Figure 4 from Nature of Stochastic Ion Heating in the Solar Wind: Testing the Dependence on Plasma Beta and Turbulence Amplitude

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Nature of Stochastic Ion Heating in the Solar Wind: Testing the Dependence on Plasma Beta and Turbulence Amplitude

Authors: Daniel Vech, Kristopher G. Klein, and Justin C. Kasper

2017 The Astrophysical Journal Letters 850 L11.

Provider: AAS Journals

Caption: Figure 4.

Cross sections of the binned T_p data in the (﹩{\epsilon }_{p},{V}_{\mathrm{SW}}﹩) space along three solar wind speed intervals. Each T_p line was normalized to its peak value.

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