# Interaction of a supersonic particle with a three-dimensional complex   plasma

**Authors:** E. Zaehringer, M. Schwabe, S. Zhdanov, D. P. Mohr, C. A. Knapek, P., Huber, I. L. Semenov, and H. M. Thomas

arXiv: 1803.00870 · 2018-03-16

## TL;DR

This study investigates how a supersonic particle interacts with a three-dimensional complex plasma in microgravity, revealing Mach cone formation, particle charge estimations, and localized heating effects at the microscopic level.

## Contribution

It provides detailed experimental observations of Mach cone structures and particle dynamics in 3D complex plasma under microgravity conditions, using high-resolution imaging.

## Key findings

- Mach cones with M ≈ 1.5 - 2 observed in plasma
- Particle charge estimations compared with standard theories
- Localized heating behind the supersonic projectile

## Abstract

The influence of a supersonic projectile on a three-dimensional complex plasma is studied. Micron sized particles in a low-temperature plasma formed a large undisturbed system in the new 'Zyflex' chamber during microgravity conditions. A supersonic probe particle excited a Mach cone with Mach number M $\approx$ 1.5 - 2 and double Mach cone structure in the large weakly damped particle cloud. The speed of sound is measured with different methods and particle charge estimations are compared to calculations from standard theories. The high image resolution enables the study of Mach cones in microgravity on the single particle level of a three-dimensional complex plasma and gives insight to the dynamics. A heating of the microparticles is discovered behind the supersonic projectile but not in the flanks of the Mach cone.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1803.00870/full.md

## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/1803.00870/full.md

## References

48 references — full list in the complete paper: https://tomesphere.com/paper/1803.00870/full.md

---
Source: https://tomesphere.com/paper/1803.00870