scholarly journals Self‐consistent Coronal Heating and Solar Wind Acceleration from Anisotropic Magnetohydrodynamic Turbulence

2007 ◽  
Vol 171 (2) ◽  
pp. 520-551 ◽  
Author(s):  
Steven R. Cranmer ◽  
Adriaan A. van Ballegooijen ◽  
Richard J. Edgar
Keyword(s):  
Solar Wind ◽  
Coronal Heating ◽  
Magnetohydrodynamic Turbulence ◽  
Solar Wind Acceleration ◽  
Self Consistent

scholarly journals Understanding coronal heating and solar wind acceleration: Case for in situ near-Sun measurements

2007 ◽  
Vol 45 (1) ◽  
Author(s):  
D. J. McComas ◽  
M. Velli ◽  
W. S. Lewis ◽  
L. W. Acton ◽  
M. Balat-Pichelin ◽  
...  
Keyword(s):  
Solar Wind ◽  
Coronal Heating ◽  
Solar Wind Acceleration

Integrating physics-based coronal heating and solar wind acceleration in a global MHD model

2013 ◽  
Author(s):  
Roberto Lionello ◽  
Marco Velli ◽  
Jon A. Linker ◽  
Zoran Mikić
Keyword(s):  
Solar Wind ◽  
Coronal Heating ◽  
Solar Wind Acceleration ◽  
Mhd Model

MULTI-SHELL MAGNETIC TWISTERS AS A NEW MECHANISM FOR CORONAL HEATING AND SOLAR WIND ACCELERATION

2015 ◽  
Vol 808 (1) ◽  
pp. 5 ◽  
Author(s):  
K. Murawski ◽  
A. K. Srivastava ◽  
Z. E. Musielak ◽  
B. N. Dwivedi
Keyword(s):  
Solar Wind ◽  
Coronal Heating ◽  
Solar Wind Acceleration

scholarly journals Coronal Heating and the Solar Wind Acceleration

2001 ◽  
Vol 203 ◽  
pp. 495-497 ◽  
Author(s):  
T. Hirayama
Keyword(s):  
Solar Wind ◽  
Electric Field ◽  
Dissipation Rate ◽  
Electron Beams ◽  
Coronal Heating ◽  
Thermal Electron ◽  
Charge Imbalance ◽  
Solar Wind Acceleration

We propose a coronal heating theory based on the magnetic twisting, which inevitably produces charge imbalance. The resulting electric field creates supra-thermal electron beams. Beams are then thermalized by classical collisions. The dissipation rate is enough to heat the corona and to accelerate the solar wind.

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