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Structure of protoplanetary discs with magnetically driven winds
Fazeleh Khajenabi, Mohsen Shadmehri,
Martin E. Pessah
, Rebecca G. Martin
Niels Bohr International Academy
4
Citations (Scopus)
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Keyphrases
Dust Layer
100%
Protoplanetary Disks
100%
Accretion Rate
100%
Mid-plane
66%
Mass Loss
66%
Observational Constraints
33%
Steady State
33%
Angular Momentum
33%
Turbulence
33%
Dust
33%
Accretion Discs
33%
Astrophysical Applications
33%
Analytical Solution
33%
Plasma Parameters
33%
Parametrization
33%
State Structure
33%
Disc Model
33%
Surface Density
33%
Physics
Protoplanetary Disk
100%
Steady State
50%
Blood Plasma
50%
Angular Momentum
50%
Circumstellar Disks
50%
Earth and Planetary Sciences
Protoplanetary Disk
100%
Angular Momentum
50%
Accretion Disk
50%
Engineering
Mass Loss
66%
Angular Momentum
33%
Disc Surface
33%
Surface Density
33%
Parametrization
33%