Japan Geoscience Union Meeting 2021

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P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM13] Study of coupling processes in solar-terrestrial system

Fri. Jun 4, 2021 5:15 PM - 6:30 PM Ch.05

convener:Mamoru Yamamoto(Research Institute for Sustainable Humanosphere, Kyoto University), Yasunobu Ogawa(National Institute of Polar Research), Satonori Nozawa(Institute for Space-Earth Environmental Research, Nagoya University), Akimasa Yoshikawa(Department of Earth and Planetary Sciences, Kyushu University)

5:15 PM - 6:30 PM

[PEM13-P07] Development of an Autonomous Method for Equatorial Spread-F (ESF) Detection of SEALION Ionosonde Data

*Septi Perwitasari1, Kornyanat Hozumi1 (1.National Institute of Information and Communications Technology)

Keywords:Equatorial Spread-F, Ionogram, Autonomous detection

Equatorial spread-F (ESF) is one of the most important features in space weather because of its significant effect on communication and navigation. Therefore, real-time information on the ESF occurrence will be useful to detect the degradation of radio propagation conditions. SEALION is an ionospheric observation network in the South East Asia that has been on operation since 2003. SEALION has 5 FMWC ionosondes installed in various locations; Chiang Mai (18.76°N, 98.93°E), Chumphon(10.72°N, 99.37°E), Phuket (7.90°N, 98.39°E), Bac Liu (9.30°N, 105.71°E), Cebu (10.35°N, 123.91°E) and Kototabang (0.20°S, 100.32°E). SEALION ionograms are often contaminated with various noises, such as stripes and random noises. Thus, a noise removal step is crucial before applying any detection algorithm. To remove the noises, we applied 4th degree polynomial fit to remove the stripes and 3x3 median filter to reduce the random noise. Following Bhaneja et al., 2009’ method, the h’F and foF2 trace are determined using an edge detection algorithm. Thresholds of non-spread F ionogram are determined by calculating the number of pixel within 100x100 pixel box from the edge of the h’F and foF2. The thresholds were calculated from ~1000 nighttime ionograms from different seasons. We identified the range type ESF when the pixel counts within the h’F box exceeded the threshold. The frequency type was identified when the pixel counts within the foF2 box exceeded the threshold. The mixed type are identified when the pixel counts in both h’F and foF2 boxes were exceeding the threshold. We have applied this method to 2013 Chiang Mai ionograms. The preliminary result shows ~88 % matching with the manual scaling. The application of this method to the data from other ionosonde stations is underway. The details of the method, result, possible improvement of the current method and the design for a real-time warning system will be discussed during the presentation.