Huirong Ji scite author profile

Abstract. On 23 September 1998 there was a 3B/M7.1 flare event starting at 06:40 UT with more than 100 minute duration radio bursts of 1134 sfu peak flux at 2840 MHz and accompanying a CME. In this paper, the event is analyzed with the data observed by Beijing Astronomical Observatory (BAG), OSRA-Tremsdorf (AlP) and SSRT-ISTP. In particular, we compare the fine structures (FS) during the triggering phase revealed in different regimes and discuss their implications.

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A modified four-arm, mode-2, wide-beam archimedean spiral antenna

Wang

et al. 2017

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Huirong Ji

A broadband spectrometer for decimeter and microwave radio bursts

A New Solar Broadband Radio Spectrometer (SBRS) in China

Nonlinear calibration and data processing of the solar radio burst

Statistical study of radio drifting pulsation structures with associated CMEs and other observations

A radio spectrometer at 2.6–3.8 GHz

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On the Initial Phase of Solar Radio Burst Event on 23 September 1998

A modified four-arm, mode-2, wide-beam archimedean spiral antenna

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