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Projekt Druckansicht

Anregung und Entwicklung von Fluktuationen im Nichtgleichgewichts-Sonnenwindplasma

Fachliche Zuordnung Astrophysik und Astronomie
Förderung Förderung von 2016 bis 2021
Projektkennung Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 315239725
 
Erstellungsjahr 2021

Zusammenfassung der Projektergebnisse

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.

Projektbezogene Publikationen (Auswahl)

 
 

Zusatzinformationen

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