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Korea Geodetic VLBI Station, Sejong

2013 
The Sejong VLBI station officially joined the IVS as a new Network Station in 2012. This report summarizes the activities of the Sejong station during 2012. The following are the activities at the station. 1) VLBI test observations were carried out with the Tsukuba 34-m antenna of the GSI in Japan. As a result, the Sejong antenna needs to improve its efficiency, which is currently in progress. 2) A survey to connect the VLBI reference point to GNSS and ground marks was conducted. 3) To see the indirect effects of RFI (Radio Frequency Interference) at this place, we checked the omni-direction (AZ 0◦ to 360◦, EL fixed at 7◦) for RFI influence. 1. General Information The Sejong station is the first geodetic VLBI station in the Republic of Korea which is dedicated to geodetic purposes only. The station is located about 120 km south of Seoul, in the middle of Sejong City, which serves as a new administrative capital. The Sejong antenna is 22 meters in diameter, and its slew speed is 5/sec in both azimuth and elevation; its specifications have been designed for the possible addition of other small antennas in the future. The observatory was constructed on the top of a small mountain in Sejong City, which was officially approved as a new town in July 2012. The city is a newly designated administrative capital city planned by the government, and it will be developed in phases over the next 20 years. The Sejong VLBI station was previously called “KVG” (Korea VLBI system for Geodesy) which was named after the project purpose in its initial stage. However, now “Sejong Station” is the official title to prevent possible confusion in addressing the station. National Geographic Information Institute (NGII, http://ngii.go.kr) manages the observatory, and Table 1 shows the staff members of the Sejong station. A newly appointed site director, Mr. Baek Dong Hyun, started work in November 2012, and Mr. Joo Hyun Hee, who showed outstanding work in Sejong VLBI construction, was transferred to another group. Staff at the observatory carry out the VLBI observation, baseline analysis, international cooperation including the IVS, antenna maintenance, and management of the observatory. Table 1. Staff members of the Sejong station. Name Function e-mail Baek Donghyun Site Director baekdh@korea.kr Yi Sangoh S/W engineer sangoh.yi@korea.kr Oh Hongjong H/W engineer stockoh11@korea.kr Han Sangchul Antenna system hsc4907@korea.kr 2. Sejong VLBI System The Sejong VLBI configuration is listed in Table 2. The IVS letter codes and the CDP and DOMES numbers have been newly registered during this year. The antenna has the Cassegrain IVS 2012 Annual Report 135 Sejong Station National Geographic Information Institute Figure 1. VLBI 22-m antenna, monument pillars 1 4, GNSS, and UCP (Unified Control Point) layout. shape, and the 22-m main reflector consists of 200 rectangular aluminium panels. Each panel has four elevation adjustments at the edge of the panel, so that the antenna main reflector surface can be properly arranged. Technical parameters of the receiver are presented in Table 3. However, some items are omitted due to the antenna efficiency improvement work. The Sejong station uses the Field System (version FS-9.10.4) and a K5 data recorder. 3. Activities in 2012 3.1. VLBI Observation The Sejong antenna carried out several fringe tests with the Tsukuba 34-m antenna in Japan. A few observations failed to get fringes due to a wrong setting for time synchronization. After that we successfully got fringes from all channels in the S and X bands. As a result, the Sejong antenna needs to improve its antenna efficiency, which is currently in progress. 3.2. Co-location We performed a ground survey that used four pillars to tie the cross point of the axes of the VLBI antenna to the Sejong GNSS monument. Figure 2 shows the local tie layout in the site. The antenna reference position was calculated by a 3D circle fitting method, with measurement of the distances from the pillars to the reflection sheet on the antenna surface. Therefore, a ground network consisting of VLBI, GNSS, and the pillars was established. Monitoring for the antenna reference position and ground subsidence of the new site will regularly be done by local tie survey. 136 IVS 2012 Annual Report National Geographic Information Institute Sejong Station Table 2. Sejong Antenna parameters. Parameters Sejong VLBI IVS letter codes Sejong (Kv) CDP number 7368 DOMES number 23907S001 Location 12718’E, 3631’N Elevation 177m Diameter of main reflector 22m Antenna type Shaped Cassegrain Aperture efficiency about 60% Pointing accuracy 0.0131 Reflector surface accuracy 86μm Operation range AZ: ±270 EL: 0 ∼ 90 Slew speed 5/sec (AZ and EL) FS Version 9.10.4 Data acquisition Rack/Recorder K4/K5 Table 3. Receiving system of the Sejong VLBI system. Bands S X K Q Freq. [GHz] 2.1-2.6 8.0-9.0 21-23 42-44 Receiver noise temp. < 20K < 30K < 50K < 80K Polarization R,L R,L R,L R,L First LO Freq. NONE NONE 13.5 GHz 33.9 GHz First IF Freq. NONE NONE 8-10 GHz 8-10 GHz IF Pout/BW -50 dbm/500 MHz Phase noise@1KHz -120 dBc/Hz Reference Freq. 100 MHz 3.3. RFI Monitoring Even at the Sejong site, RFI is unavoidable. We scanned all directions (AZ 0 to 360) at a fixed elevation of 7 to see the maximum values in S band (2.2 ∼ 2.4GHz). Figure 3 shows the change of signal power. It shows that most RFI is detected over 2.3 GHz. It is also direction-dependent. In other words, there was more RFI coming from the north direction. 4. Future Plans We will take on the following activities in 2013: 1) The Sejong station, as a new IVS Network Station in 2012, will participate in regular IVS sessions. 2) Antenna efficiency improvement is currently in progress. 3) After that, we will proceed to join IVS observing as soon as possible by contacting the IVS Coordinating Center. 4) A local tie survey is also planned. IVS 2012 Annual Report 137 Sejong Station National Geographic Information Institute Figure 2. Facilities for local ties at the Sejong station. Figure 3. RFI measurement results using a spectrum analyzer. 138 IVS 2012 Annual Report
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