Direct Evidence of Drift‐Compressional Wave Generation in the Earth's Magnetosphere Detected by Arase

Author:

Yamamoto K.1ORCID,Rubtsov A. V.2ORCID,Kostarev D. V.2ORCID,Mager P. N.2ORCID,Klimushkin D. Yu.2ORCID,Nosé M.3ORCID,Matsuoka A.4ORCID,Asamura K.5ORCID,Miyoshi Y.6ORCID,Yokota S.7ORCID,Kasahara S.1ORCID,Hori T.6ORCID,Keika K.1ORCID,Kasahara Y.8ORCID,Kumamoto A.9ORCID,Tsuchiya F.9ORCID,Shoji M.6ORCID,Nakamura S.6ORCID,Shinohara I.5ORCID

Affiliation:

1. Graduate School of Science The University of Tokyo Tokyo Japan

2. Institute of Solar‐Terrestrial Physics SB RAS Irkutsk Russia

3. School of Data Science Nagoya City University Nagoya Japan

4. Graduate School of Science Kyoto University Kyoto Japan

5. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency Sagamihara Japan

6. Institute for Space‐Earth Environmental Research, Nagoya University Nagoya Japan

7. Graduate School of Science Osaka University Toyonaka Japan

8. Graduate School of Natural Science and Technology Kanazawa University Kanazawa Japan

9. Graduate School of Science Tohoku University Sendai Japan

Abstract

AbstractWe present the first direct evidence of an in situ excitation of drift‐compressional waves driven by drift resonance with ring current protons in the magnetosphere. Compressional Pc4–5 waves with frequencies of 4–12 mHz were observed by the Arase satellite near the magnetic equator at L ∼ 6 in the evening sector on 19 November 2018. Estimated azimuthal wave numbers (m) ranged from −100 to −130. The observed frequency was consistent with that calculated using the drift‐compressional mode theory, whereas the plasma anisotropy was too small to excite the drift‐mirror mode. We discovered that the energy source of the wave was a drift resonance instability, which was generated by the negative radial gradient in a proton phase space density at 20–25 keV. This proton distribution is attributed to a temporal variation of the electric field, which formed the observed multiple‐nose structures of ring current protons.

Funder

Ministry of Science and Higher Education of the Russian Federation

Publisher

American Geophysical Union (AGU)

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