# Solar wind collisional heating

**Authors:** O. Pezzi

arXiv: 1704.08020 · 2017-08-02

## TL;DR

This paper investigates how collisions affect heating in the solar wind by comparing nonlinear and linearized Landau operators, revealing that nonlinearities accelerate dissipation of velocity space structures.

## Contribution

It extends previous work by directly comparing nonlinear and linearized Landau operators, emphasizing the importance of nonlinearities in accurately modeling collisional effects.

## Key findings

- Nonlinear Landau operator leads to faster dissipation of velocity structures.
- Linearized operator overestimates characteristic relaxation times.
- Retaining nonlinearities is crucial for accurate collisional heating modeling.

## Abstract

To properly describe heating in weakly collisional turbulent plasmas such as the solar wind, inter-particle collisions should be taken into account. Collisions can convert ordered energy into heat by means of irreversible relaxation towards the thermal equilibrium. Recently, Pezzi et al. (Phys. Rev. Lett., vol. 116, 2016, p. 145001) showed that the plasma collisionality is enhanced by the presence of fine structures in velocity space. Here, the analysis is extended by directly comparing the effects of the fully nonlinear Landau operator and a linearized Landau operator. By focusing on the relaxation towards the equilibrium of an out of equilibrium distribution function in a homogeneous force-free plasma, here it is pointed out that it is significant to retain nonlinearities in the collisional operator to quantify the importance of collisional effects. Although the presence of several characteristic times associated with the dissipation of different phase space structures is recovered in both the cases of the nonlinear and the linearized operators, the influence of these times is different in the two cases. In the linearized operator case, the recovered characteristic times are systematically larger than in the fully nonlinear operator case, this suggesting that fine velocity structures are dissipated slower if nonlinearities are neglected in the collisional operator.

## Full text

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## Figures

10 figures with captions in the complete paper: https://tomesphere.com/paper/1704.08020/full.md

## References

87 references — full list in the complete paper: https://tomesphere.com/paper/1704.08020/full.md

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Source: https://tomesphere.com/paper/1704.08020