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Application of the Field System-FS9 and a PC to the antenna control unit interface in radio astronomy in Peru

Published online by Cambridge University Press:  01 August 2006

Erick Vidal
Affiliation:
Instituto Geofísico del Perú, Calle Badajoz 169, Urb. Mayorazgo IV Etapa, Ate-Vitarte, Lima 3, Perú email: evidal@axil.igp.gob.pe
José Ishitsuka
Affiliation:
Instituto Geofísico del Perú, Calle Badajoz 169, Urb. Mayorazgo IV Etapa, Ate-Vitarte, Lima 3, Perú email: evidal@axil.igp.gob.pe National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan email: pepe@hotaka.mtk.nao.ac.jp
Yasuhiro Koyama
Affiliation:
National Institute of Information and Communications Technology 893-1 Hirai, Kashima, Ibaraki, Japan email: koyama@nict.go.jp
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Abstract

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We are in the process to transform a 32m antenna in Peru, used for telecommunications, into a Radio Telescope to perform Radio Astronomy in Peru. The 32m antenna of Peru constructed by NEC was used for telecommunications with communications satellites at 6 GHz for transmission, and 4 GHz for reception.

In collaboration of National Institute of Information and Communications Technology (NICT) Japan, and National Observatory of Japan we developed an Antenna Control System for the 32m antenna in Peru. It is based on the Field System FS9, software released by NASA for VLBI station, and an interface to link PC within FS9 software (PC-FS9) and Antenna Control Unit (ACU) of the 32 meters antenna.

The PC-FS9 controls the antenna, commands are translated by interface into control signals compatibles with the ACU using: an I/O digital card with two 20bits ports to read azimuth and elevation angles, one 16bits port for reading status of ACU, one 24bits port to send pulses to start or stop operations of antenna, two channels are analogue outputs to drive the azimuth and elevation motors of the antenna, a LCD display to show the status of interface and error messages, and one serial port for communications with PC-FS9.

The first experiment of the control system was made with 11m parabolic antenna of Kashima Space Research Center-NICT, where we tested the right working of the routines implemented for de FS9 software, and simulations was made with looped data between output and input of the interface, both test were done successfully.

With this scientific instrument we will be able to contribute with researching of astrophysics. We expect to into a near future to work at 6.7GHz to study Methanol masers, and higher frequencies with some improvements of the surface of the dish.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007