https://orcid.org/0000-0003-2579-7266
errata, addenda, acceleration of particles, accretion, accretion discs, MHD, plasmas, turbulence, cosmic rays
This is an erratum to the paper ‘Acceleration and escape processes of high-energy particles in turbulence inside hot accretion flows’ (DOI: https://doi.org/10.1093/mnras/stz329), which was published in MNRAS, 485, 163–178 (2019). In Fig. 4, we mistakenly plotted the quantities using the wrong axes, causing the spiral shape inconsistent with that in fig. 6. The correct plots are shown here. The other results are unaffected, and the conclusions remain unchanged.
Figure 4.
Colormaps in the equatorial plane for run A. The upper and lower panels show the density and the magnetic energy density, respectively.
ACKNOWLEDGEMENTS
We thank Takeru K. Suzuki for pointing out the mistake.
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
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