Zobrazeno 1 - 10
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pro vyhledávání: '"SZKLARSKI, Jacek"'
Autor:
Szklarski, Jacek T.
Magnetorotational instability (MRI) is one of the most important and most common instabilities in astrophysics. Today it is widely accepted that it serves as a major source of turbulent viscosity in accretion disks, the most energy efficient objects
Externí odkaz:
http://opus.kobv.de/ubp/volltexte/2008/1600/
Autor:
Zawidzki, Machi, Szklarski, Jacek
Publikováno v:
In Advances in Engineering Software March 2020 141
Autor:
Stefani, Frank, Gerbeth, Gunter, Gundrum, Thomas, Hollerbach, Rainer, Priede, Jānis, Rüdiger, Günther, Szklarski, Jacek
Publikováno v:
Phys.Rev.E80:066303,2009
The magnetorotational instability (MRI) is thought to play a key role in the formation of stars and black holes by sustaining the turbulence in hydrodynamically stable Keplerian accretion discs. In previous experiments the MRI was observed in a liqui
Externí odkaz:
http://arxiv.org/abs/0904.1027
Autor:
Stefani, Frank, Gerbeth, Gunter, Gundrum, Thomas, Szklarski, Jacek, Ruediger, Guenther, Hollerbach, Rainer
The magnetorotational instability (MRI) plays an essential role in the formation of stars and black holes. By destabilizing hydrodynamically stable Keplerian flows, the MRI triggers turbulence and enables outward transport of angular momentum in accr
Externí odkaz:
http://arxiv.org/abs/0812.3790
Autor:
Szklarski, Jacek, Rüdiger, Günther
Publikováno v:
Phys.Rev.E76:066308,2007
We study magnetic effects induced by rigidly rotating plates enclosing a cylindrical MHD Taylor-Couette flow at the finite aspect ratio $H/D=10$. The fluid confined between the cylinders is assumed to be liquid metal characterized by small magnetic P
Externí odkaz:
http://arxiv.org/abs/0710.5600
Autor:
Stefani, Frank, Gundrum, Thomas, Gerbeth, Gunter, Rüdiger, Günther, Szklarski, Jacek, Hollerbach, Rainer
Publikováno v:
NewJ.Phys.9:295,2007
The magnetorotational instability (MRI) plays a key role in the formation of stars and black holes, by enabling outward angular momentum transport in accretion disks. The use of combined axial and azimuthal magnetic fields allows the investigation of
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701030
Autor:
Szklarski, Jacek, Rüdiger, Günther
Publikováno v:
Astron.Nachr.327:844-849,2006
The magnetorotational instability (MRI) in cylindrical Taylor-Couette flow with external helical magnetic field is simulated for infinite and finite aspect ratios. We solve the MHD equations in their small Prandtl number limit and confirm with time-d
Externí odkaz:
http://arxiv.org/abs/astro-ph/0608703
Autor:
Stefani, Frank, Gundrum, Thomas, Gerbeth, Gunter, Rüdiger, Günther, Schultz, Manfred, Szklarski, Jacek, Hollerbach, Rainer
Publikováno v:
Phys.Rev.Lett. 97 (2006) 184502
A recent paper [R. Hollerbach and G. Rudiger, Phys. Rev. Lett. 95, 124501 (2005)] has shown that the threshold for the onset of the magnetorotational instability (MRI) in a Taylor-Couette flow is dramatically reduced if both axial and azimuthal magne
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606473
Autor:
Zawidzki, Machi, Szklarski, Jacek
Publikováno v:
In Advances in Engineering Software December 2018 126:147-160
Autor:
Zawidzki, Machi, Szklarski, Jacek
Publikováno v:
In Applied Soft Computing Journal September 2018 70:501-512