In Situ Signature of Cyclotron Resonant Heating in the Solar Wind

The dissipation of magnetized turbulence is an important paradigm for describing heating and energy transfer in astrophysical environments such as the solar corona and wind; however, the specific collisionless processes behind dissipation and heating remain relatively unconstrained by measurements....

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Veröffentlicht in:	Physical review letters 2022-10, Vol.129 (16), p.165101-165101, Article 165101
Hauptverfasser:	Bowen, Trevor A, Chandran, Benjamin D G, Squire, Jonathan, Bale, Stuart D, Duan, Die, Klein, Kristopher G, Larson, Davin, Mallet, Alfred, McManus, Michael D, Meyrand, Romain, Verniero, Jaye L, Woodham, Lloyd D
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext
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