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Constraining Solar Wind Heating Processes by Kinetic Properties of Heavy Ions
We analyze the heavy ion components (A \>4 amu ) in collisionally young solar wind plasma and show that there is a clear, stable dependence of temperature on mass, probably reflecting the conditions in the solar corona. We consider both linear and power law forms for the dependence and find that a simple linear fit of the form Ti/Tp=(1.35 \textpm.02 )mi/mp describes the observations twice as well as the equivalent best fit power law of the form Ti/Tp=(m< ...
Tracy, Patrick; Kasper, Justin; Raines, Jim; Shearer, Paul; Gilbert, Jason; Zurbuchen, Thomas;
Published by: Physical Review Letters Published on: 06/2016
YEAR: 2016   DOI: 10.1103/PhysRevLett.116.255101