Radio Telescope


WCC's Lanihuli Observatory operates a slewable log-periodic radio telescope that supports NASA's Radio JOVE Project, which monitors natural radio emission from Jupiter, the Sun and our Milky Way Galaxy. This radio telescope can be tuned to frequencies between 18 and 30 MHz. In addition, the observatory's NOAA Weather Satellite 1.5-meter diameter mesh dish antenna, which is tuned to 1700 MHz for satellite reception, can also be used to record radio emission from the Sun.

Log-Period Antenna
Cosmic Ray Detector

Lanihuli Iki (NOAA Dish Antenna)
Cosmic Ray Detector

Log-Periodic Antenna (Radio JOVE)

Signals captured by the log-period antenna are routed to the observatory's control room and processed by an FS200 radio spectrograph that operates within the range from 18 to 30 MHz. This spectrograph is capable of scanning 200 channels 10 times per second, yielding a total of 2000 samples per second.  

Radio Telescope Control Center
Radio Telescope Control Room

This log-periodic antenna is used primarily to support the WCC's Radio JOVE Project, which is sponsored by NASA Goddard Space Flight Center. This project focuses on monitoring three particular radio sources:        

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1.5m Mesh Dish Antenna (NOAA Weather Station)

The NOAA Weather Tracking antenna is capable of recording the solar image at a frequence of 1700 MHz. While this technique is normally used to align the antenna for accurate tracking of the polar orbiting NOAA satellites, it can also serve to record a radio image of the Sun. The following shows a typical scanned plot of the Sun's radio noise:

NOAA Solar Radio Noise Plot

Histograph plot of Solar Radio Noise


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Center for Aerospace Education
Windward Community College
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updated: 2/20/22