Japan Geoscience Union Meeting 2022

Presentation information

[E] Poster

S (Solid Earth Sciences ) » S-GC Geochemistry

[S-GC35] Volatiles in the Earth - from Surface to Deep Mantle

Sun. May 29, 2022 4:00 PM - 6:00 PM Online Poster Zoom Room (18) (Ch.18)

convener:Hirochika Sumino(Department of General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo), convener:Yama Tomonaga(Swiss Federal Institute of Aquatic Science and Technology), Yuji Sano(Center for Advanced Marine Core Research, Kochi University ), convener:Takeshi Hanyu(Japan Agency for Marine-Earth Science and Technology, Research Institute for Marine Geodynamics), Chairperson:Yama Tomonaga(Swiss Federal Institute of Aquatic Science and Technology), Takeshi Hanyu(Japan Agency for Marine-Earth Science and Technology, Research Institute for Marine Geodynamics), Yuji Sano(Center for Advanced Marine Core Research, Kochi University), Hirochika Sumino(Department of General Systems Studies, Graduate School of Arts and Sciences, The University of Tokyo)

4:00 PM - 6:00 PM

[SGC35-P05] Solar flare activity as a new, unknown source of 3He in the atmosphere

*Yuji Sano1, Teresa M Escobar2, Naoto Takahata2, Maoliang Zhang3, Daisuke Goto4, Daniele L Pinti5, Bernard Marty6 (1.Center for Advanced Marine Core Research, Kochi University , 2.Atmosphere and Ocean Research Institute, University of Tokyo, 3.Tianjin University, 4.National Institute of Polar Research, 5.University of Quebeck, Montreal, 6.University of Lorraine)

Keywords:Helium Isotopes, Atmosphere, Solar flare

Measurements of helium in the atmosphere suggest a supply of crustal 4He from fossil fuel emissions since the onset of industrial activity [1,2]. However, corresponding 3He/4He ratio of air appears near-constant [3,4], which calls for an unknown source of 3He to compensate contribution of anthropogenic 4He. Here we report 3He/4He variations measured in atmospheric air during a solar flare event. Samples were collected in Ny-Ålesund, Svalbard islands near the North Pole. On September 6th, 2017, a massive solar explosion, or solar flare, occurred. The solar wind was expected to reach the Earth on September 8th [5]. Therefore, the dates of air sample collection were set for eight days about one week apart, from August 30th to October 18th, 2017. The 3He/4He ratios were measured in the samples and calibrated against the standard atmosphere collected in Kashiwa City, Chiba Prefecture, Japan [6]. The 3He/4He ratios varied from -6.1‰ to +7.9‰ compared the air standard. The 3He/4He ratios of 12 samples agreed with the atmospheric values of Kashiwa within uncertainties. A total of five samples showed an excess of 3He compared the atmospheric ratio. These samples were collected on September 13th, 20th, and 27th, immediately after the solar flare event of September 6th. If the solar wind, enhanced by solar flares, was fed into the atmosphere by the auroral precipitation mechanism [7], it would increase the polar atmospheric helium isotope ratio. The helium would then be diluted by diffusion and the excess 3He would rapidly disappear. We therefore propose that the unknown source of 3He capable to compensate for anthropogenic addition of 4He is the injection of solar wind-derived 3He into the atmosphere.

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