Application of statistical analysis techniques to solar and stellar phenomena
Currently, solar observers are investigating spectroscopic images of the Sun's outermost atmosphere (the corona), which are challenging long-held views on the density and temperature structure of this environment. The corona is "filled" with magnetic strands but determining their prec...
Main Author: | |
---|---|
Published: |
University of Central Lancashire
2009
|
Subjects: | |
Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.733478 |