Turbulent Alfvén wave driven coronal loops
Authors
Organisations
| Type | Conference Proceeding (Non-Journal item) |
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| Original language | English |
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| Title of host publication | SOHO 15 Workshop: Coronal Heating |
| Pages | 426-430 |
| Number of pages | 5 |
| Edition | 575 |
| Publication status | Published - 2004 |
| Event | SOHO 15 Workshop: Coronal Heating - , United Kingdom of Great Britain and Northern Ireland Duration: 06 Sep 2004 → 09 Sep 2004 |
Publication series
| Name | European Space Agency, (Special Publication) ESA SP |
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| ISSN (Print) | 0379-6566 |
Conference
| Conference | SOHO 15 Workshop: Coronal Heating |
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| Country | United Kingdom of Great Britain and Northern Ireland |
| Period | 06 Sep 2004 → 09 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.