Ion pitch-angle scattering by Alfvén waves

1997 ◽  
Vol 4 (11) ◽  
pp. 4103-4117 ◽  
Author(s):  
Y. Li ◽  
Peter H. Yoon ◽  
C. S. Wu ◽  
A. T. Weatherwax ◽  
J. K. Chao ◽  
...  
Keyword(s):  
Pitch Angle ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Angle Scattering

scholarly journals On heating of solar wind protons by the breaking of large amplitude Alfvén waves

2018 ◽  
Author(s):  
Horia Comişel ◽  
Yasuhiro Nariyuki ◽  
Yasuhito Narita ◽  
Uwe Motschmann
Keyword(s):  
Solar Wind ◽  
Pitch Angle ◽  
Plasma Heating ◽  
Alfven Waves ◽  
Distribution Functions ◽  
Alfven Wave ◽  
Alfvén Waves ◽  
Parametric Decay ◽  
Angle Scattering ◽  
Velocity Distribution Functions

Abstract. By means of hybrid simulations, we present a study on plasma heating by the field-aligned parametric decay of a monochromatic left-handed polarized Alfven wave. Simultaneous multidimensional comparisons of the wave modes and proton kinetics suggest that parametric decay of Alfven waves and pitch angle scattering of solar wind protons are interrelated. Parametric decay mechanism yields counter-propagating Alfven waves that can shape and broaden via pitch angle scattering mechanism both the sunward and antisunward sides of the proton velocity distribution functions in agreement with in situ measurements of fast stream solar wind plasmas.

scholarly journals Relativistic Alfvén Waves on the jet of BL Lacertae

2014 ◽  
Vol 10 (S313) ◽  
pp. 147-152
Author(s):  
Marshall H. Cohen ◽  
David L. Meier
Keyword(s):  
Magnetic Field ◽  
Pitch Angle ◽  
Lorentz Factor ◽  
Alfven Waves ◽  
Longitudinal Component ◽  
Mhd Waves ◽  
Alfvén Waves ◽  
Bl Lacertae ◽  
Pattern Speeds ◽  
Helical Magnetic Field

AbstractThe jet of BL Lac displays transverse patterns that propagate downstream superluminally. We suggest that they are transverse Alfvén waves propagating on the longitudinal component of a helical magnetic field. The speed of the wave adds relativistically to the speed of the beam, and the apparent speed of the pattern is greater than the beam speed. Models for the jet and the MHD waves give values for the Lorentz factor of the beam of 3–4.4 and pitch angle of the helical magnetic field of 43° - 65°. These are consistent with other estimates, if the beam and pattern speeds are allowed to differ.

Nongyroresonant Pitch Angle Scattering

1999 ◽  
Vol 518 (2) ◽  
pp. 974-984 ◽  
Author(s):  
B. R. Ragot
Keyword(s):  
Pitch Angle ◽  
Angle Scattering

scholarly journals On the origin of solar wind. Alfvén waves induced jump of coronal temperature

2007 ◽  
Vol 44 (3) ◽  
pp. 533-536 ◽  
Author(s):  
T. M. Mishonov ◽  
M. V. Stoev ◽  
Y. G. Maneva
Keyword(s):  
Solar Wind ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Coronal Temperature

AMPTE/CCE observations of substorm-associated standing Alfvén waves in the midnight sector

1988 ◽  
Vol 15 (11) ◽  
pp. 1287-1290 ◽  
Author(s):  
K. Takahashi ◽  
S. Kokubun ◽  
T. Sakurai ◽  
R. W. McEntire ◽  
T. A. Potemra ◽  
...  
Keyword(s):  
Alfven Waves ◽  
Alfvén Waves

Dynamics of nonlinear Alfvén waves in the shallow water magnetohydrodynamic equations

2019 ◽  
Vol 4 (5) ◽  
Author(s):  
Martin Magill ◽  
Aaron Coutino ◽  
Benjamin A. Storer ◽  
Marek Stastna ◽  
Francis J. Poulin
Keyword(s):  
Shallow Water ◽  
Alfven Waves ◽  
Alfvén Waves ◽  
Magnetohydrodynamic Equations
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