PDS_VERSION_ID = PDS3 RECORD_TYPE = STREAM OBJECT = TEXT NOTE = "MSI BROWSE Directory information file" PUBLICATION_DATE = 2001-09-11 END_OBJECT = TEXT END ***** File BROWINFO.TXT This directory (BROWSE/) contains the browse facilities, the MSI Digital Image Map (DIM) Browse Facility for the NEAR Multispectral Imager (MSI) archive. It consists of a directory structure ('BROWSE/BASEMAPS/') with an HTML table file ('MOSAICS.HTM') and the associated files for the browse facility, stored under the subdirectory structure. The HTML and image files are accessible to the contemporary, popular browsers. NOTE ==== The labels and manifest tables ('manifest.tab') written for these files and the approach used in archiving this facility make use of prototype standards which have not yet been formally incorporated into the PDS system. For this reason, support for this facility within the PDS is extremely limited. Once the standards have been fully accepted and integrated into the PDS archives, the labels and files in this directory will be updated by the Small Bodies Node to reflect the final version of the standard. Structure ========= The browse facility consists of two parts: 1. An HTML file containing a table of MSI DIMs, listing some information and links to various related images and other files; and 2. A subdirectory structure containing the referenced files. ===================================== MSI Digital Image Map Browse Facility ===================================== HTML table: BROWSE/BASEMAPS/MOSAICS.HTM NEAR Shoemaker - MSI Digital Image Maps --------------------------------------- Produced by: M. Robinson The NEAR Shoemaker spacecraft returned over 160,000 images of the surface of 433 Eros. A sampling of mosaic products is provided which should give a fair sampling of the mapping possibilities of this dataset. A tremendous strength of the imaging experiment was the repeat coverage for a given area under varying lighting conditions. Several examples of repeat coverage are presented. A global mosaic was created from 100s of images (F4_16_00N000). Due to Eros' unusual orbital inclination it was not possible to cover the asteroid with uniform lighting conditions, thus gross changes in brightness from frame-to-frame are common in the global product. Questions concerning the DIMs should be directed to Mark Robinson, 1847 Sheridan Road, Evanston, IL, 60208, robinson@earth.northwestern.edu,