***** File LBLFORM.TXT PDS Label Descriptions The International Halley Watch agreed early on in the project that all data would be submitted from the individual disciplines to the Lead Center using the FITS format. When the decision was made to distribute this information on CD-ROM, it was determined that the data had to have even broader accessibility. For this reason, the original FITS files, with contiguous headers and data, were split into separate files. The original FITS byte stream could then be recovered by concatenating the appropriate header and data files. PDS labels were constructed to allow definition of the data files for the Planetary Data System. For each original data input there must always be a PDS detached label with the extension .LBL. The convention for naming files on the CD-ROM was proposed by the IHW Lead Center to include a unique data qualifier for the data. A specific set of rules was established to identify the net and subnet for each discipline (given by a letter code). A CD-ROM running number relates the information contained in the various indices to the files containing the actual data. A short list of this convention by discipline and subnet (or experiment) is given below: PDS Object FITS Discipline Letter File Ext (description) NAXIS = Code text 1 Astrometry ASTR .lbl fits_label (no data) 0 IR Studies IRIM .lbl table (filter) 0,2 IR " IRFT .lbl table(photometry) 0,2 IR " IRPH .lbl table(polarimetry) 0,2 IR " IRPOL .lbl spectrum 2 IR " IRSP .lbl image 2 IR " IRIM .lbl fits_label (no data) 0 Large Scale Phen LSPN .lbl image(compress) 0,1 Large " LSPN .lbl image(browse) 2 Large " LSPN .lbl image 2 Near Nucleus NNSN .lbl table (broad band) 0,2 Photometry Polar PMAG .lbl table (narrow band) 0,2 " PFLX .lbl table (polarization) 0,2 " PPOL .lbl fits_label (no data) 0 Radio Studies RSCN,SL .lbl spectrum 1 " RSOH .lbl spectrum(multiple) 2 " RSOH .lbl image(multiple) 3 " RSOC .lbl spectrum 1 Spectroscopy SPEC .lbl image 2 " SPEC .lbl fits_label (no data) 0 Amateur AMDR,PG .lbl table (magnitude) 0,2 " AMV .lbl Note that the Subnet coding (explained in the Filenaming Conventions) is one way to distinguish file extension and content. The file extensions follow suggestions by the Planetary Data System (SPIDS v1.1) for tabular and image data. In addition, for IHW FITS, the original headers and data were split into separate files, with filename extensions as listed below. .LBL - detached PDS stream format These PDS labels are metadata (as headers describing data submitted to the archive). There has been no effort to duplicate the documentation contained in the full FITS headers because the PDS and FITS headers for a given data file differ only in the filename extension. Instead we have attempted to use the power of the PDS label syntax to fully describe the data structures and thus gain access to software by that group. Standards for the Preparation and Interchange of Data Sets, Martin, T. Z., et al, Document D-4683, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA document version 1.1 was the primary reference to the Object Description Language (ODL) necessary to create the PDS labels. (We thankfully acknowledge the help of M. Martin, JPL, for assisting the IHW through version 1.1 of the ODL that allows for SPECTRUM.) The basic PDS descriptors such as SFDU_LABEL, RECORD_TYPE, RECORD_BYTES, and FILE_RECORDS are explained in the SPIDS document. The RECORD_TYPE for all data files is FIXED_LENGTH. The PDS labels have been formed as fixed length (78 byte) with an embedded CR and LF.