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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
RADIAL EVOLUTION OF A MAGNETIC CLOUD: MESSENGER , STEREO , AND VENUS EXPRESS OBSERVATIONS
The Solar Orbiter and Solar Probe Plus missions will provide observations of magnetic clouds closer to the Sun than ever before, and it will be good preparation for these missions to make full use of the most recent in situ data sets from the inner heliosphere\textemdashnamely, those provided by MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) and Venus Express\textemdashfor magnetic cloud studies. We present observations of the same magnetic cloud made by MESSENGER at Mercury and later by Solar T ...
Good, S.; Forsyth, R.; Raines, J.; Gershman, D.; Slavin, J.; Zurbuchen, T.;
Published by: The Astrophysical Journal Published on: 07/2015
YEAR: 2015   DOI: 10.1088/0004-637X/807/2/177
magnetic fields; parker solar probe; Solar Probe Plus; Solar wind; Sun: coronal mass ejections: CMEs; Sun: heliosphere