magnetorotational instability
GPTKB entity
Statements (24)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
physical phenomenon
|
| gptkbp:abbreviation |
MRI
|
| gptkbp:appliesTo |
protoplanetary disks
accretion disks galactic disks |
| gptkbp:cause |
turbulence in accretion disks
|
| gptkbp:describedYear |
1959
|
| gptkbp:describes |
instability in differentially rotating, magnetized fluids
|
| gptkbp:developedBy |
gptkb:John_Hawley
gptkb:Steven_Balbus |
| gptkbp:enables |
angular momentum transport
|
| gptkbp:explains |
efficient accretion in disks
|
| gptkbp:field |
astrophysics
magnetohydrodynamics |
| gptkbp:firstDescribed |
gptkb:Evgeny_Velikhov
|
| https://www.w3.org/2000/01/rdf-schema#label |
magnetorotational instability
|
| gptkbp:popularizedBy |
1991
|
| gptkbp:relatedTo |
gptkb:Rayleigh_instability
magnetohydrodynamic turbulence |
| gptkbp:requires |
differential rotation
weak magnetic field |
| gptkbp:bfsParent |
gptkb:Magnetohydrodynamics
gptkb:Z-pinch |
| gptkbp:bfsLayer |
6
|