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Characteristics of solar wind suprathermal halo electrons
DOI: 10.1051/0004-6361/202038830 Bibcode: 2020A&A...642A.130L

Fichtner, H.; Pierrard, V.; Lazar, M. +1 more

A suprathermal halo population of electrons is ubiquitous in space plasmas, as evidence of their departure from thermal equilibrium even in the absence of anisotropies. The origin, properties, and implications of this population, however, are poorly known. We provide a comprehensive description of solar wind halo electrons in the ecliptic, contras…

2020 Astronomy and Astrophysics
Ulysses Cluster 18
Statistics of solar wind electron breakpoint energies using machine learning techniques
DOI: 10.1051/0004-6361/202037840 Bibcode: 2020A&A...639A..46B

Walsh, A. P.; Rae, I. J.; Smith, A. W. +4 more

Solar wind electron velocity distributions at 1 au consist of a thermal "core" population and two suprathermal populations: "halo" and "strahl". The core and halo are quasi-isotropic, whereas the strahl typically travels radially outwards along the parallel or anti-parallel direction with respect to the interplanetary magnetic field. Using Cluster…

2020 Astronomy and Astrophysics
Cluster 8