***** File COMPRESS.TXT Microdensitometry performed at the NASA/Goddard Space Flight Center of more than 1000 wide-field plates of Halley's Comet has resulted in the creation of 20 gigabytes of Large-Scale Phenomena (L-SP) data for the IHW to deposit on CD-ROM. In its original uncompressed form -- every pixel being represented by a 2-byte number -- this would have required between 35 and 40 disks for the L-SP data alone! Primarily to reduce project costs, but also to create a CD-ROM archive of a size more manageable to the end user, the IHW decided several years ago that data compression techniques would be used to reduce the number of disks by a substantial factor (two or more). Following an experimentation period during which several techniques were examined, a previous pixel algorithm was chosen to accomplish the compression. While not offering the maximum compression factor among all possible techniques (including nesting of techniques), previous pixel compression does offer the advantages of being extremely simple in concept and of permitting fast, "on the fly" decompression, while at the same time yielding typical compression factors close to two. The algorithm works as follows. The compressed image byte stream starts with the byte value 255 (FF hex) followed by the full 2-byte value of the first pixel, with the bytes in standard FITS byte ordering. Thereafter, if the difference between the "i"th pixel and the "i-1"th pixel is less than 127 (absolute), that difference has the value 127 added to it (to avoid negative byte values) and is placed in the compressed byte stream as a single byte value. If, on the other hand, the difference is greater than 127 (absolute), the value 255 is placed in the byte stream followed by the original 2-byte value for the "i"th pixel. We then proceed to the next pixel as before. Thus, every 2-byte value in the compressed byte stream is prefixed with the flag value 255. Every value without such a prefix is presumed to be a 1-byte difference. The compression was accomplished using the program called PACKER, which was run on an IBM 3081 at the NASA/Goddard Space Flight Center. The source for the program is in the file PACKER.FOR, located in the SOFTWARE directory of this disc. A decompression algorithm is provided in the DECOMP subdirectory of the SOFTWARE directory, and descriptions of these routines are given in the DECOMP.TXT and PCDECOMP.TXT files of the DOCUMENT directory. The FITS header for each compressed image has been modified using the FITS extensions. The details of the modifications to the header are found in the file COMPINFO.TXT in the DOCUMENT directory. The extensions on the filenames for the compressed data (.IMQ = image, .HDR = header, and .LBL = label) follow the IHW filename conventions. To reconstruct the original FITS byte stream, the .HDR and the .IMQ files for the appropriate observation must be concatenated.