Zobrazeno 1 - 10
of 74
pro vyhledávání: '"M J Pueschel"'
Publikováno v:
New Journal of Physics, Vol 18, Iss 7, p 075018 (2016)
A notable feature of plasma turbulence is its propensity to retain features of the underlying linear eigenmodes in a strongly turbulent state—a property that can be exploited to predict various aspects of the turbulence using only linear informatio
Externí odkaz:
https://doaj.org/article/558bd2f604ba4033b474d9e43b5de7ce
Publikováno v:
SN Applied Sciences, Vol 4, Iss 1, Pp 1-14 (2021)
Abstract Cosmic-ray transport in astrophysical environments is often dominated by the diffusion of particles in a magnetic field composed of both a turbulent and a mean component. This process, which is two-fold turbulent mixing in that the particle
Externí odkaz:
https://doaj.org/article/d6f926516472474ea47a169d37a9ad7f
Publikováno v:
Physics of Plasmas, 30(4):042303. American Institute of Physics
Physics of Plasmas, 30, 042303
Physics of Plasmas, 30, 042303
The magnetic drift and the electric potential play an important role in microtearing destabilization by increasing the growth rate of this instability in the presence of collisions, while in electrostatic plasma micro-turbulence, zonal electric poten
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::89cf4b56dea9c02fead7179c283375c6
https://doi.org/10.1063/5.0104879
https://doi.org/10.1063/5.0104879
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 514(2), 2658-2666. Wiley-Blackwell
Monthly Notices of the Royal Astronomical Society, 514, 2658–2666
Monthly Notices of the Royal Astronomical Society, 514, 2658–2666
Understanding the time scales for diffusive processes and their degree of anisotropy is essential for modelling cosmic-ray transport in turbulent magnetic fields. We show that the diffusion time scales are isotropic over a large range of energy and t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a61fadd2a45448e590482500cc7c2f82
https://research.tue.nl/nl/publications/8a741fb6-c72b-48d9-aab8-2fd6fc08a27e
https://research.tue.nl/nl/publications/8a741fb6-c72b-48d9-aab8-2fd6fc08a27e
Autor:
D. R. Hatch, C. Michoski, D. Kuang, B. Chapman-Oplopoiou, M. Curie, M. Halfmoon, E. Hassan, M. Kotschenreuther, S. M. Mahajan, G. Merlo, M. J. Pueschel, J. Walker, C. D. Stephens
Publikováno v:
Physics of Plasmas, 29(6):062501. American Institute of Physics
This paper reports on the development of reduced models for electron temperature gradient (ETG) driven transport in the pedestal. Model development is enabled by a set of 61 nonlinear gyrokinetic simulations with input parameters taken from pedestals
Publikováno v:
Physics of Plasmas, 29, 012303
Physics of Plasmas, 29(1):012303. American Institute of Physics
Physics of Plasmas, 29(1):012303. American Institute of Physics
The linear and nonlinear properties of ion-temperature-gradient-driven turbulence with adiabatic electrons are modeled for axisymmetric configurations for a broad range of triangularities δ, both negative and positive. Peak linear growth rates decre
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5643bfa864ad043d3bb20fee6a38f46d
https://www.differ.nl/bibcite/reference/8866
https://www.differ.nl/bibcite/reference/8866
Publikováno v:
SN Applied Sciences, 4, 15
Sn Applied Sciences
SN Applied Sciences, 4(1):15. Springer
Appl.Sciences
Appl.Sciences, 2022, 4, pp.15. ⟨10.1007/s42452-021-04891-z⟩
SN Applied Sciences, Vol 4, Iss 1, Pp 1-14 (2021)
Sn Applied Sciences
SN Applied Sciences, 4(1):15. Springer
Appl.Sciences
Appl.Sciences, 2022, 4, pp.15. ⟨10.1007/s42452-021-04891-z⟩
SN Applied Sciences, Vol 4, Iss 1, Pp 1-14 (2021)
Cosmic-ray transport in astrophysical environments is often dominated by the diffusion of particles in a magnetic field composed of both a turbulent and a mean component. This process, which is two-fold turbulent mixing in that the particle motion is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::80c07b9a37ce03e02685c7be4f9cb98e
https://www.differ.nl/bibcite/reference/8868
https://www.differ.nl/bibcite/reference/8868
Publikováno v:
Physics of Plasmas, 29(9):092301. American Institute of Physics
Physics of Plasmas, 29, 092301
Physics of Plasmas, 29, 092301
Visco-resistive magnetohydrodynamic turbulence, driven by a two-dimensional unstable shear layer that is maintained by an imposed body force, is examined by decomposing it into dissipationless linear eigenmodes of the initial profiles. The down-gradi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6251baa9a04b2a415c2d2d12a4905f6
https://arxiv.org/abs/2208.03342
https://arxiv.org/abs/2208.03342
Publikováno v:
Physics of Plasmas, 29, 070701
Physics of Plasmas, 29(7):070701. American Institute of Physics
Physics of Plasmas, 29(7):070701. American Institute of Physics
Straining of magnetic fields by large-scale shear flow, generally assumed to lead to intensification and generation of small scales, is re-examined in light of the persistent observation of large-scale magnetic fields in astrophysics. It is shown tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2beef0291a0ac25154a059a8d229bb1f
https://www.differ.nl/bibcite/reference/8803
https://www.differ.nl/bibcite/reference/8803
Publikováno v:
Journal of Plasma Physics, 87, 905870401
The variation of pressure-gradient-driven turbulence with plasma $\beta$ (up to $\beta \approx 15\,\%$ ) is investigated in linear, magnetized plasma. The magnitude of magnetic fluctuations is observed to increase substantially with increasing $\beta