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Correction to: Solar Phys (2019) 294:34https://doi.org/10.1007/s11207-019-1421-yThis article was published with an omission in the Acknowledgement text. Please find in this document the correct Acknowledgement text that should be regarded as the final version by the reader.Acknowledgement The work by S. Perri has been supported by the Agenzia Spaziale Italiana under the contract ASI-INAF 2015-039-R...
The propagation of energetic particles in the solar wind depends in a sensitive way on the pitch-angle scattering of particles in the presence of magnetic turbulence. The well-known quasi-linear theory gives an expression for the pitch-angle scattering rate under the assumption of small turbulence levels, but both in the solar wind and in other astrophysical environments the turbulent magnetic field...
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