Alfvénic turbulence driven temperature anisotropies of thermal non-equilibrium ions

Kasper et al. have found that solar-wind helium could be heated to be nearly 7 times hotter than hydrogen on average from the observation of the Wind spacecraft. The stochastic Fermi mechanism is employed to investigate this phenomenon via the ion-cyclotron resonant process (Kasper J. C. et al., Phy...

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Published in:Europhysics letters Vol. 123; no. 6; pp. 65004 - 65010
Main Authors: Liu, Hai-Feng, Yang, Lang, Tang, Chang-Jian, Luo, Yang, Zhang, Xin, Xu, Yu-Hong
Format: Journal Article
Language:English
Published: Les Ulis EDP Sciences, IOP Publishing and Società Italiana di Fisica 01-09-2018
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Abstract Kasper et al. have found that solar-wind helium could be heated to be nearly 7 times hotter than hydrogen on average from the observation of the Wind spacecraft. The stochastic Fermi mechanism is employed to investigate this phenomenon via the ion-cyclotron resonant process (Kasper J. C. et al., Phys. Rev. Lett., 110 (2013) 091102). Due to strong ion cyclotron resonances caused by counterpropagating Alfvén waves, the helium could be thermalized to be 7 times hotter than hydrogen. In this paper, a new aspect, the non-resonant interaction between thermal non-equilibrium particles and turbulent Alfvén waves, is utilized to illustrate the above observation analytically and numerically. The result of our model is broadly consistent with the observational result. Additionally, this paper predicts that the various temperature anisotropies of ions may exist in the solar-wind core which different thermal non-equilibrium factors lead to. This work builds up a close relation among non-resonant heating of thermal non-equilibrium ions, differential flow, and temperature anisotropy.
AbstractList Kasper et al. have found that solar-wind helium could be heated to be nearly 7 times hotter than hydrogen on average from the observation of the Wind spacecraft. The stochastic Fermi mechanism is employed to investigate this phenomenon via the ion-cyclotron resonant process (Kasper J. C. et al., Phys. Rev. Lett., 110 (2013) 091102). Due to strong ion cyclotron resonances caused by counterpropagating Alfvén waves, the helium could be thermalized to be 7 times hotter than hydrogen. In this paper, a new aspect, the non-resonant interaction between thermal non-equilibrium particles and turbulent Alfvén waves, is utilized to illustrate the above observation analytically and numerically. The result of our model is broadly consistent with the observational result. Additionally, this paper predicts that the various temperature anisotropies of ions may exist in the solar-wind core which different thermal non-equilibrium factors lead to. This work builds up a close relation among non-resonant heating of thermal non-equilibrium ions, differential flow, and temperature anisotropy.
Author Zhang, Xin
Luo, Yang
Xu, Yu-Hong
Yang, Lang
Tang, Chang-Jian
Liu, Hai-Feng
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  surname: Xu
  fullname: Xu, Yu-Hong
  organization: Southwest Jiaotong University Chengdu Institute of Fusion Science, School of Physical Science and Technology, 610041, China
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Snippet Kasper et al. have found that solar-wind helium could be heated to be nearly 7 times hotter than hydrogen on average from the observation of the Wind...
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SubjectTerms 52.35.Bj
52.35.Mw
Anisotropy
Cyclotron resonance
Equilibrium
Helium
Hydrogen
Magnetohydrodynamic waves
Resonant interactions
Solar wind
Turbulence
Wind spacecraft
Title Alfvénic turbulence driven temperature anisotropies of thermal non-equilibrium ions
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