Related Experiment Video
Updated: Sep 24, 2025

Building Langmuir Probes and Emissive Probes for Plasma Potential Measurements in Low Pressure, Low Temperature Plasmas
Published on: May 25, 2021
Spontaneous magnetization of collisionless plasma.
Muni Zhou1, Vladimir Zhdankin2,3, Matthew W Kunz3,4
1Plasma Science and Fusion Center, Massachusetts Institute of Technology, Cambridge, MA 02139.
Cosmic magnetic fields originate from generic plasma turbulence, not just astrophysical processes. This study explains the spontaneous generation of these initial magnetic fields, advancing our understanding of cosmic magnetogenesis.
Area of Science:
- Astrophysics
- Plasma Physics
- Cosmology
Background:
- Dynamically significant magnetic fields are observed throughout the Universe.
- The origin of these cosmic magnetic fields remains a fundamental unsolved problem in astrophysics.
Purpose of the Study:
- To provide a new theoretical framework for understanding the origin of cosmic magnetism.
- To investigate the role of plasma microphysics in the generation of magnetic fields.
Main Methods:
- Utilizing kinetic plasma physics to analyze astrophysical turbulence.
- Developing theoretical models and performing numerical simulations.
Main Results:
- Demonstrating the spontaneous generation of initial magnetic fields by astrophysical turbulence.
- Showing that cosmic plasmas can become ubiquitously magnetized through these processes.
Conclusions:
- This work presents a paradigm for cosmic magnetogenesis, explaining the origin of primordial magnetic fields.
- The findings lay the groundwork for understanding how these seed fields are amplified by turbulent dynamos.
Related Concept Videos
Potential Due to a Magnetized Object
The vector...
Paramagnetism
Atomic Nuclei: Nuclear Relaxation Processes
Diamagnetism
Diamagnetism was discovered by Anton Brugmans in 1778 when he observed that bismuth gets repelled by magnetic fields, thus theorizing that diamagnets get repelled by magnets....
Atomic Nuclei: Nuclear Magnetic Moment
Magnetostatic Boundary Conditions

