TY - JOUR
T1 - Alfvénic-turbulence-heated magnetic loops
T2 - Effects of lateral expansion and magnetic twist
AU - Li, Bo
AU - Li, Xing
N1 - Copyright:
Copyright 2017 Elsevier B.V., All rights reserved.
PY - 2006/2/15
Y1 - 2006/2/15
N2 - Using a 1.5-dimensional two-fluid magnetic loop model in which loops are heated by Alfvénic turbulence, we explore the effects on the loop parameters of the varying cross-section and the magnetic twist. The introduced magnetic twist is set to be around the kink instability threshold for a curved loop. It is found that: (i) The lateral expansion, which takes place close to footpoints, can significantly influence the heating profile, leading to a significant footpoint plasma flow. When observed on disc, the corresponding footpoint blue/red shift may be found for upper transition region lines, (ii) The effects introduced by magnetic twist are twofold. Firstly, the twist-related force may contribute to the axial force balance. Secondly, the projection effect reduces the electron and proton thermal conductivities. The former is found to be of little significance; however, the latter gives rise to considerable changes compared to the untwisted case.
AB - Using a 1.5-dimensional two-fluid magnetic loop model in which loops are heated by Alfvénic turbulence, we explore the effects on the loop parameters of the varying cross-section and the magnetic twist. The introduced magnetic twist is set to be around the kink instability threshold for a curved loop. It is found that: (i) The lateral expansion, which takes place close to footpoints, can significantly influence the heating profile, leading to a significant footpoint plasma flow. When observed on disc, the corresponding footpoint blue/red shift may be found for upper transition region lines, (ii) The effects introduced by magnetic twist are twofold. Firstly, the twist-related force may contribute to the axial force balance. Secondly, the projection effect reduces the electron and proton thermal conductivities. The former is found to be of little significance; however, the latter gives rise to considerable changes compared to the untwisted case.
KW - Lateral expansion
KW - Magnetic twists
KW - Solar coronal loop
KW - Turbulence heating
UR - http://www.scopus.com/inward/record.url?scp=32644444406&partnerID=8YFLogxK
U2 - 10.1098/rsta.2005.1715
DO - 10.1098/rsta.2005.1715
M3 - Article
AN - SCOPUS:32644444406
SN - 1364-503X
VL - 364
SP - 533
EP - 536
JO - Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
JF - Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
IS - 1839
ER -