PDS logoPlanetary Data System
PDS Information
Find a Node - Use these links to navigate to any of the 8 publicly accessible PDS Nodes.

This bar indicates that you are within the PDS enterprise which includes 6 science discipline nodes and 2 support nodes which are overseen by the Project Management Office at NASA's Goddard Space Flight Center (GSFC). Each node is led by an expert in the subject discipline, supported by an advisory group of other practitioners of that discipline, and subject to selection and approval under a regular NASA Research Announcement.

Menu: Skip within this page

 

MPC @ SBN

MPC Home

MPC Annex

MPC FEEDBACK

The MPC Users' Group (MUG) invites community feedback on any issues, concerns, or questions about the MPC.

SBN FEEDBACK

Please provide feedback on the SBN website.

PDS Support

Vega 1 Raw Dust Impact Mass Analyzer Observations of Comet Halley

Status: ARCHIVED

Abstract: The PUMA data were submitted by IKI in two unique forms, a GROUPS FITS file and undocumented binary file. In one original form, the data in this set were received as 4,027 separate FITS files, one for each spectrum. These files have been reformatted and combined into four tables, one for each of the PUMA instrument operating modes. Within each table, the spectra are in order of original FITS file number. This order is assumed to be chronological, based on time given by the BLISI clock, in sec.

VEGA1-C-PUMA-2-RDR-HALLEY-V1.0 Browse Download (6.6 MB)

Citation to use when referencing this data set: "Dyachkov, A., V., VEGA1 PUMA DUST MASS SPECTROMETER DATA V1.0, VEGA1-C-PUMA-2-RDR-HALLEY-V1.0, NASA Planetary Data System, 1997"

Useful links: