Japan Geoscience Union Meeting 2024

Presentation information

[E] Oral

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

[P-EM11] Space Weather and Space Climate

Tue. May 28, 2024 1:45 PM - 3:15 PM Exhibition Hall Special Setting (2) (Exhibition Hall 6, Makuhari Messe)

convener:Ryuho Kataoka(National Institute of Polar Research), Mary Aronne(NASA Goddard Space Flight Center), Yumi Bamba(National Institute of Information and Communications Technology), Antti Pulkkinen(NASA Goddard Space Flight Center), Chairperson:Ryuho Kataoka(National Institute of Polar Research), Mary Aronne

3:00 PM - 3:15 PM

[PEM11-21] Observation of the Doppler frequency shift of the HF wave transmitted by an ionosonde

*Takashi Iwamoto1, Mao Konishi1 (1.Mitsubishi Electric Corporation)

Keywords:observation, Doppler frequency shift, ionosonde, equatorial spread F, cross-correlation, replica

Navigation satellite systems are now used in a wide variety of applications and are known to suffer from ionospheric disturbances such as the post-sunset equatorial spread F (ESF). For forecasting post-sunset ESF, the potential of ionosondes is assessed and the vertical plasma drift velocity is reported to correlate with the post-sunset ESF with a criterion of 30 m/s for high probability of occurrence. The difference between two consecutive ionograms is used to estimate the velocity [1]. However, the velocity can also be measured directly as the Doppler frequency shift of the wave reflected from the ionosphere [2]. An example of such an observation is shown as below.

The Doppler frequency shift of the pulse train transmitted by the Chung-Li ionosonde [3] starting at 19:00 on January 18, 2024 (UT) is analyzed as shown in the figure. A heat map of the absolute values of the summed cross-correlations between the received samples and the model replicas is plotted against the Doppler frequency shift multiplied by the replicas (horizontal axis) and the relative time of flight (vertical axis). A course resolution of 2 Hz of the Doppler frequency shift is shown. This resolution can resolve the 30 m/s vertical velocity, when the ionosphere reflects the 10 MHz vertical incident wave. It is straightforward to obtain a more accurate estimate of the Doppler frequency shift according to the signal-to-noise ratio of the samples using the maximum likelihood method.

[1] P. Abadi, U. A. Ahmad, Y. Otsuka, P. Jamjareegulgarn, A. Almahi, S. Perwitasari, S. Supriadi, W. Harjupa, and R. R. Septiawan, `Assessing the potential of ionosonde for forecasting post-sunset equatorial spread F: an observational experiment in Southeast Asia,’ Earth Planets Space, vol. 75, 2023.
[2] T. Iwamoto, M. Konishi, N. Ikeda, and S. Kameoka, `Observation of Doppler frequency shift and time of flight of a temporally modulated HF wave propagating through ionosphere,’ the Japan Geoscience Union Meeting 2022, Chiba, Japan, May 2022.
[3] K.-J. Ke, C.-L. Su, R.-M. Kuong, H.-C. Chen, H.-S. Lin, P.-H. Chiu, C.-Y. Ko, and Y.-H. Chu, `New Chung-Li Ionosonde in Taiwan: System Description and Preliminary Results,’ Remote Sensing, vol. 14, 2022.

Figure caption:
A heat map of the absolute values of the summed cross-correlations between the received samples of the pulse train transmitted starting at 19:00 on January 18, 2024 (UT) and the model replicas is plotted against the Doppler frequency shift multiplied by the replicas (horizontal axis) and the relative time of flight (vertical axis).