The polar coronal holes and the fast solar wind: Some recent results

Details The polar coronal holes and the fast solar wind: Some recent results The polar coronal holes and the fast solar wind: Some recent results

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..598..299p&link_type=abstract

SOLAR AND GALACTIC COMPOSITION: A Joint SOHO/ACE Workshop. AIP Conference Proceedings, Volume 598, pp. 299-304 (2001).

Computer Science

Particle Emission, Solar Wind, Composition

Scientific paper

We report on recent results on the source regions of the fast solar wind: the Polar Coronal Holes (PCH). They concern a comparison between the effective temperatures for a large set of different ions obtained from observations in the inner corona of PCH and from a fast wind numerical model based on the ion-cyclotron resonant dissipation of high-frequency Alfvén waves. We also report on some preliminary results from our modeling concerning the Fe/O ratio in the inner corona in PCH. .

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