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2. Magnetohydrodynamics - Wikipedia

   en.wikipedia.org/wiki/Magnetohydrodynamics

   A magnetohydrodynamic drive or MHD propulsor is a method for propelling seagoing vessels using only electric and magnetic fields with no moving parts, using magnetohydrodynamics. The working principle involves electrification of the propellant (gas or water) which can then be directed by a magnetic field, pushing the vehicle in the opposite ...

3. Magnetohydrodynamic turbulence - Wikipedia

   en.wikipedia.org/wiki/Magnetohydrodynamic_Turbulence

   Magnetohydrodynamics (MHD) deals with what is a quasi-neutral fluid with very high conductivity. The fluid approximation implies that the focus is on macro length-and-time scales which are much larger than the collision length and collision time respectively.

4. Alfvén's theorem - Wikipedia

   en.wikipedia.org/wiki/Alfvén's_theorem

   Informally, Alfvén's theorem refers to the fundamental result in ideal magnetohydrodynamic theory that electrically conducting fluids and the magnetic fields within are constrained to move together in the limit of large magnetic Reynolds numbers (R m)—such as when the fluid is a perfect conductor or when velocity and length scales are infinitely large.

5. Magneto-hydrodynamic - Wikipedia

   en.wikipedia.org/?title=Magneto-hydrodynamic&...

   Download QR code; Print/export Download as PDF; Printable version; In other projects Appearance. move to sidebar hide. From Wikipedia, the free encyclopedia.

6. Hopf fibration - Wikipedia

   en.wikipedia.org/wiki/Hopf_fibration

   5 Notes. 6 References. ... Download as PDF; Printable version; ... Similar patterns of fields are found as soliton solutions of magnetohydrodynamics: [4]

7. Magnetic Reynolds number - Wikipedia

   en.wikipedia.org/wiki/Magnetic_Reynolds_number

   In magnetohydrodynamics, the magnetic Reynolds number (R m) is a dimensionless quantity that estimates the relative effects of advection or induction of a magnetic field by the motion of a conducting medium to the magnetic diffusion. It is the magnetic analogue of the Reynolds number in fluid mechanics and is typically defined by: