Linked from

The 46 pages that link to Magnetohydrodynamics, each with the reason it gives.

• Star formationRelated: Simulations use it to test how magnetic fields alter cloud collapse and fragmentation.

• Stellar windNarrower topic: Its equations describe the wind’s coupled plasma flow and magnetic field.

• Accretion diskNarrower topic: Magnetic fields couple disk regions and shape their stresses, turbulence, and outflows.

• HydrodynamicsBroader topic: It extends liquid-flow analysis to conducting fluids under electromagnetic forces.

• Plasma physicsRelated: It captures large-scale plasma motion when fluid behavior is a useful approximation.

• Lorentz forceNarrower topic: Its fluid forces include the collective Lorentz force on moving charges.

• Relativistic jetRelated: Magnetohydrodynamic forces help accelerate and collimate plasma in many astrophysical jets.

• Spherical harmonicsRelated: Global magnetic-field models often expand angular structure in spherical harmonics.

• Fluid dynamicsBroader topic: It extends ordinary fluid dynamics by coupling flow to electromagnetic forces.

• Earth's magnetic fieldNarrower topic: This broader framework describes the coupled fluid motion and magnetic forces inside the core.

• Magnetic confinement fusionRelated: Its equations describe large-scale plasma motion and many confinement instabilities.

• Solar magnetic fieldNarrower topic: It provides the physical framework for understanding magnetic fields embedded in solar plasma.

• HeliosphereNarrower topic: It describes the coupled plasma and magnetic-field behavior that shapes the heliosphere.

• Radio galaxyRelated: Magnetic fields and plasma dynamics shape the launching and collimation of radio jets.

• Alfvén waveNarrower topic: Its equations describe Alfvén waves when plasma is treated as a conducting fluid.

• Solar dynamoNarrower topic: It supplies the fluid-and-field equations used to describe solar dynamo action.

• GeodynamoNarrower topic: It provides the physical framework for fluid motion generating and reshaping the geodynamo’s magnetic field.

• Circumgalactic mediumRelated: Magnetic fields may shape gas transport, yet their circumgalactic structure is poorly constrained.

• Coronal heating problemNarrower topic: Its equations describe the magnetic structures and waves implicated in coronal heating.

• Earth's outer coreNarrower topic: Its equations describe how core flow and magnetic fields influence each other.

• Interstellar magnetic fieldNarrower topic: This framework describes how the field and ionized interstellar gas move together.

• Pulsar wind nebulaNarrower topic: It describes the coupled flow and magnetic structure of the nebula.

• Interplanetary magnetic fieldNarrower topic: Its equations describe how the solar wind transports and deforms the field.

• Lyman SpitzerRelated: Its equations describe how magnetic fields and conducting plasma move together in fusion devices.

• Stellar magnetic fieldNarrower topic: Its equations describe how stellar plasma and magnetic fields evolve together.

• ChromosphereNarrower topic: Magnetic forces shape chromospheric plasma, which is modeled as a conducting fluid.

• Flocculent spiral galaxyNarrower topic: Magnetic fields and gas flows influence the structure of star-forming regions in galactic disks.

• Hannes AlfvénBroader topic: Alfvén helped establish this framework for describing plasma and liquid-metal flows.

• HeliopauseNarrower topic: Models of the heliopause combine plasma flow with magnetic forces.

• Adaptive mesh refinementRelated: AMR can track localized current sheets and other steep magnetic structures.

• Solar physicsRelated: It supplies the main physical framework for modeling solar plasma and magnetic structures.

• Solenoidal vector fieldBroader topic: Its incompressible models couple two divergence-free fields: velocity and magnetic field.

• Astrophysical fluid dynamicsRelated: It describes plasma flows in stars, disks, and the interstellar medium.

• Magnetosphere of SaturnRelated: It describes large-scale interactions between Saturn’s magnetic field and its plasma.

• Space physicsRelated: It provides a large-scale description of plasma flows and magnetic structures.

• Astrophysical jetNarrower topic: Its equations describe how magnetic fields can accelerate and shape jet plasma.

• Circumstellar discRelated: Magnetic stresses can transport angular momentum through ionized regions of a disc.

• Vlasov equationCompared with: It describes plasma at fluid scales, while Vlasov models retain the particle velocity distribution.

• Alfvén's theoremNarrower topic: Alfvén's theorem is a conservation result within this broader framework.

• Astrophysical electromagnetic fieldsBroader topic: It describes how cosmic plasma flows carry, amplify, and reshape magnetic fields.

• Computational astrophysicsRelated: It models magnetized plasmas in stars, accretion disks, and interstellar space.

• Electrokinetic flowsCompared with: It couples fluid motion to magnetic forces, unlike electrokinetics' interfacial electric forcing.

• First-principles calculations in plasma physicsCompared with: Its fluid closure is efficient but suppresses much particle-scale kinetic behavior.

• High-energy-density plasmaRelated: Magnetic fields can redirect heat flow and alter plasma stability.

• Laboratory studies of space and astrophysical plasmasNarrower topic: It supplies a macroscopic framework for interpreting many laboratory plasma experiments.

• Magnetohydrodynamic techniquesNarrower topic: These techniques apply magnetohydrodynamic principles to measurement and control.