Electron energy transport in the solar wind: Ulysses observations

Details Electron energy transport in the solar wind: Ulysses observations Electron energy transport in the solar wind: Ulysses observations

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..210s&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 210

Computer Science

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind, Waves, Oscillations, And Instabilities In Plasmas And Intense Beams

Scientific paper

Previous analysis suggests that the whistler heat flux instability is responsible for the regulation of the electron heat flux of the solar wind. For an interval of quiescent solar wind during the in-ecliptic phase of the Ulysses mission, the plasma wave data in the whistler frequency regime are compared to the predictions of the whistler heat flux instability model. The data is well constrained by the predicted upper bound on the electron heat flux and a clear correlation between wave activity and electron heat flux dissipation is observed.

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