Voyager 1 Plasma Science Experiment (PLS) Jupiter Data Bundle Readme Introduction ============ This document contains information pertaining to the Voyager 1 Plasma Science Experiment (PLS) Jupiter Data Bundle, which contains data recorded during the Voyager 1 Jupiter Encounter and submitted to the Planetary Data System (PDS) by Voyager PLS investigators. This bundle includes derived values of the electron density and moment temperature at Jupiter during the Voyager 1 encounter in the PLS voltage range (10-5950 eV/q), solar wind plasma data upstream of Jupiter before the Voyager 1 encounte with fit and moment parameters, 96 second inbound and outbound magnetosheath L-mode ion data, 96 second averaged outbound M-mode magnetosheath ion data and 96 second averaged ion moment data. While the full Jupiter Encounter Phase has been defined as 1979-01-06 to 1979-04-13, this archive is limited primarily to the period from 1979-02-15 to 1979-03-24 (inclusive). This bundle is organized into several collections, including data-ele-mom-96s, data-ion-inbndwind-96s, data-ion-l-mode-96s, data-ion-m-mode-96s, data-ion-mom-96s and document. PDS4 documentation is all XML. There is an XML label for every product in the archive. Every effort has been made to insure that the data are of the best quality available. However, users are encouraged to verify the correctness of the data prior to submitting any publications or other work based on these data and report any issues to PDS/PPI. This is a PDS4 archive of the following PDS data set: VG1-J-PLS-5-SUMM-ELE-MOM-96.0SEC-V1.1 (https://doi.org/10.17189/1519890) VG1-J-PLS-5-SUMM-ION-INBNDSWIND-96S-V1.0 (https://doi.org/10.17189/1519891) VG1-J-PLS-5-SUMM-ION-L-MODE-96S-V1.0 (https://doi.org/10.17189/1519892) VG1-J-PLS-5-SUMM-ION-M-MODE-96S-V1.0 (https://doi.org/10.17189/1519893) VG1-J-PLS-5-SUMM-ION-MOM-96.0SEC-V1.1 (https://doi.org/10.17189/1519894) These data sets were originally archived under PDS3 in the VG_1501 volume. Under the PDS3 standard all archives were self contained and could in principle be stored in a single file system (disk, CD-ROM, etc.). PDS4 takes advantage of the modern network capabilities that allow archives to be distributed. As a result, some of the documents and meta data previously stored in the PDS3 catalog files are no longer maintained locally, but are maintained in a central repository. Those files are referenced by unique PDS logical identifiers that are included in the document collection inventory. Contacts ======== For questions or problems regarding this bundle, please contact the PDS Planetary Plasma Interactions Node: Email pds_operator@igpp.ucla.edu