Physics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005spie.5901...67d&link_type=abstract
Solar Physics and Space Weather Instrumentation. Edited by Fineschi, Silvano; Viereck, Rodney A. Proceedings of the SPIE, Volume
Physics
1
Scientific paper
The measurements of velocity and temperature of coronal electrons are of immense importance to the study of coronal dynamics, especially in the low solar corona. In this lies interesting physics yet to fully explain the theoretical reasoning for the million degree hot coronal plasma and the cause for the initial acceleration of this coronal plasma. In this regard it would be equally important if both of these coronal electron parameters, namely the velocity and the temperature of these coronal electrons, could be determined simultaneously and globally all around the low solar corona. The purpose of this paper is twin fold. First, to lay out an instrumental procedure that allows for the measurement of a coronal signature that could measure all around the low solar corona simultaneously. Second, to describe a theoretical procedure that allows for deriving both the coronal electron temperature and its bulk flow velocity from the measured coronal signature.
Cyr Orville Chris St.
Davila Joseph M.
Reginald Nelson Leslie
No associations
LandOfFree
Coronal electron velocity and temperature from Thomson scattered visible light 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 Coronal electron velocity and temperature from Thomson scattered visible light, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Coronal electron velocity and temperature from Thomson scattered visible light will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-801663