Turbulent Alfvén wave driven coronal loops

Authors Organisations
Type Conference Proceeding (Non-Journal item)
Original languageEnglish
Title of host publicationSOHO 15 Workshop: Coronal Heating
Pages426-430
Number of pages5
Edition575
Publication statusPublished - 2004
EventSOHO 15 Workshop: Coronal Heating - , United Kingdom of Great Britain and Northern Ireland
Duration: 06 Sep 200409 Sep 2004

Publication series

NameEuropean Space Agency, (Special Publication) ESA SP
ISSN (Print)0379-6566

Conference

ConferenceSOHO 15 Workshop: Coronal Heating
CountryUnited Kingdom of Great Britain and Northern Ireland
Period06 Sep 200409 Sep 2004
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Abstract

Results from continued work with our unique 1D, two-fluid coronal loop model are presented. A range of loop lengths have been tested with a range of heating profiles. Plasma flow is driven by turbulent Alfvén waves. We can produce cool, EUV and X-ray loops and can produce stable isothermal solutions. We can also simulate strong footpoint heating producing footpoint temperatures in excess of 1MK. This finding leads us to the study of EUV 'moss' and appears to be symptomatic of rapid wave energy release.