K Keika
Overview
Explore the profile of K Keika including associated specialties, affiliations and a list of published articles.
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Articles
4
Citations
51
Followers
0
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Recent Articles
1.
Kurita S, Miyoshi Y, Saito S, Kasahara S, Katoh Y, Matsuda S, et al.
Sci Rep
. 2025 Jan;
15(1):992.
PMID: 39809762
Electromagnetic whistler-mode chorus waves are a key driver of variations in energetic electron fluxes in the Earth's magnetosphere through the wave-particle interaction. Traditionally understood as a diffusive process, these interactions...
2.
Kistler L, Asamura K, Kasahara S, Miyoshi Y, Mouikis C, Keika K, et al.
Nat Commun
. 2023 Oct;
14(1):6143.
PMID: 37903790
Both solar wind and ionospheric sources contribute to the magnetotail plasma sheet, but how their contribution changes during a geomagnetic storm is an open question. The source is critical because...
3.
Miyoshi Y, Hosokawa K, Kurita S, Oyama S, Ogawa Y, Saito S, et al.
Sci Rep
. 2021 Jul;
11(1):13724.
PMID: 34257336
Pulsating aurorae (PsA) are caused by the intermittent precipitations of magnetospheric electrons (energies of a few keV to a few tens of keV) through wave-particle interactions, thereby depositing most of...
4.
Angelopoulos V, Cruce P, Drozdov A, Grimes E, Hatzigeorgiu N, King D, et al.
Space Sci Rev
. 2019 Mar;
215(1):9.
PMID: 30880847
Electronic Supplementary Material: The online version of this article (10.1007/s11214-018-0576-4) contains supplementary material, which is available to authorized users.
5.
Kasahara S, Miyoshi Y, Yokota S, Mitani T, Kasahara Y, Matsuda S, et al.
Nature
. 2018 Feb;
554(7692):337-340.
PMID: 29446380
Auroral substorms, dynamic phenomena that occur in the upper atmosphere at night, are caused by global reconfiguration of the magnetosphere, which releases stored solar wind energy. These storms are characterized...