Japan Geoscience Union Meeting 2022

Presentation information

[E] Poster

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

[P-EM12] Study of coupling processes in solar-terrestrial system

Fri. Jun 3, 2022 11:00 AM - 1:00 PM Online Poster Zoom Room (5) (Ch.05)

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

11:00 AM - 1:00 PM

[PEM12-P03] Automatic derivation of ionospheric electron density profile by VIPIR2 ionosonde observation and its validation

*Michi Nishioka1, Hideo Maeno1, Hiroyuki Yamakawa1, Susumu Saito2, Takuya Tsugawa1 (1.National Institute of Information and Communications Technology, 2.Electronic Navigation Research Institute (ENRI), National Institute of Maritime, Port and Aviation Technology (MPAT))

Keywords:ionosonde, electron density profile, machine learning

An ionosonde transmits high-frequency radio waves towards the ionosphere while sweeping frequencies and measures delay time until the transmitted radio waves are reflected to the ionosonde by the ionosphere. Normally, the observation data is recorded as “ionogram” in which the signal strength is indicated with the horizontal axis of the frequency and the vertical axis of virtual height. The virtual height is derived by multiplying the speed of light by flight time and dividing by two. The virtual height is different from true height since the propagation speed of the transmission radio wave is a function of the electron density distribution and the geomagnetic field. In order to obtain the electron density distribution with respect to the “true height” from the ionogram, a procedure is required in which an echo trace is performed to read the frequency and delay time of the reflected echo one by one, and the propagation speed is considered and converted to the electron density with respect to the true height.

National Institute of Information and Communications Technology has been conducting routine ionosonde observations for many years. In this project, some parameters such as critical frequencies and virtual heights of the E- and F- layers are automatically derived, however, the echo trace has not been conducted yet. Recently, we developed a technique to trace ionospheric echoes using machine learning. The traced echoes were subjected to a procedure of deriving electron density profile against true height using the POLynominal Analysis program (POLAN). In this presentation, we will overview our derivation technique of ionospheric electron density profile. We also show some results of its validation using density profile data observed with an incoherent scatter radar and LEO satellite occultation data.