The Hiraiso Radio Spectrograph (HiRAS) for Monitoring Solar Radio Bursts

Details The Hiraiso Radio Spectrograph (HiRAS) for Monitoring Solar Radio Bursts The Hiraiso Radio Spectrograph (HiRAS) for Monitoring Solar Radio Bursts

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995clrj..42...111k&link_type=abstract

Journal of the Communications Research Laboratory, vol. 42, p. 111

Computer Science

Radio Signals, Spectrographs, Solar Radio Bursts, Monitors, Data Processing, Television Systems, Spectrograms, Spectra, Signal To Noise Ratios, Frequencies, Broadband

Scientific paper

A wideband radio spectrograph for monitoring solar radio emissions (receiving 25-2500 MHz) was newly installed at Hiraiso Solar Terrestrial Research Center in 1993. The spectrograph consists of three different frequency band antennas. Spectrum data from each antenna is combined to form a composite dynamic spectrogram. A data processing method based on the selection of minimum-data has been developed to remove man made interference such as radio and television signals. from raw spectrum-data. It has been successfully applied to actual observations and has served to improve the signal-to-noise ratio of solar- burst emission spectrogram.

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