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MHD Instabilities in Accretion Disks and Their Implications in Driving Fast Magnetic Reconnection
Luis H.S. Kadowaki
, Elisabete M. De Gouveia Dal Pino
,
James McLellan Stone
Astrophysical Sciences
Princeton Institute for Computational Science and Engineering
Research output
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Contribution to journal
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Article
›
peer-review
33
Scopus citations
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Engineering
Magnetohydrodynamics
100%
Magnetic Field
100%
Magnetohydrodynamic Generator
100%
Azimuthal
100%
Computer Simulation
100%
Peak Value
100%
Magnetic Flux
100%
Density Distribution
100%
Physics
Magnetohydrodynamic Generator
100%
Circumstellar Disk
100%
Accretion Disk
100%
Taylor Instability
50%
Magnetohydrodynamics
25%
Steady State
25%
Magnetic Field
25%
Density Distribution
25%
Current Sheet
25%
Magnetic Flux
25%
Solar Corona
25%
Earth and Planetary Sciences
Accretion Disk
100%
Taylor Instability
50%
Density Distribution
25%
Current Sheet
25%
Magnetohydrodynamics
25%
Solar Corona
25%
Keyphrases
Magnetic Loops
16%