Zobrazeno 1 - 10
of 63
pro vyhledávání: '"Szklarski, J."'
Autor:
Szklarski, J.
Publikováno v:
Astron.Nachr. 328 (2007) 499
Magnetorotational instability (MRI) is one of the most important and most common instabilities in astrophysics, it is widely accepted that it serves as a source of turbulent viscosity in accretion disks -- the most energy efficient objects in the Uni
Externí odkaz:
http://arxiv.org/abs/0704.2320
Autor:
Zawidzki, M., Szklarski, J.
Publikováno v:
In Applied Soft Computing Journal December 2019 85
Autor:
Stefani, F., Gerbeth, G., Gundrum, T., Hollerbach, R., Kirillov, O., Priede, J., Rüdiger, G., Szklarski, J.
Publikováno v:
AIMS 8th International Conference, 25.-28.05.2010, Dresden, Germany
The magnetorotational instability (MRI) is widely believed to play a key role in cosmic structure formation by maintaining turbulence and enabling angular momentum transport in accretion disks. The helical version of MRI (HMRI) was recently shown to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::204a121a948172088b0cc83cc38e0bf0
https://www.hzdr.de/publications/Publ-14129-1
https://www.hzdr.de/publications/Publ-14129-1
Autor:
Gundrum, T., Gerbeth, G., Stefani, F., Hollerbach, R., Priede, J., Rüdiger, G., Szklarski, J.
Publikováno v:
16th Couette-Taylor Workshop, 09.-11.09.2009, Princeton, USA
The magnetorotational instability (MRI) is believed to play a key role in the formation of stars and black holes by triggering turbulence in hydrodynamically stable Keplerian accretion discs. Although the MRI had been discovered by Velikhov as early
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::c4141c6ddef38e9b6f5ff992b5ab224b
https://www.hzdr.de/publications/Publ-12756-1
https://www.hzdr.de/publications/Publ-12756-1
Autor:
Stefani, F., Gerbeth, G., Gundrum, T., Hollerbach, R., Kirillov, O., Priede, J., Rüdiger, G., Szklarski, J.
Publikováno v:
12th MHD Days, 08.-09.12.2009, Potsdam, Germany
We give a survey about the recent experiments on the helical magnetorotational instability (MRI) in the framework of the Potsdam ROssendorf Magnetic InStability Experiment (PROMISE). By comparing the experimental results with numerical simulations we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::ba5bd6e76fb80e14efecad202a6a57db
https://www.hzdr.de/publications/Publ-13489-1
https://www.hzdr.de/publications/Publ-13489-1
Autor:
Stefani, F., Gerbeth, G., Gundrum, T., Hollerbach, R., Priede, J., Rüdiger, G., Szklarski, J.
Publikováno v:
Contributions to Geophysics and Geodesy 39(2009), 90-90
Natural dynamos, 30.08.-05.09.2009, Stara Lesna, Slovakia
Natural dynamos, 30.08.-05.09.2009, Stara Lesna, Slovakia
The magnetorotational instability (MRI) is known to play a key role in the formation of stars and black holes by triggering turbulence in hydrodynamically stable Keplerian accretion discs. As discussed recently, it might also play a role in the angul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::0942f2fe8a058aec4e8a00046df601fc
https://www.hzdr.de/publications/Publ-12757-2
https://www.hzdr.de/publications/Publ-12757-2
Publikováno v:
11th MHD days, 01.-03.12.2008, Ilmenau, Germany
The magnetorotational instability (MRI) is widely believed to play an essential role in the formation of stars and black holes. Destabilizing hydrodynamically stable Keplerian flows, the MRI triggers turbulence and enables outward transport of angula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::2fc2b81bb79de9a45795ef5a53910f3a
https://www.hzdr.de/publications/Publ-12022-1
https://www.hzdr.de/publications/Publ-12022-1
Publikováno v:
6th International Symposium on Ultrasonic Doppler Methods for Fluid Mechanics and Fluid Engineering, 09.-11.09.2008, Praha, Czech Republic
6th International Symposium on Ultrasonic Doppler Methods for Fluid Mechanics and Fluid Engineering, 09.-11.09.2008, Praha, Czech RepublicProceedings of the 6th International Symposium on Ultrasonic Doppler Methods for Fluid Mechanics and Fluid Engineering, Praque, Czech Republic: Czech Technical University in Praque, 978-80-87117-05-7, 65-68
6th International Symposium on Ultrasonic Doppler Methods for Fluid Mechanics and Fluid Engineering, 09.-11.09.2008, Praha, Czech RepublicProceedings of the 6th International Symposium on Ultrasonic Doppler Methods for Fluid Mechanics and Fluid Engineering, Praque, Czech Republic: Czech Technical University in Praque, 978-80-87117-05-7, 65-68
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:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::51a5304373b9074d4ee2b66139436910
https://www.hzdr.de/publications/Publ-10867-1
https://www.hzdr.de/publications/Publ-10867-1
Publikováno v:
Geophysical Research Abstracts 10(2008), 01989
The magnetorotational instability (MRI) is one of the most promising candidates to explain turbulence and angular momentum transport in accretion disks which is essential to understand the mass accumulation of stars and black holes. Only recently, a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______4577::9a4defb4d1da330ced13e0590d1d490b
https://www.hzdr.de/publications/Publ-10969-1
https://www.hzdr.de/publications/Publ-10969-1
Publikováno v:
15th International Couette-Taylor Workshop, 09.-12.07.2007, Le Havres, France
15th International Couette-Taylor Workshop, 09.-12.07.2007, Le Havre, FranceProceedings of the 15th International Couette-Taylor Workshop, Le Havre, 266-269
15th International Couette-Taylor Workshop, 09.-12.07.2007, Le Havre, FranceProceedings of the 15th International Couette-Taylor Workshop, Le Havre, 266-269
Cosmic magnetic fields are not only passive by-products of the hydromagnetic dynamo effect, they also play an active role in the formation of stars and black holes by virtue of the Magnetorotational Instability (MRI). By destabilizing Keplerian flows
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b62700f61599a398de3d80c3532010c8
https://www.hzdr.de/publications/Publ-9758-1
https://www.hzdr.de/publications/Publ-9758-1