Abstract
We find again, as in VG16 (Verdini and Grappin 2016), two final stable attractors: the GYRO and the R-SLAB. We find, however, some discrepancies with respect to the results obtained in VG16 that we explain in detail here.
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Montagud-Camps, V. (2019). Discussion. In: Turbulent Heating and Anisotropy in the Solar Wind. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-030-30383-9_8
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DOI: https://doi.org/10.1007/978-3-030-30383-9_8
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