Corresponding Person: [email protected]@asiaa.sinica.edu.tw Phone: 886-2-33652200,...

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Corresponding Person: [email protected] Phone: 886-2-33652200, Fax: 886-2-23677849 S.W. Chang 2008/03 ASIAA SMA Antenna Monitoring System of Submillimeter Array Su-Wei Chang , Derek Kubo * , Paul Yamaguchi , Brain Koge * ‡: Academia Sinica Institute of Astronomy & Astrophysics, Taipei, Taiwan, R.O.C. * : Academia Sinica, Institute for Astronomy & Astrophysics, Hilo, HI 96720, USA : Smithsonian Submillimeter Array, Hilo, HI 96720, USA Introduction An antenna monitoring system (AMS) is developed for monitori ng specific critical signals within the antenna of Submillimeter Arr ay (SMA). This system is composed by a network of RF-switches whi ch controlled by the National Instrument (NI) ethernet to TTL switc h controller, and using HP 8563E spectrum analyzer to monitor all t he signals. Figure 1 describes the proposed system setup in an ant enna cabin which has the capability to monitor one of twenty sign als using a spectrum analyzer. The monitored signals are as follows: a) Gunn 109MHz IF monitor (8 possible signals) b) 109/200 MHz monitor references for both LO1 and LO2 (2 signals) c) 200 MHz YIG PLL error monitor for YIG1 and YIG2 (2 signals) d) YIG1 and YIG2 monitor outputs (2 signals, 5.3 to 8.7 GHz) e) IF1 and IF2 post amplified and leveled monitor outputs (2 signals, 4 to 6 GHz) f) MRG LO1 and LO2 monitor reference (1 signal, 5.5 to 8.5 GHz) These test points permit monitoring of the signals without interrup tion through the use of built-in directional couplers allowing simul taneous measurement with observations. All switches will be TTL c ontrolled and of 50 Ohm termination to prevent reflection of unmo nitored signals. The switches will likely be located within the metal enclosure to minimize the number of physical penetrations and to reduce potential EMI leakage into the cabin. Fig. 1. Proposed Antenna Monitoring System Fig. 2. These pictures show the two switches located inside the IF/LO enclos ure. Left photo – JFW switch (S3) connected to the low frequency sign als, mid photo – Miteq switch (S4) connected to the high frequency si gnals, right photo – the connectors J7 to J12 mounted on the enclosu re TTL controller Dow-Key Switch (S5) DC Power Suppl y Fig. 3. Left photo is the HP 8563E Spectrum Analyzer. Right photo sh ows the NI ethernet to TTL switch controller, the Dow-Key swi tch (S5) which is the final switch collected all the input signal s and went to the spectrum analyzer, and the DC power supp ly to power all the switches and the TTL controller Remote Software Programming The first version of the remote software for the AMS syste m was programmed and tested. The Labview software is used t o control the TTL controller and monitor the spectrum analyzer. There are 15 JPEG spectrum photos and one row data taken by the software automatically. This program resides on a PC whic h is physically located at the summit of Manua Kea. Fig. 4. The first version of the Labview remote program. Left photo – the front controlled panel, right photo – the monitoring spect rum results Fig. 5. The 15 spectrum photos and one row data taken by the Labvi ew program Conclusion and Future Works The AMS system has been prototyped and tested in antenna 7 for development purposes. The program successfully control the RF switches and also display the desired signals of interest. The further progress is revised the program and integrated into the SMA Observation Center for the real operation purpose.

Transcript of Corresponding Person: [email protected]@asiaa.sinica.edu.tw Phone: 886-2-33652200,...

Page 1: Corresponding Person: swchang@asiaa.sinica.edu.twswchang@asiaa.sinica.edu.tw Phone: 886-2-33652200, Fax: 886-2-23677849 S.W. Chang 2008/03 ASIAA SMA Antenna.

Corresponding Person: [email protected]: 886-2-33652200, Fax: 886-2-23677849

S.W. Chang 2008/03

ASIAA

SMA

Antenna Monitoring System of Submillimeter Array Su-Wei Chang ‡, Derek Kubo* , Paul Yamaguchi†, Brain Koge*

‡: Academia Sinica Institute of Astronomy & Astrophysics, Taipei, Taiwan, R.O.C.* : Academia Sinica, Institute for Astronomy & Astrophysics, Hilo, HI 96720, USA

† : Smithsonian Submillimeter Array, Hilo, HI 96720, USA

IntroductionAn antenna monitoring system (AMS) is developed for monitoring speci

fic critical signals within the antenna of Submillimeter Array (SMA). This system is composed by a network of RF-switches which controlled by the National Instrument (NI) ethernet to TTL switch controller, and using HP 8563E spectrum analyzer to monitor all the signals. Figure 1 describes the proposed system setup in an antenna cabin which has the capability to monitor one of twenty signals using a spectrum analyzer. The monitoredsignals are as follows:

a) Gunn 109MHz IF monitor (8 possible signals) b) 109/200 MHz monitor references for both LO1 and LO2 (2 signals) c) 200 MHz YIG PLL error monitor for YIG1 and YIG2 (2 signals) d) YIG1 and YIG2 monitor outputs (2 signals, 5.3 to 8.7 GHz) e) IF1 and IF2 post amplified and leveled monitor outputs (2 signals, 4 to 6 GHz) f) MRG LO1 and LO2 monitor reference (1 signal, 5.5 to 8.5 GHz)

These test points permit monitoring of the signals without interruption through the use of built-in directional couplers allowing simultaneous measurement with observations. All switches will be TTL controlled and of 50 Ohm termination to prevent reflection of unmonitored signals. The switches will likely be located within the metal enclosure to minimize the number of physical penetrations and to reduce potential EMI leakage intothe cabin.

Fig. 1. Proposed Antenna Monitoring System

Fig. 2. These pictures show the two switches located inside the IF/LO enclosure. Left photo – JFW switch (S3) connected to the low frequency signals, mid photo – Miteq switch (S4) connected to the high frequency signals, right photo – the connectors J7 to J12 mounted on the enclosure

TTL controller

Dow-Key

Switch (S5)

DC Power Supply

Fig. 3. Left photo is the HP 8563E Spectrum Analyzer. Right photo shows the NI ethernet to TTL switch controller, the Dow-Key switch (S5) which is the final switch collected all the input signals and went to the spectrum analyzer, and the DC power supply to power all the switches and the TTL controller

Remote Software Programming The first version of the remote software for the AMS system was pro

grammed and tested. The Labview software is used to control the TTL controller and monitor the spectrum analyzer. There are 15 JPEG spectrum photos and one row data taken by the software automatically. This program resides on a PC which is physically located at the summitof Manua Kea.

Fig. 4. The first version of the Labview remote program. Left photo – the front controlled panel, right photo – the monitoring spectrum results

Fig. 5. The 15 spectrum photos and one row data taken by the Labview program

Conclusion and Future Works The AMS system has been prototyped and tested in antenna 7 for

development purposes. The program successfully control the RF switches and also display the desired signals of interest. The further progress is revised the program and integrated into the SMA Observation Center for the real operation purpose.