# On the origin of the magnetic energy in the quiet solar chromosphere

## TL;DR

This study uses high-resolution 3D radiative MHD simulations to investigate the origin and evolution of magnetic energy in the quiet solar chromosphere, revealing energy conversion processes and magnetic field saturation levels.

## Contribution

It demonstrates that kinetic energy in the lower chromosphere converts into magnetic energy, which saturates at 4 to 30 G, highlighting the local processes responsible for magnetic energy in the quiet Sun.

## Key findings

- Magnetic flux from the photosphere is insufficient to sustain chromospheric magnetic fields.
- Kinetic energy in the lower chromosphere converts into magnetic energy via shocks.
- Magnetic energy saturates at 4 to 30 G due to energy conversion processes.

## Abstract

The presence of magnetic field is crucial in the transport of energy through the solar atmosphere. Recent ground-based and space-borne observations of the quiet Sun have revealed that magnetic field accumulates at photospheric heights, via a local dynamo or from small-scale flux emergence events. However, most of this small-scale magnetic field may not expand into the chromosphere due to the entropy drop with height at the photosphere. Here we present a study that uses a high resolution 3D radiative MHD simulation of the solar atmosphere with non-grey and non-LTE radiative transfer and thermal conduction along the magnetic field to reveal that: 1) the net magnetic flux from the simulated quiet photosphere is not sufficient to maintain a chromospheric magnetic field (on average), 2) processes in the lower chromosphere, in the region dominated by magneto-acoustic shocks, are able to convert kinetic energy into magnetic energy, 3) the magnetic energy in the chromosphere increases linearly in time until the r.m.s. of the magnetic field strength saturates at roughly 4 to 30 G (horizontal average) due to conversion from kinetic energy, 4) and that the magnetic features formed in the chromosphere are localized to this region.