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Mediation of collisionless turbulent dissipation through cyclotron resonance - Nature Astronomy

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Mediation of collisionless turbulent dissipation through cyclotron resonance - Nature Astronomy

The dissipation of turbulence in astrophysical systems is fundamental to energy transfer and heating in environments ranging from the solar wind and corona to accretion disks and the intracluster medium. Although turbulent dissipation is relatively well understood in fluid dynamics, astrophysical plasmas often exhibit exotic behaviour, arising from the lack of interparticle collisions, which complicates turbulent dissipation and heating in these systems.

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Mediation of collisionless turbulent dissipation through cyclotron resonance - Nature Astronomy

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Mediation of collisionless turbulent dissipation through cyclotron resonance - Nature Astronomy

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