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Electron energy transport in the solar wind: Ulysses observationsThe electron heat flux in the solar wind has been measured by the Ulysses solar wind plasma experiment in the ecliptic from 1 to 5 AU and out of the ecliptic during the recently completed pass over the solar south pole and the ongoing pass over the solar north pole. Although the electron heat flux contains only a fraction of the kinetic energy of the solar wind. the available energy is sufficient to account for the non-adiabatic expansion of the solar wind electrons. The Ulysses measurements indicate that the electron heat flux is actively dissipated in the solar wind. The exact mechanism or mechanisms is unknown. but a model based on the whistler heat flux instability predicts radial gradients for the electron heat flux in good agreement with the data. We will present measurements of the correlation between wave activity measured by the unified radio and plasma experiment (URAP) and the electron heat flux throughout the Ulysses mission. The goal is to determine if whistler waves are a good candidate for the observed electron heat flux dissipation. The latitudinal gradients of the electron heat flux. wave activity. and electron pressure will be discussed in light of the changes in the magnetic field geometry from equator to poles.
Document ID
19960021284
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Scime, Earl
(West Virginia Univ. Morgantown, VA United States)
Gary, S. Peter
(Los Alamos National Lab. NM United States)
Phillips, J. L.
(Los Alamos National Lab. NM United States)
Corniileau-Wehrlin, N.
(Centre des Etudes Terrestraire et Planetaire Velizy, France)
Solomon, J.
(Centre des Etudes Terrestraire et Planetaire Velizy, France)
Date Acquired
August 17, 2013
Publication Date
June 30, 1995
Subject Category
Solar Physics
Accession Number
96N24680
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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