Japan Geoscience Union Meeting 2025

Presentation information

[E] Oral

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

[P-EM15] Dynamics of Magnetosphere and Ionosphere

Thu. May 29, 2025 3:30 PM - 5:00 PM 302 (International Conference Hall, Makuhari Messe)

convener:Shun Imajo(Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University), Yuka Sato(Nippon Institute of Technology), Akiko Fujimoto(Kyushu Institute of Technology), Kazuhiro Yamamoto(Institute for Space-Earth Environmental Research), Chairperson:Tomoaki Hori(Institute for Space-Earth Environmental Research, Nagoya University), Mizuki Fukizawa(National Institute of Polar Research)


4:30 PM - 4:45 PM

[PEM15-21] Diurnal periodicity in Earth’s radio emissions

*Alexandra Ruth Fogg1, Caitríona M. Jackman1, Simon J. Walker1, Matthew J. Rutala1 (1.School of Cosmic Physics, Dublin Institute for Advanced Studies, DIAS Dunsink Observatory, Dublin D15 XR2R, Ireland)

Keywords:Earth, Space Weather, Radio Emissions, Auroral Kilometric Radiation, Diurnal periodicity, Substorm

Planetary radio emissions have potential as a very valuable remote diagnostic of planetary rotation rates as well as magnetospheric dynamics. Auroral Kilometric Radiation (AKR) is Earth’s strongest natural radio emission, and is anisotropically beamed from a source locked to auroral latitude magnetic field lines. These field lines are tied to the deep interior of the rotating planet, and hence it is theorised that an observer at a fixed local time will observe a diurnal variation in AKR power, as if the Earth and its emission were a lighthouse. In this study we explore this proposed 24 hour periodicity in AKR power using a decade of observations from Wind/WAVES.