TY - GEN
T1 - Turbulent Alfvén wave driven coronal loops
AU - O'Neill, I. J.
AU - Li, X.
N1 - Copyright:
Copyright 2011 Elsevier B.V., All rights reserved.
PY - 2004
Y1 - 2004
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=22144431589&partnerID=8YFLogxK
M3 - Conference Proceeding (Non-Journal item)
AN - SCOPUS:22144431589
T3 - European Space Agency, (Special Publication) ESA SP
SP - 426
EP - 430
BT - SOHO 15 Workshop: Coronal Heating
T2 - SOHO 15 Workshop: Coronal Heating
Y2 - 6 September 2004 through 9 September 2004
ER -