# Dissipative invariants in MHD turbulence

## TL;DR

This paper investigates the role of dissipative invariants in isotropic homogeneous MHD turbulence using distributed chaos and DNS, also discussing effects of magnetic fields in solar contexts.

## Contribution

It introduces a novel analysis of dissipative invariants in MHD turbulence through distributed chaos and numerical simulations, with implications for solar magnetic fields.

## Key findings

- Dissipative invariants influence turbulence dynamics.
- Weak magnetic fields modify turbulence behavior.
- Results applicable to solar magnetic phenomena.

## Abstract

Role of the dissipative invariants in isotropic homogeneous MHD turbulence has been studied using the distributed chaos approach and results of direct numerical simulations. Effects of weak imposed mean magnetic field and magnetic fields in undisturbed solar photosphere are also briefly discussed in this context.