MHD Wave Heating Diagnostics

Authors Organisations
Type Conference Proceeding (Non-Journal item)
Original languageEnglish
Title of host publicationMagnetic Coupling between the Interior and Atmosphere of the Sun
Pages287-288
ISBN (Electronic)978-3-642-02859-5
DOI
Publication statusPublished - 2010

Publication series

NameAstrophysics and Space Science Proceedings
PublisherSpringer
ISSN (Print)1570-6591
ISSN (Electronic)1570-6605
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Abstract

Analyzing the structure of solar coronal loops is crucial to our understanding of the processes that heat and maintain the coronal plasma at multimillion degree temperatures. The determination of the physical parameters of coronal loops remains both an observational and theoretical challenge. A novel diagnostic technique for quiescent coronal loops based on the analysis of power spectra of Doppler-shift time series is developed and proposed to test on real data.