Received: from dutlru3.lr.tudelft.nl (dutlru3.lr.tudelft.nl [130.161.165.63]) by igscb.jpl.nasa.gov (8.9.3/8.9.3) with ESMTP id NAA29905 for ; Tue, 11 Jan 2000 13:49:19 -0800 Received: (from bac@localhost) by dutlru3.lr.tudelft.nl (8.9.3/8.9.3) id WAA12622 for igsmail@igscb.jpl.nasa.gov; Tue, 11 Jan 2000 22:49:17 +0100 From: Boudewijn Ambrosius Message-Id: <200001112149.WAA12622@dutlru3.lr.tudelft.nl> Subject: [IGSMAIL-2668]: Changes at WSRT (Westerbork, the Netherlands) To: igsmail@igscb.jpl.nasa.gov Date: Tue, 11 Jan 2000 22:49:16 +0100 (MET) X-Mailer: ELM [version 2.5 PL2] MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit Sender: owner-igsmail Precedence: bulk ****************************************************************************** IGS Electronic Mail 11 Jan 13:49:22 PST 2000 Message Number 2668 ****************************************************************************** Author: Boudewijn Ambrosius & Danny van Loon (DEOS/DUT) On January 5th, 2000, around 14:00 UT, the ROGUE SNR-12 RM (nr. 209) at station WSRT (Westerbork, the Netherlands) was replaced by an AOA SNR-12 ACT (nr. 225) receiver. This reflects our continuous efforts to establish the WSRT station as a high quality replacement for the KOSG station, which is still operational, but which may be phased out sometime in the future. We hope the WSRT station will eventually take over the role as the principal IGS reference point in the Netherlands from the highly successful KOSG station, which has been operational for almost 10 years now. Once again, we urge all analysis centers to include the WSRT station in their primary networks, since it has been dedicated to become the fundamental geodetic reference point in the Netherlands, replacing KOSG. The last few hours of tracking data from the SNR-12 receiver of WSRT on day 5 have NOT been distributed to IGS to avoid data incompatibility. Therefore only a partial file with data from the new ACT receiver on that day was submitted. Since then, full daily files have been submitted for subsequent days, including the C1 data type. Around the same time, the reciever was changed, the H-MASER frequency standard at WSRT broke down. After this was noticed on January 6th, the external H-MASER was disconnected and the receiver was temporarily reconfigured to run from its internal oscillator in clock steering mode on January 6th, at about 16:00 UT. We hope the H-MASER will soon be repaired after which it will be reconnected. The above changes are reflected in an updated site log, which will be submitted later today. Boudewijn and Danny