Simulations of jet formation from a magnetized accretion disk (Q1911028)
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scientific article; zbMATH DE number 865823
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | Simulations of jet formation from a magnetized accretion disk |
scientific article; zbMATH DE number 865823 |
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Simulations of jet formation from a magnetized accretion disk (English)
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29 May 1996
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Formations of plasma jet flows resulting from a differentially rotating magnetized Keplerian gaseous disk are investigated for various time intervals. The initial magnetic field is poloidal and is distorted by the rotation of the disk. This change of the magnetic field induces jet-like outflows of matter which are time-dependent at the beginning and seem to tend to a stationary state after approximately 60 rotation periods. The considered simulations of jet formations can be used in astrophysical applications to active galactic nuclei and stellar systems.
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stellar atmospheres
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plasma flows
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active galactic nuclei
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stellar systems
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