Author: BSW Team Subject: New ANTEX v1.3 converter Dear BSW users, The IGS plans to change the antenna model from relative PCV to absolute PCV in the near future. The official date of the changes to the new IGS antenna model is not yet specified in detail (see: http://igscb.jpl.nasa.gov/mail/igsmail/2005/msg00193.html). * The new converter The BSW, Version 5.0, is already prepared for these changes. The only program that needs to be updated is the tool that converts files from ANTEX v1.3 to Bernese PCV format. In addition the satellite information file has to be updated. The new converter allows for a variety of new and helpful options including - preparation of a completely new Bernese PCV file (relative or absolute) from ANTEX, - updating of the currently used old Bernese PCV file (containing old satellite antenna names and no radome codes) with information from ANTEX, - updating of the Bernese PCV file in case of new PCV calibration values, - conversion of relative Bernese PCV file (with all included antennas) to an absolute Bernese PCV file, - merging of new or individually calibrated antenna patterns from (relative or absolute) ANTEX to your existing (relative or absolute) Bernese PCV file, and - adding patterns of antenna radome combinations that are not included in ANTEX to the Bernese PCV file. * Consistency of phase eccentricity file and satellite information file If absolute receiver antenna patterns are used, absolute satellite antenna patterns have to be used, too. Because absolute ANTEX files contain satellite-specific patterns, the implementation of the new converter requires the replacement of the satellite information file. Because satellite antenna offsets are stored in this file (as in previous versions), care has to be taken to always use the phase eccentricity file together with the corresponding satellite information file. Note that Version 4.2 is not capable to handle absolute satellite antenna patterns. * Radome codes Because, according to the new IGS policy, radome codes will be used consistently for all antennas, the new converter forces the use of radome codes. Take your time to adapt your Bernese PCV file and station information file accordingly. More information is provided in a detailed readme file (see below). * How to proceed Note, that it is not necessary to switch to the new satellite information file before the official change of the antenna model in the IGS. But performing the switch to the new (relative) files already now is a good preparation for the official switch within the IGS. Some of the users already want to run tests with the new absolute antenna models. Consistent Bernese phase eccentricity files and satellite information files are prepared by AIUB and are available at the anonymous ftp server (see below). Be sure to never mix absolute and relative PCV and satellite information files! * More details For detailed instructions concerning the ANTEX converter and the new satellite information files see the readme_antex.txt file available at the anonymous ftp server http://www.aiub.unibe.ch/download/BSWUSER50/GEN We hope that the new converter helps you to smoothly switch to absolute antenna phase patterns. In case of problems or questions do not hesitate to contact us. Best regards The BSW Team