Dense coronal plasma is confined in magnetic loops, the building blocks of the bright X-ray corona. We overview recent findings from the analysis of confined coronal plasma observed with SoHO and TRACE and its interpretation. Internal substructuring, mass transport and dynamics, and heating processes are discussed.
REALE F (2005). Sub-Structuring Dynamics and Heating in Dense Coronal Structures. In ESA, Editors: D. Danesy, S. Poedts, A. De Groof and J. Andries (pp.27.1-27.7).
Sub-Structuring Dynamics and Heating in Dense Coronal Structures
REALE, Fabio
2005-01-01
Abstract
Dense coronal plasma is confined in magnetic loops, the building blocks of the bright X-ray corona. We overview recent findings from the analysis of confined coronal plasma observed with SoHO and TRACE and its interpretation. Internal substructuring, mass transport and dynamics, and heating processes are discussed.
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