XMAGNET: Velocity structure functions of active galactic nucleus-driven turbulence in the multiphase intracluster medium

Open Access

Fig. 9.

Relationship between the power-law index $m_{cold}^{us}$ $m_{\mathrm{cold}}^{\mathrm{us}}$ of the unsmoothed (“us”) projected VSFs (horizontal axis) and Δm, which represents the increase in the power-law index resulting from smoothing. Lines of equal power-law index for smoothed VSFs ( $m_{cold}^{s}$ $m_{\mathrm{cold}}^{\mathrm{s}}$ ) are also indicated for comparison (gray lines).

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