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Generation and Evolution of Fluctuations in a Non-equilibrium Solar Wind Plasma

Subject Area Astrophysics and Astronomy
Term from 2016 to 2021
Project identifier Deutsche Forschungsgemeinschaft (DFG) - Project number 315239725
 
Final Report Year 2021

Final Report Abstract

Natural plasmas from heliosphere, e.g., the expanding solar wind and planetary magnetospheres, are plasmas out of thermal equilibrium. This is unequivocally proved by the in-situ observations, which reveal not only non-Maxwellian velocity distributions of plasma particles, e.g., kinetic anisotropies and suprathermal, Kappa-distributed populations, but also a multi-scale spectra of wave turbulence and fluctuations. The project has proved a strong inter-connection between these two components, by advanced investigations of the kinetic (low-scale) instability mechanisms. On the one hand, anisotropic distributions are important sources of wave instabilities and low-scale fluctuations. It was shown that temperature anisotropy instabilities are markedly enhanced by the suprathermal populations. On the other hand, the low-scale plasma waves can interact resonantly with electrons and protons in the solar wind, triggering their departures from thermal equilibrium and explaining an enhanced presence of suprathermal halo populations with increasing the heliocentric distance.

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