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相关论文: Ionization fronts in negative corona discharges

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We present a method for including steady-state gas flows in the plasma physics code Cloudy, which was previously restricted to modeling static configurations. The numerical algorithms are described in detail, together with an example…

天体物理学 · 物理学 2009-11-10 William J. Henney , S. Jane Arthur , Robin J. R. Williams , Gary J. Ferland

Pictures show that streamer or sprite discharge channels emerging from the same electrode sometimes seem to reconnect or merge though their heads carry electric charge of the same polarity; one might therefore suspect that reconnections are…

等离子体物理 · 物理学 2009-01-16 S. Nijdam , C. G. C. Geurts , E. M. van Veldhuizen , U. Ebert

The photoionization-driven evaporation of planetary atmospheres has emerged as a potentially fundamental process for planets on short period orbits. While 1-D studies have proven the effectiveness of stellar fluxes at altering the…

地球与行星天体物理 · 物理学 2018-12-19 Alex Debrecht , Jonathan Carroll-Nellenback , Adam Frank , John McCann , Ruth Murray-Clay , Eric G. Blackman

To characterize the conditions required to reach advanced divertor regimes, a one-dimensional computational model has been developed based on a coordinate transformation to incorporate two-dimensional effects. This model includes transport…

plasm-ph · 物理学 2009-10-28 R. A. Vesey , D. E. Post , G. Bateman

Interchange reconnection is thought to play an important role in determining the dynamics and material composition of the slow solar wind that originates from near coronal hole boundaries. To explore the implications of this process we…

太阳与恒星天体物理 · 物理学 2022-07-20 Roger B. Scott , Stephen J. Bradshaw , Mark G. Linton

Positive and negative streamers are studied in ambient air at 1 bar; they emerge from a needle electrode placed 40 mm above a planar electrode. The amplitudes of the applied voltage pulses range from 5 to 96 kV; most pulses have rise times…

等离子体物理 · 物理学 2008-11-21 T. M. P. Briels , J. Kos , G. J. J. Winands , E. M. van Veldhuizen , Ute Ebert

We have investigated the evaporation of close-in exoplanets irradiated by ionizing photons. We find that the properties of the flow are controlled by the ratio of the recombination time to the flow time-scale. When the recombination…

地球与行星天体物理 · 物理学 2016-01-13 James E. Owen , Marcelo A. Alvarez

A major goal of solar physics is understanding the transition of the medium from the closed-loop magnetic configuration of the corona to the open structure of the heliospheric current sheet. The evolution of solar wind streamers, an…

太阳与恒星天体物理 · 物理学 2026-04-20 Forrest Mozer , Kyungeun Choi , Richard Sydora , Andrii . Voshchepynets

Small scale transients occur in the Solar corona at much higher frequencies than flares and play a significant role in coronal dynamics. Here we study three well-identified transients discovered by Hi-C and also detected by the EUV channels…

太阳与恒星天体物理 · 物理学 2021-10-01 Abhishek Rajhans , Durgesh Tripathi , Vinay L. Kashyap

Structural aspects of crystal nucleation in undercooled liquids are explored using a nonlinear hydrodynamic theory of crystallization proposed recently [G. I. Toth et al., J. Phys.: Condens. Matter 26, 055001 (2014)], which is based on…

材料科学 · 物理学 2017-05-24 Frigyes Podmaniczky , Gyula I. Toth , Gyorgy Tegze , Laszlo Granasy

Continuum simulation is employed to study ion transport and fluid flow through a nanopore in a solid-state membrane under an applied potential drop. Results show the existence of concentration polarization layers on the surfaces of the…

流体动力学 · 物理学 2015-06-16 Mao Mao , Sandip Ghosal , Guohui Hu

The procedure has been developed for extracting homocharge and heterocharge currents from experimentally measured thermally stimulated depolarization currents of corona poled PVDF. Application of different depolarization modes supplemented…

材料科学 · 物理学 2007-05-23 S. N. Fedosov , A. F. Butenko , A. E. Sergeeva

Oceanic internal waves often have curvilinear fronts and propagate over various currents. We present the first study of long weakly-nonlinear internal ring waves in a three-layer fluid in the presence of a background linear shear current.…

流体动力学 · 物理学 2022-07-01 D. Tseluiko , N. S. Alharthi , R. Barros , K. R. Khusnutdinova

The aim of this work is to improve the modelling of ion populations in higher density, lower temperature astrophysical plasmas, of the type commonly found in lower solar and stellar atmospheres. Ion population models for these regions…

太阳与恒星天体物理 · 物理学 2019-06-26 R. P. Dufresne , G. Del Zanna

Reaction fronts evolving in a porous medium exhibit a rich dynamical behaviour. In presence of an adverse flow, experiments show that the front slows down and eventually gets pinned, displaying a particular sawtooth shape. Extensive…

无序系统与神经网络 · 物理学 2016-10-28 Thomas Gueudré , Awadhesh Kumar Dubey , Laurent Talon , Alberto Rosso

We study the traveling wave solutions of a lattice Boltzmann model for the planar streamer fronts that appear in the transport of electrons through a gas in a strong electrical field. To mimic the physical properties of the impact…

计算物理 · 物理学 2007-05-23 Wim Vanroose , Giovanni Samaey , Pieter Van Leemput

Observations of active regions and limb prominences often show cold, dense blobs descending with an acceleration smaller than that of free fall. The dynamics of these condensations falling in the solar corona is investigated in this paper…

太阳与恒星天体物理 · 物理学 2014-03-03 R. Oliver , R. Soler , J. Terradas , T. V. Zaqarashvili , M. L. Khodachenko

In this paper we study the lateral instability of streamer discharges using a continuum discharge model. We observe similarities to Kelvin-Helmholz instability in fluids. In strong electric fields, lateral long wave length perturbations can…

等离子体物理 · 物理学 2021-05-11 M. Arrayás , M. A. Fontelos

A novel type of particle "cooling", called Ionization Cooling, is applicable to slow (v of the order of 0.1c) ions stored in a small ring. The many traversals through a thin foil enhance the nuclear reaction probability, in a steady…

高能物理 - 唯象学 · 物理学 2011-05-18 C. Rubbia , A. Ferrari , Y. Kadi , V. Vlachoudis

Between the base of the solar corona and the Alfven critical point, the solar-wind density decreases by approximately five orders of magnitude, but the temperature varies by a factor of only a few. In this paper, I show that such…

太阳与恒星天体物理 · 物理学 2021-06-16 Benjamin D. G. Chandran