Nature of Stochastic Ion Heating in the Solar Wind: Testing the Dependence on Plasma Beta and Turbulence Amplitude
The solar wind undergoes significant heating as it propagates away from the Sun; the exact mechanisms responsible for this heating are not yet fully understood. We present for the first time a statistical test for one of the proposed mechanisms: stochastic ion heating. We use the amplitude of magnet...
Main Authors: | , , |
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Language: | en |
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IOP PUBLISHING LTD
2017
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Online Access: | http://hdl.handle.net/10150/626264 http://arizona.openrepository.com/arizona/handle/10150/626264 |