Image processing for the PMO broad-band solar fast spectrometer at 4.5-7.5 GHz

Details Image processing for the PMO broad-band solar fast spectrometer at 4.5-7.5 GHz Image processing for the PMO broad-band solar fast spectrometer at 4.5-7.5 GHz

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cha%26a..28..112j&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 28, Issue 1, p. 112-119.

Astronomy and Astrophysics

Astrophysics

Sun, Radio Radiation-Techniques, Image Processing

Scientific paper

For the postprocessing of the spectral image of a microwave burst observed by the PMO solar fast spectrometer at 4.5-7.5 GHz, we have used various image-processing methods to remove noise and interference, to make the image reflect better the burst event, and to intensify the more interesting details. The software is developed on the platform of MATLAB with good results.

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