***** File BROWSE.TXT Effective use of the 1,612 images contained in these IHW/Large-Scale Phenomena (L-SP) compressed image CD-ROMs requires that the user of the disks be able to "browse through the data" quickly to find those images and intervals which are of high scientific interest. Because of the long decompression and transfer times of the full-resolution images with current image display hardware, the goal of efficient browsing of the data can be met only if the images are placed on the discs at least a second time, in either subsampled or filtered form, and uncompressed. This was done for the compressed images on this disk and the results are located in the BROWSE directory of this CD-ROM. A set of "browse images" has been generated for which the images are uncompressed, subsampled and are no larger than 256 pixels in either dimension. In addition, the digital data have been scaled into a numerical range of 0 to 255 (one byte per pixel; the precision for most of the original images is 10 bits, requiring two bytes per pixel). The BROWSE directory of each L-SP compressed image CD-ROM contain datafiles, FITS headers, and PDS labels for the compressed images on that CD-ROM; this includes both images of Comet Halley and of calibration objects Note that the 1,612 total L-SP digital images (1,439 of the Comet, 173 of calibration objects) are deposited on multiple CD-ROMs "dedicated" to the L-S imagery. The browse images are actually stored in three places within the total set of IHW CD-ROMs. In addition to the subset of images stored in the BROWSE directory of each IHW/L-SP compressed image CD-ROM, the entire set of 1,612 digital images exists on the last of the IHW/L-SP dedicated disks in strict time order. The browse images are also interleaved with data from the other IHW disciplines in the daily data subdirectories on the "mixed" CD-ROMs. The browse data were obtained by taking the "n"th row and column for the original image starting at row "n/2" and column "n/2". The value for "n" was determined from the larger of the two axes such that the quantity (original length / n) was less than or equal to 256. For the images which were digitized at GSFC, the original densitometer values ranged between 0 and 1023 The density values in the images were divided by 4 in order to convert the density to a single byte. For those images digitized elsewhere, the density scaling factor was chosen so that the density in the browse image was less than or equal to 255. The FITS header records for the browse images have had their astrometric information adjusted to reflect the change both in pixel spacing and image origin. Thus, should the user wish, (crude) astrometry can be performed with the browse images. In addition, HISTORY keywords have been inserted to document the linear scale and density scale changes. The creation of the browse images was accomplished using the program MIDGET, which can be found a MIDGET.FOR in the SOFTWARE directory of this CD-ROM.