Mars Atmosphere and Volatile EvolutioN (MAVEN) Solar Wind Ion Analyzer (SWIA) Calibrated PDS Archive Bundle LID = urn:nasa:pds:maven.swia.calibrated Bundle Description ================== Overview -------- The MAVEN SWIA calibrated PDS archive bundle contains fully calibrated SWIA data, including ion velocity distributions, energy spectra, and density, temperature, and velocity moments from onboard calculations. The data files include tables of sensitivity and energy/angle maps are included. Data consist of Coarse and Fine resolution 3d distributions and energy spectra and moments from onboard computations. The Coarse and Fine resolution data come in two forms, termed "Survey" and "Archive" The Survey data nominally represents data with lower resolution (time, angle, and/or energy) but complete temporal coverage. The Archive data nominally represents data with higher resolution (time, angle, and/or energy), but incomplete temporal coverage, selected by ground command to provide better characterization of "interesting" time periods, based on human selection of time intervals using the Survey data. Version History --------------- Bundle Modification Version Date Description ------- ------------ --------------------------------------------------- 1.0 2015-05-29 MAVEN Release 1 (2015-06-05) 1.1 2015-08-11 MAVEN Release 2 (2015-08-17) 1.2 2015-11-16 MAVEN Release 3 (2015-11-16) 1.3 2016-02-11 MAVEN Release 4 (2016-02-15) 1.4 2016-05-16 MAVEN Release 5 (2016-05-16). Consists of an incremental release of SWIA calibrated data. Coverage is 2014-03-19 to 2016-02-14. 1.5 2016-08-15 MAVEN Release 6 (2016-08-15). Consists of an incremental release of SWIA calibrated data. Coverage is 2014-03-19 to 2016-05-14. 1.6 2016-11-15 MAVEN Release 7 (2016-11-15). Consists of an incremental release of SWIA calibrated data. Coverage is 2016-05-15 to 2016-08-14. Data Processing Notes ===================== Data Timing Uncertainty ----------------------- Some of the data files in this bundle may extend beyond the time for which the Spacecraft Clock (SCLK) drift rate was defined based upon the SPICE MAVEN SCLK kernel used to process them. As a result the SCLK drift rate may have been predicted, resulting in small errors in the time (typically less than a few 1/100's seconds). Where this may be the case a note has been included in the individual PDS product labels. Bundle Contents =============== Collections ----------- This bundle includes the following collections: * Coarse Survey 3D - Full 3D ion distributions in units of differential energy flux from SWIA coarse survey data (LID = urn:nasa:pds:maven.swia.calibrated:data.coarse_svy_3d) * Coarse Archive 3D - Full 3d ion distributions in units of differential energy flux from SWIA coarse archive data (LID = urn:nasa:pds:maven.swia.calibrated:data.coarse_arc_3d) * Fine Survey 3D - Full 3d ion distributions in units of differential energy flux from SWIA fine survey data (LID = urn:nasa:pds:maven.swia.calibrated:data.fine_svy_3d) * Fine Archive 3D - Full 3d ion distributions in units of differential energy flux from SWIA fine archive data (LID = urn:nasa:pds:maven.swia.calibrated:data.fine_arc_3d) * Onboard Survey Moments - Ion density, temperature, and velocity moments in physical units and coordinates calculated onboard from SWIA coarse or fine data (depending on mode) (LID = urn:nasa:pds:maven.swia.calibrated:data.onboard_svy_mom) * Onboard Survey Spectra - Ion energy spectra in units of differential energy flux calculated onboard from SWIA coarse data (LID = urn:nasa:pds:maven.swia.calibrated:data.onboard_svy_spec) Data File Naming ---------------- Data files in this bundle are named according to the following convention: mvn_swi_l2__
_v_r.cdf where: = A descriptor used to identify the data file type = 4-digit year of data coverage date = 2-digit month of year of data coverage date
= 2-digit day of month of data coverage date = 2-digit software version = 2-digit data file version under the specified software version Key Documents ============= Halekas, J.S., MAVEN SWIA PDS Archive SIS - This document contains a description of the MAVEN SWIA Calibrated PDS Archive bundle oganization and data product structure and contents. It is located in the document collection for this bundle (LID = urn:nasa:pds:maven.swia.calibrated:document). Contacts ======== This volume was produced for the Planetary Data System (PDS) at the Planetary Plasma Interactions (PPI) node at the University of California, Los Angeles (UCLA). The data files were generated by Dr. Jasper Halekas at the University of Iowa. The data were delivered to the PPI node via the MAVEN Science Data Center (SDC) located at the Laboratory for Atmospheric and Space Physics (LASP) in Boulder, Colorado. The PDS metadata were generated at the PPI node. For questions regarding this archive, please contact Mr. Joseph Mafi at the PDS PPI Node: Email jmafi@igpp.ucla.edu Telephone 310-206-6073 For question regarding the data, please contact Dr. Jasper Halekas: Internet jasper-halekas@uiowa.edu Telephone (319) 335-1929 For questions regarding PDS Standards or other archives available from the PDS, please contact PDS Operator at the PDS Engineering Node (at JPL): Email pds_operator@jpl.nasa.gov Telephone 818-354-4321 The PDS assumes no legal liability for errors on this archive. All users are encouraged to verify the correctness of the data prior to submitting any publications or other work based on these data. Please report errors on this archive to the PPI of the PDS through contact information provided above.