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Stochastic Heating in the Sub-Alfvénic Solar Wind

Trevor A. Bowen ^1,*, Tamar Ervin ^1,2, Alfred Mallet¹, Benjamin D. G. Chandran ³, Nikos Sioulas¹, Philip A. Isenberg³, Stuart D. Bale ^1,2, Jonathan Squire⁴, Kristopher G. Klein⁵ et al.

Oreste Pezzi ⁶

¹Space Sciences Laboratory, University of California, Berkeley, California 94720-7450, USA
²Physics Department, University of California, Berkeley, California 94720-7300, USA
³Department of Physics and Astronomy, University of New Hampshire, Durham, New Hampshire 03824, USA
⁴Department of Physics, University of Otago, 730 Cumberland Street, Dunedin 9016, New Zealand
⁵Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona, USA
⁶Institute for Plasma Science and Technology, National Research Council of Italy, G. Amendola 122/D, Bari, I-70126, Italy

^*Contact author: tbowen@berkeley.edu

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Articles Citing

Stochastic Heating in the Sub-Alfvénic Solar Wind

The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes

Quasi-linear theory of perpendicular ion heating by critically balanced turbulence

Solar Wind Heating near the Sun: A Radial Evolution Approach

Ion Stochastic Heating by Wave-induced Field Line Curvature in Space Plasmas

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