Zobrazeno 1 - 10
of 62
pro vyhledávání: '"Michał Hanasz"'
Publikováno v:
Proceedings of 27th European Cosmic Ray Symposium — PoS(ECRS).
We investigate the impact of gas accretion in streams on the evolution of disc galaxies, using magneto-hydrodynamic simulations including advection and anisotropic diffusion of cosmic rays generated by supernovae as the only source of feedback. Strea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25fd77a6c2c1199765d7c64da34678bc
http://arxiv.org/abs/2109.12360
http://arxiv.org/abs/2109.12360
Publikováno v:
Living Reviews in Computational Astrophysics
We review numerical methods for simulations of cosmic ray (CR) propagation on galactic and larger scales. We present the development of algorithms designed for phenomenological and self-consistent models of CR propagation in kinetic description based
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8848fc49564c62db07c3a089e2147ac9
Publikováno v:
The Astrophysical Journal Supplement Series. 253:18
We present an efficient algorithm to follow spectral evolution of cosmic rays (CR) coupled with an MHD system on Eulerian grids. The algorithm is designed for studies of CR energy spectrum evolution in MHD simulations of a galactic interstellar mediu
Publikováno v:
Proceedings of the International Astronomical Union. 8:225-236
We review recent developments of amplification models of galactic and intergalactic magnetic field. The most popular scenarios involve variety of physical mechanisms, including turbulence generation on a wide range of physical scales, effects of supe
Autor:
Dominik Wóltański, Michał Hanasz, Marian Soida, B. Kulesza-Zydzik, Rafał Pawłaszek, Katarzyna Otmianowska-Mazur, Harald Lesch, Kacper Kowalik, Grzegorz Kowal
Publikováno v:
EAS Publications Series. 56:347-354
We present new developments on the cosmic-ray driven, galactic dynamo, modeled by means of direct, resistive CR–MHD simulations, performed with ZEUS and PIERNIK codes. The dynamo action, leading to the amplification of large–scale galactic magnet
Autor:
Michał Hanasz, Harald Lesch, Grzegorz Kowal, Marian Soida, Kacper Kowalik, Rafał Pawłaszek, Dominik Wóltański, K. Otmianowska-Mazur, Barbara Kulesza-Żydzik
Publikováno v:
Proceedings of the International Astronomical Union. 4:479-484
We present new developments on the Cosmic--Ray driven, galactic dynamo, modeled by means of direct, resistive CR--MHD simulations, performed with ZEUS and PIERNIK codes. The dynamo action, leading to the amplification of large--scale galactic magneti
Autor:
R. Kosiński, Michał Hanasz
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 376:861-870
We investigate the Parker instability (PI) influenced by thermal processes in a non-adiabatic, gravitationally stratified interstellar medium and discuss a model including the photoionization heating together with the supplemental heating mechanisms
Publikováno v:
Astronomische Nachrichten. 327:469-472
We present a further development of the first numerical model of the magnetohydrodynamical dynamo, driven by cosmic rays in the interstellar medium (Hanasz et al. 2004). The cosmic rays are produced in randomly occurring supernova remnants. Our model
Autor:
Michał Hanasz, R. Kosiński
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 368:759-768
We study Parker instability (PI) operating in a non-adiabatic, gravitationally stratified, interstellar medium. We discuss models with two kinds of heating mechanisms. The first one results from photoionization models. The other, relying on supplemen