Ideal magnetic-fluid induction and divergence
Research context
research method · conditional · As of 2026-10-10
Ideal conducting-fluid motion evolves magnetic flux by induction and preserves an initially solenoidal field.
Key knowledge
Ideal conducting-fluid motion evolves magnetic flux by induction and preserves an initially solenoidal field. Frozen flux applies only within that limit; reconnection requires nonideal effects or kinetic physics.
Values and equations
∂B/∂t=curl(v×B); div B=0
- B
- Magnetic field T
- v
- Fluid velocity m s^-1
- t
- Time s
Conditions and scope
- Nonrelativistic fluid, negligible displacement current, sufficient scale separation and ideal conductivity.
- Initial/boundary data and numerical divergence control are essential.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
Astrophysical fluid dynamics: Sections 3–5 and 9: ideal MHD, stress, waves, energy and angular-momentum fluxes (selected source body inspected).
2026-10-10 · Bounded source check of the recorded statement and conditions. This does not certify a unique physical model, reproduce the cited study or replace independent branch review.
Entry details
Permanent link to this entry ↗- Record identity
- research-earth-ideal-induction
- Revision
- research.1
- Structured reference record
- Postgraduate & research reference