EGU2020-21810
https://doi.org/10.5194/egusphere-egu2020-21810
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Ionospheric Weather Observations of FORMOSAT-7/COSMIC-2

Fu-Yuan Chang1, Jann-Yenq Liu1, Chi-Yen Lin1, Shih-Ping Chen2, and Charles Lin2
Fu-Yuan Chang et al.
  • 1Center for Astronautical Physic and Engineering, National Central University, Taoyuan, Taiwan (tigerjyliu@gmail.com)
  • 2Department of Geosciences, National Cheng Kung University, Tainan, Taiwan (charles@mail.ncku.edu.tw )

FORMOSAT-7/COSMIC-2 (F7/C2), with the mission orbit of 550 km altitude, 24-deg inclination, and a period of 97 minutes, was launched on June 25, 2019.  Tri-GNSS Radio occultation (RO) receiver System (TGRS), Ion Velocity Meter (IVM), and RF Beacon (RFB) onboard F7/C2 six small satellites allow scientists to three-dimensionally observe the plasma structure and dynamics in the mid-latitude, low-latitude, and equatorial ionosphere.  Measurements of F7/C2 RO as well as the IVM ion density, ion temperature, and ion velocity have a better understanding on mechanisms of the plasma depletion bays, non-migrating tides, and scintillations.  Moreover, observations of ionospheric F7/C2 RO electron density profiles and the total electron content derived from global ground-based GNSS receivers are used to carry out ionospheric weather monitoring, nowcast, and forecast for positioning, navigation, and communication application.

How to cite: Chang, F.-Y., Liu, J.-Y., Lin, C.-Y., Chen, S.-P., and Lin, C.: Ionospheric Weather Observations of FORMOSAT-7/COSMIC-2, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-21810, https://doi.org/10.5194/egusphere-egu2020-21810, 2020