Other
Scientific paper
Sep 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..249e&link_type=abstract
SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 249-2
Other
Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind
Scientific paper
Constraints on coronal plasma parameters derived from remote and in situ observations are reviewed. The coronal observations include measurements of polarized white light and the widths and intensities of spectral lines. Emphasis is placed on electron temperatures derived from these measurements. In situ observations include mass flux, velocity and ion composition. Some of these observational results are in contradiction to each other. It is discussed how these contradictions could be overcome and what it means for the physical properties of the coronal plasma. The observations will are placed in context with different theoretical models of ion formation and solar wind expansion. Emphasis is placed on the fast solar wind originating in the polar coronal holes.
Chen Yao
Edgar Richard
Esser Ruth
Lie-Svendsen Øystein
No associations
LandOfFree
Observational and theoretical constraints on the heating and acceleration of the fast solar wind does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Observational and theoretical constraints on the heating and acceleration of the fast solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational and theoretical constraints on the heating and acceleration of the fast solar wind will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1148888