The effect of variations in the magnetic field direction from turbulence on kinetic-scale instabilities

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 3.

PDF of data in –Δ^ρ parameter space for (a) oblique fire-hose unstable and (b) mirror-mode unstable data distributions. Panel (c) shows the same PDF for equivalent persistence intervals sampled from the stable data. The vertical lines shown in (a) and (b) denote the breakpoints previously identified by Opie et al. (2022).

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