PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT PUBLICATION_DATE = 2015-03-24 NOTE = "Description of the DOCUMENT directory contents for the EPPS document volume." END_OBJECT = TEXT END The DOCUMENT directory contains documentation that is considered to be either necessary or useful for users to understand the archive data sets. Documents may be included in multiple forms (ASCII, PDF, MS Word, HTML with image file pointers, etc.). Documents in different formats are included in subdirectories that collect together those with the same content. Included are the following documents. DOCINFO.TXT: Identifies and describes the function of each file in the DOCUMENT directory. (This File) EPPS_DDR_SIS.PDF (.DOCX, .TXT, .LBL): The EPPS DDR SIS: "MESSENGER Software Interface Specification for the Derived Data Records of the Energetic Particle and Plasma Spectrometer". The document is provided in multiple formats, the original being the MS Word document which has been saved in the PDF/A archive format, and in plain ASCII text. The PDS label describes all of the document versions. Contains a tutorial whose purpose is to enable the user to construct 2D angular flux maps (AFM) and energy resolved pitch angle (ERPA) distributions from observations by the Fast Imaging Plasma Spectrometer (FIPS) on MESSENGER. These data products are useful for a variety of investigations of the Mercury plasma environment. Studies of the plasma mantle and sodium plasma population have made extensive use of the AFM to investigate plasma isotropy or bulk flow directions (Gershman et al. 2015; DiBraccio et al. 2015). Work done with the magnetic cusp at Mercury utilized both the AFM and the ERPA distribution. With the combination of the directional and pitch angle information, details of the energization and precipitation processes in the cusp could be elucidated (Raines et al. 2014). The tutorial includes a primary document, sample IDL codes and sample data. Contains a turorial whose purpose is to enable the user to interpret the density, temperature, and pressure (NTP) moments from observations by the Fast Imaging Plasma Spectrometer (FIPS) on MESSENGER. These parameters are useful for a variety of investigations of Mercury’s plasma environment. For example, these moments were used to determine the average characteristics of the plasma sheet (Raines et al., 2011; Gershman et al., 2014) and to distinguish the plasma sheet from the magnetotail lobes (Sun et al., 2016). The derived moments were also used to assess the pressure balance across the dayside magnetopause to understand the nature of dayside magnetic reconnection at Mercury (Gershman et al., 2013). he tutorial includes a primary document, sample IDL codes and sample data. The EPPS instrument paper is available online: Andrews, G. B., T. H. Zurbuchen, B. H. Mauk, H. Malcom, L. A. Fisk, G. Gloeckler, G. C. Ho, J. S. Kelley, P. L. Koehn, T. W. LeFevere, S. S. Livi, R. A. Lundgren, and J. M. Raines, The Energetic Particle and Plasma Spectrometer instrument on the MESSENGER spacecraft, Space Science Reviews, 2007, DOI: 10.1007/s11214-007-9272-5. [ANDREWSETAL2007]