Thermal conductivity with bells and whistlers: Suppression of the magnetothermal instability in galaxy clusters

Open Access

Fig. 8.

Marginal distributions of the 3D runs with respect to the modified plasma $\tilde{β}$ $\tilde{\beta}$ (top), the isothermality parameter σ (bottom left), and the effective thermal diffusivity χ/χ₀ (bottom right). Stronger whistler suppression decreases the overall magnetic energy levels and brings part of the domain out of isothermality.

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