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 |
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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. |
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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 |
Author_xml | – sequence: 1 givenname: Hai-Feng surname: Liu fullname: Liu, Hai-Feng organization: Sichuan University Physics Department, - Chengdu, 610041, China – sequence: 2 givenname: Lang surname: Yang fullname: Yang, Lang organization: Southwest Jiaotong University Chengdu Institute of Fusion Science, School of Physical Science and Technology, 610041, China – sequence: 3 givenname: Chang-Jian surname: Tang fullname: Tang, Chang-Jian organization: Sichuan University Physics Department, - Chengdu, 610041, China – sequence: 4 givenname: Yang surname: Luo fullname: Luo, Yang organization: Southwest Jiaotong University Chengdu Institute of Fusion Science, School of Physical Science and Technology, 610041, China – sequence: 5 givenname: Xin surname: Zhang fullname: Zhang, Xin organization: Southwest Jiaotong University Chengdu Institute of Fusion Science, School of Physical Science and Technology, 610041, China – sequence: 6 givenname: Yu-Hong 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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