EGU24-2985, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-2985
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Equatorial Plasma Density Irregularities Observed by Advanced Ionospheric Probe Onboard FORMOSAT-5 Satellite

Chi-Kuang Chao
Chi-Kuang Chao
  • Department of Space Science and Engineering, National Central University, Chung-Li, Taiwan (ckchao@jupiter.ss.ncu.edu.tw)

A FORMOSAT-5 satellite was launched on 25 August 2017 CST into a 98.28° inclination sun-synchronous circular orbit at 720 km altitude along the 1030/2230 local time sectors.  Advanced Ionospheric Probe (AIP), a piggyback science payload developed by National Central University for the FORMOSAT-5 satellite, has measured in-situ ionospheric plasma concentrations at a 1,024 Hz sampling rate over a wide range of spatial scales for more than 6 years.  In this poster, global plasma density irregularities in the pre-midnight sector had been seasonally selected from FORMOSAT-5/AIP data during 2018 to 2023.  Yearly variations of these irregularity patterns with solar cycle could be clearly observed.

How to cite: Chao, C.-K.: Equatorial Plasma Density Irregularities Observed by Advanced Ionospheric Probe Onboard FORMOSAT-5 Satellite, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-2985, https://doi.org/10.5194/egusphere-egu24-2985, 2024.