@article{915798,
      recid = {915798},
      author = {Montagud-Camps, Victor,},
      title = {Turbulent heating and anisotropy in the solar wind : a  numerical study /},
      pages = {1 online resource (xvii, 123 pages) :},
      note = {"Doctoral thesis accepted by Paris-Sud University, Orsay,  France."},
      abstract = {This book presents two important new findings. First, it  demonstrates from first principles that turbulent heating  offers an explanation for the non-adiabatic decay of proton  temperature in solar wind. Until now, this was only proved  with reduced or phenomenological models. Second, the book  demonstrates that the two types of anisotropy of turbulent  fluctuations that are observed in solar wind at 1AU  originate not only from two distinct classes of conditions  near the Sun but also from the imbalance in Alfvén wave  populations. These anisotropies do not affect the overall  turbulent heating if we take into account the relation  observed in solar wind between anisotropy and Alfvén wave  imbalance. In terms of the methods used to obtain these  achievements, the author shows the need to find a very  delicate balance between turbulent decay and expansion  losses, so as to directly solve the magnetohydrodynamic  equations, including the wind expansion effects.},
      url = {http://library.usi.edu/record/915798},
      doi = {https://doi.org/10.1007/978-3-030-30383-9,  https://doi.org/10.1007/978-3-030-30},
}