On the Stability of Cylindrical Tangential Discontinuity, Generation and Damping of Helical Waves
A. I. Ershkovich, P.L. Israelevich

TL;DR
This paper analyzes the stability of cylindrical interfaces in fluids and plasmas, showing that helical waves in different contexts are governed by the same physics and can be simulated in laboratory settings.
Contribution
It demonstrates that helical waves in plasma tails and water jets are described by a unified dispersion relation, linking astrophysical phenomena with laboratory experiments.
Findings
Helical waves are described by a common dispersion equation.
Magnetic fields and surface tension have similar stabilizing effects.
Resonance damping of Kelvin-Helmholtz instability is demonstrated.
Abstract
Stability of cylindrical interface between two ideal incompressible fluids, including the magnetic field, surface tension and gravitational field is studied in linear approximation. We found that helical waves arising both in plasma comet tails and on the vertical cylindrical water jet in the air are described by the same dispersion equation where the comet tail magnetic field plays the same stabilizing role as surface tension for water jet. Hence they represent the same phenomenon of Kelvin-Helmholtz instability. Thus helical waves in comet tails and astrophysical jets may be simulated in the laboratory. The resonance nature of the Kelvin- instability damping is demonstrated.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geomagnetism and Paleomagnetism Studies
