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Title: Surface Alfven Wave Reflection as the Slow Wind Formation Mechanism in the Alfven Wave Driven Solar Atmosphere Model
The heating near the coronal hole boundary is included into the AWSoM model via the Alfven wave interaction with the boundary between the closed and open field lines. Although the excessive heating on the Alfven surface wave is possible (Evans et al 2012), we chose to parameterize the surface effect in terms of excessive nonlinear reflection proportional to the transverse gradient of density. The efficiency of such reflection is derived analytically and compared with the solar wind observation data at 1 AU.  more » « less
Award ID(s):
1836821
PAR ID:
10220235
Author(s) / Creator(s):
; ; ; ;
Date Published:
Journal Name:
2020 Fall AGU Meeting
Issue:
Paper SH032-07
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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