                
    Email               pds_operator@igpp.ucla.edu                              
                                                                                
These data were originally archived in the following PDS3 data sets:            
GO-E-EPD-4-SUMM-EARTH1-15MIN-V1.0 (https://doi.org/10.17189/1519639),           
GO-E-EPD-4-SUMM-EARTH2-15MIN-V1.0 (https://doi.org/10.17189/1519640),           
GO-V-EPD-4-SUMM-5.0MIN-V1.0 (https://doi.org/10.17189/1519697),                 
GO-E-EPD-2-SAMP-EARTH1-PAD-V1.0 (https://doi.org/10.17189/1519637),             
GO-E-EPD-2-SAMP-EARTH2-PAD-V1.0 (https://doi.org/10.17189/1519638),             
GO-V-EPD-2-SAMP-PAD-V1.0 (https://doi.org/10.17189/1519696).                    
                                                                                
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.                                                                   
                                                                                
These data were originally a partial of the remake of the PDS3 volumes          
GO_0021, GO_0026 and GO_0065 for the ESA Special Publication 1230.              
                                                                                
There were no known deficiencies or errors reported in the errata.txt files     
under PDS3.                                                                     
                                                                                
During the migration from PDS3 to PDS4 no issues were found and corrected       
in the PDS4 metadata. The data remain unchanged.