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相关论文: Ionization fronts in negative corona discharges

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Using an analogy to the classical Stefan problem, we construct evolution equations for the fluid pore pressure on both sides of a propagating stress-induced damage front. Closed form expressions are derived for the position of the damage…

地球物理 · 物理学 2014-09-01 K. C. Lewis , Satish Karra , Sharad Kelkar

Aims. We aim to improve the understanding of the physical mechanisms behind the slower than free-fall motion and the two-stage evolution (an initial phase of acceleration followed by an almost constant velocity phase) detected in coronal…

太阳与恒星天体物理 · 物理学 2020-02-05 David Martínez-Gómez , Ramón Oliver , Elena Khomenko , Manuel Collados

Recent observations of the solar corona with the LASCO coronagraph on board of the SOHO spacecraft have revealed the occurrence of triple helmet streamers even during solar minimum, which occasionally go unstable and give rise to large…

天体物理学 · 物理学 2015-05-13 T. Wiegelmann , K. Schindler , T. Neukirch

Ion source modification is proposed for efficient production of ion beam and extending of operating Lifetime. Ionization efficiency of the Bernas type ion source has been improved by using a small anode-thin rod, oriented along the magnetic…

等离子体物理 · 物理学 2019-12-10 V Dudnikov , G Dudnikova , A Dudnikov

We consider the evolution of fronts by mean curvature in the presence of obstacles. We construct a weak solution to the flow by means of a variational method, corresponding to an implicit time-discretization scheme. Assuming the regularity…

数值分析 · 数学 2015-06-03 Luís Almeida , Antonin Chambolle , Matteo Novaga

The physical processes in the solar corona that shape the solar wind remain an active research topic. Modeling efforts have shown that energy and plasma exchanges near the transition region plays a crucial role in modulating solar wind…

The solar corona has been revealed in the past decade to be a highly dynamic nonequilibrium plasma environment. Both the loop-filled coronal base and the extended acceleration region of the solar wind appear to be strongly turbulent, but…

天体物理学 · 物理学 2008-11-26 Steven R. Cranmer

Reaction-diffusion models with nonlocal constraints naturally arise as limiting cases of coupled bulk-surface models of intracellular signalling. In this paper, a minimal, mass-conserving model of cell-polarization on a curved membrane is…

斑图形成与孤子 · 物理学 2022-10-04 Pearson W. Miller , Daniel Fortunato , Matteo Novaga , Stanislav Y. Shvartsman , Cyrill B. Muratov

We investigate spreading properties of solutions of a large class of two-component reaction-diffusion systems, including prey-predator systems as a special case. By spreading properties we mean the long time behaviour of solution fronts…

偏微分方程分析 · 数学 2019-07-08 Arnaud Ducrot , Thomas Giletti , Hiroshi Matano

Janus --or two-sided, charged membranes offer promise as ionic current rectifiers. In such systems, pores consisting of two regions of opposite charge can be used to generate a current from a gradient in salinity. The efficiency of…

This paper presents a new resolution strategy for multi-scale streamer discharge simulations based on a second order time adaptive integration and space adaptive multiresolution. A classical fluid model is used to describe plasma…

Close-in hot Jupiters are exposed to a tremendous photon flux that ionizes the neutral escaping material from the planet leaving an observable imprint that makes them an interesting laboratory for testing theoretical models. In this work we…

地球与行星天体物理 · 物理学 2016-02-17 E. M. Schneiter , A. Esquivel , C. S. Villarreal D'Angelo , P. F. Velazquez , A. C. Raga , A. Costa

We numerically investigate the geometry and transport properties of infection fronts within the spatial SIR model in two dimensions. The model incorporates short-range correlated quenched random transmission rates. Our findings reveal that…

无序系统与神经网络 · 物理学 2024-09-18 Renzo Zagarra , Karina Laneri , Alejandro B. Kolton

Strong magnetic fields are of vital importance to the physics of the solar corona. They easily move a rarefied coronal plasma. Physical origin of the main structural element of the corona, the so-called coronal streamers, is discussed. It…

太阳与恒星天体物理 · 物理学 2013-03-14 Boris Somov

For a magnetic flux tube, or indeed any flux, to emerge into the Solar corona from the convection zone it must pass through the partially ionised layers of the lower atmosphere: the photosphere and the chromosphere. In such regions the…

天体物理学 · 物理学 2011-02-11 T. D. Arber , M. Haynes , J. E. Leake

In this paper we present a numerical study of the dynamics of partially ionized coronal rain blobs. We use a two-fluid model to perform a high-resolution 2D simulation that takes into account the collisional interaction between the charged…

太阳与恒星天体物理 · 物理学 2022-12-07 David Martínez-Gómez , Ramón Oliver , Elena Khomenko , Manuel Collados

There has been a long-lasting debate on the question of whether or not electric currents in solar active regions are neutralized. That is, whether or not the main (or direct) coronal currents connecting the active region polarities are…

The appearance of the coronavirus (COVID-19) in late 2019 has dominated the news in the last few months as it developed into a pandemic. In many mathematics and physics classrooms, instructors are using the time series of the number of…

物理教育 · 物理学 2020-07-24 Paulo H. Acioli

Thomas-Fermi model is applied to describe some basic properties of a negative hydrogen ion in a strong electric field. The equilibrium ionic size, energy and polarizability of the ion are calculated. Collective modes of the dipole…

材料科学 · 物理学 2013-02-25 Yuri Kornyushin

A turbulent dynamo in spherical geometry with an outer corona is simulated to study the sign of magnetic helicity in the outer parts. In agreement with earlier studies, the sign in the outer corona is found to be opposite to that inside the…

太阳与恒星天体物理 · 物理学 2017-08-18 Axel Brandenburg , Mohira B. Ashurova , Sarah Jabbari