KnowraMagnetohydrodynamicsLinked fromLinked fromThe 46 pages that link to Magnetohydrodynamics, each with the reason it gives.All 46Broader topic 5Related 16Narrower topic 22Compared with 3Stellar 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.Lorentz forceNarrower topic: Its fluid forces include the collective Lorentz force on moving charges.Earth's magnetic fieldNarrower topic: This broader framework describes the coupled fluid motion and magnetic forces inside the core.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.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.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.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.HeliopauseNarrower topic: Models of the heliopause combine plasma flow with magnetic forces.Astrophysical jetNarrower topic: Its equations describe how magnetic fields can accelerate and shape jet plasma.Alfvén's theoremNarrower topic: Alfvén's theorem is a conservation result within this broader framework.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.
KnowraMagnetohydrodynamicsLinked fromLinked fromThe 46 pages that link to Magnetohydrodynamics, each with the reason it gives.All 46Broader topic 5Related 16Narrower topic 22Compared with 3Stellar 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.Lorentz forceNarrower topic: Its fluid forces include the collective Lorentz force on moving charges.Earth's magnetic fieldNarrower topic: This broader framework describes the coupled fluid motion and magnetic forces inside the core.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.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.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.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.HeliopauseNarrower topic: Models of the heliopause combine plasma flow with magnetic forces.Astrophysical jetNarrower topic: Its equations describe how magnetic fields can accelerate and shape jet plasma.Alfvén's theoremNarrower topic: Alfvén's theorem is a conservation result within this broader framework.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.