Characteristics of Resonant Electrons Interacting With Whistler Waves in the Nearest Dipolarizing Magnetotail

The Magnetospheric Multiscale spacecraft observations in the burst mode allow the determination of the characteristics of resonant electrons interacting with quasi‐parallel whistler waves during prolonged dipolarizations in the near Earth magnetotail at −22 RE

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Bibliographische Detailangaben
Veröffentlicht in:	Journal of geophysical research. Space physics 2021-07, Vol.126 (7), p.n/a, Article 2021
Hauptverfasser:	Malykhin, A. Y., Grigorenko, E. E., Shklyar, D. R., Panov, E. V., Le Contel, O., Avanov, L., Giles, B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Anisotropy Astronomy & Astrophysics Astrophysics Bursts Collisionless plasmas Configurations Cyclotrons dipolarizations Dipoles Earth and Planetary Astrophysics Electron distribution Electron precipitation Electrons Energy Energy dissipation Energy distribution Energy transfer Geomagnetic tail Gyrofrequency Heat exchange Kinetic energy Magnetic fields Magnetospheres magnetotail Magnetotails Particle interactions Physical Sciences Physics Pitch (inclination) Plasma heating plasma sheet Plasma waves Science & Technology Spacecraft Time Transformations Wave energy Wave power Wave propagation wave‐particle interactions Whistler waves Whistlers
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Beschreibung
Zusammenfassung:	The Magnetospheric Multiscale spacecraft observations in the burst mode allow the determination of the characteristics of resonant electrons interacting with quasi‐parallel whistler waves during prolonged dipolarizations in the near Earth magnetotail at −22 RE
ISSN:	2169-9380 2169-9402
DOI:	10.1029/2021JA029440