Effects of the background turbulence on the relaxation of ion temperature anisotropy in space plasmas
Author
dc.contributor.author
Moya Fuentes, Pablo
Author
dc.contributor.author
Navarro, Roberto E.
Admission date
dc.date.accessioned
2021-09-21T15:00:12Z
Available date
dc.date.available
2021-09-21T15:00:12Z
Publication date
dc.date.issued
2021
Cita de ítem
dc.identifier.citation
Frontiers in Physics April 2021 Volume 9 Article 624748
es_ES
Identifier
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10.3389/fphy.2021.624748
Identifier
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https://repositorio.uchile.cl/handle/2250/182022
Abstract
dc.description.abstract
Turbulence in space plasmas usually exhibits two regimes separated by a spectral break that divides the so called inertial and kinetic ranges. Large scale magnetic fluctuations are dominated by non-linear MHD wave-wave interactions following a -5/3 or -2 slope power-law spectrum. After the break, at scales in which kinetic effects take place, the magnetic spectrum follows a steeper power-law k(-alpha) shape given by a spectral index alpha > 5/3. Despite its ubiquitousness, the possible effects of a turbulent background spectrum in the quasilinear relaxation of solar wind temperatures are usually not considered. In this work, a quasilinear kinetic theory is used to study the evolution of the proton temperatures in an initially turbulent collisionless plasma composed by cold electrons and bi-Maxwellian protons, in which electromagnetic waves propagate along a background magnetic field. Four wave spectrum shapes are compared with different levels of wave intensity. We show that a sufficient turbulent magnetic power can drive stable protons to transverse heating, resulting in an increase in the temperature anisotropy and the reduction of the parallel proton beta. Thus, stable proton velocity distribution can evolve in such a way as to develop kinetic instabilities. This may explain why the constituents of the solar wind can be observed far from thermodynamic equilibrium and near the instability thresholds.
es_ES
Patrocinador
dc.description.sponsorship
ANID, Chile, through FONDECyT 11180947
1191351
CONICyT-PAI 79170095