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- AMER INST PHYSICS
- ELSEVIER SCIENCE BV
- INT ATOMIC ENERGY AGENCY
- Biblioteca Digitais de Teses e Dissertações da USP
- Universidade Rice
- Facultad de Ciencias Exactas y Naturales. Universidad de Buenos Aires
- Elsevier
- Universidade Cornell
- American Astronomical Society
- Instituto de Astronomía, UNAM
- Mais Publicadores...

## Escape patterns of chaotic magnetic field lines in a tokamak with reversed magnetic shear and an ergodic limiter

Fonte: AMER INST PHYSICS
Publicador: AMER INST PHYSICS

Tipo: Artigo de Revista Científica

ENG

Relevância na Pesquisa

65.95%

#PRESERVING NONTWIST MAPS#TORE-SUPRA#STOCHASTIC BOUNDARIES#HAMILTONIAN-DYNAMICS#ENHANCED CONFINEMENT#HOMOCLINIC TANGLES#POLOIDAL DIVERTOR#TRANSPORT#PLASMA#TEXTOR#Physics, Fluids & Plasmas

The existence of a reversed magnetic shear in tokamaks improves the plasma confinement through the formation of internal transport barriers that reduce radial particle and heat transport. However, the transport poloidal profile is much influenced by the presence of chaotic magnetic field lines at the plasma edge caused by external perturbations. Contrary to many expectations, it has been observed that such a chaotic region does not uniformize heat and particle deposition on the inner tokamak wall. The deposition is characterized instead by structured patterns called magnetic footprints, here investigated for a nonmonotonic analytical plasma equilibrium perturbed by an ergodic limiter. The magnetic footprints appear due to the underlying mathematical skeleton of chaotic magnetic field lines determined by the manifold tangles. For the investigated edge safety factor ranges, these effects on the wall are associated with the field line stickiness and escape channels due to internal island chains near the flux surfaces. Comparisons between magnetic footprints and escape basins from different equilibrium and ergodic limiter characteristic parameters show that highly concentrated magnetic footprints can be avoided by properly choosing these parameters. (c) 2008 American Institute of Physics.; FAPESP (Sao Paulo); Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES); CNPq; Fundacao Araucaria (Parana)

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## Transport control in fusion plasmas by changing electric and magnetic field spatial profiles

Fonte: ELSEVIER SCIENCE BV
Publicador: ELSEVIER SCIENCE BV

Tipo: Artigo de Revista Científica

ENG

Relevância na Pesquisa

85.95%

#Plasma physics#Magnetic field lines#Tokamaks#ERGODIC DIVERTOR#DRIFT WAVES#TORE-SUPRA#TOKAMAK#EDGE#STOCHASTICITY#CONFINEMENT#OPERATION

For magnetically confined plasmas in tokamaks, we have numerically investigated how Lagrangian chaos at the plasma edge affects the plasma confinement. Initially, we have considered the chaotic motion of particles in an equilibrium electric field with a monotonic radial profile perturbed by drift waves. We have showed that an effective transport barrier may be created at the plasma edge by modifying the electric field radial profile. In the second place, we have obtained escape patterns and magnetic footprints of chaotic magnetic field lines in the region near a tokamak wall with resonant modes due to the action of an ergodic magnetic limiter. For monotonic plasma current density profiles we have obtained distributions of field line connections to the wall and line escape channels with the same spatial pattern as the magnetic footprints on the tokamak walls. (c) 2008 Elsevier B.V. All rights reserved.

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## Chaotic transport in reversed shear tokamaks

Fonte: INT ATOMIC ENERGY AGENCY
Publicador: INT ATOMIC ENERGY AGENCY

Tipo: Artigo de Revista Científica

ENG

Relevância na Pesquisa

65.92%

#MAGNETIC-FIELD LINES#SCRAPE-OFF LAYER#ERGODIC DIVERTOR#HOMOCLINIC TANGLES#DRIFT WAVES#CONFINEMENT#DYNAMICS#PLASMAS#PERTURBATIONS#STOCHASTICITY#Physics, Fluids & Plasmas

For tokamak models using simplified geometries and reversed shear plasma profiles, we have numerically investigated how the onset of Lagrangian chaos at the plasma edge may affect the plasma confinement in two distinct but closely related problems. Firstly, we have considered the motion of particles in drift waves in the presence of an equilibrium radial electric field with shear. We have shown that the radial particle transport caused by this motion is selective in phase space, being determined by the resonant drift waves and depending on the parameters of both the resonant waves and the electric field profile. Moreover, we have shown that an additional transport barrier may be created at the plasma edge by increasing the electric field. In the second place, we have studied escape patterns and magnetic footprints of chaotic magnetic field lines in the region near a tokamak wall, when there are resonant modes due to the action of an ergodic magnetic limiter. A non-monotonic safety factor profile has been used in the analysis of field line topology in a region of negative magnetic shear. We have observed that, if internal modes are perturbed, the distributions of field line connection lengths and magnetic footprints exhibit spatially localized escape channels. For typical physical parameters of a fusion plasma...

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## Plasma confinement in tokamaks with robust torus

Fonte: ELSEVIER SCIENCE BV
Publicador: ELSEVIER SCIENCE BV

Tipo: Artigo de Revista Científica

ENG

Relevância na Pesquisa

65.95%

#Robust tori#Transport barriers#Chaos#Non-linear map#Hamiltonian system#MAGNETIC-FIELD LINES#TOROIDAL GEOMETRY#TRANSPORT#SHEAR#RESONANCES#OPERATION

We present a non-linear symplectic map that describes the alterations of the magnetic field lines inside the tokamak plasma due to the presence of a robust torus (RT) at the plasma edge. This RT prevents the magnetic field lines from reaching the tokamak wall and reduces, in its vicinity, the islands and invariant curve destruction due to resonant perturbations. The map describes the equilibrium magnetic field lines perturbed by resonances created by ergodic magnetic limiters (EMLs). We present the results obtained for twist and non-twist mappings derived for monotonic and non-monotonic plasma current density radial profiles, respectively. Our results indicate that the RT implementation would decrease the field line transport at the tokamak plasma edge. (C) 2010 Elsevier B.V. All rights reserved.; FAPESP; Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP); Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq); CNPQ; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES); CAPES

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## Estudo de instalações de linhas subterrâneas de alta tensão com relação a campos magnéticos.; Study of installations of high voltage underground lines with regard to magnetic field.

Fonte: Biblioteca Digitais de Teses e Dissertações da USP
Publicador: Biblioteca Digitais de Teses e Dissertações da USP

Tipo: Dissertação de Mestrado
Formato: application/pdf

Publicado em 09/08/2010
PT

Relevância na Pesquisa

66.08%

#Cabos elétricos#Campo magnético#Electric cables#Linhas subterrâneas de transmissão de energia elétrica#Magnetic field#Underground electrical power transmission lines

Atualmente, a intensidade de campo elétrico, campo magnético e campo eletromagnético é um fator determinante não só para a implantação de novas instalações, mas também, para as instalações existentes no sistema elétrico. Apesar de não existir nenhum estudo conclusivo que comprove a evidência direta entre a exposição a estes campos e os efeitos nocivos na saúde das pessoas, muitos países, inclusive o Brasil, definiram em suas legislações limites básicos à exposição de campos elétrico e magnético provenientes dos sistemas elétricos. Este trabalho tem como objetivo contribuir para análise de campo magnético de linhas subterrâneas de alta tensão existentes ou linhas em fase inicial de projeto, visando atender os limites de exposição vigentes na legislação local. Nele é apresentada a metodologia de cálculo de campo magnético baseada na Lei de Biot-Savart e no princípio da superposição. Estudos analíticos para verificação da influência dos parâmetros de instalação e elétricos de linhas sobre o campo magnético são apresentados para linhas subterrâneas de alta tensão compostas por um e dois circuitos com diferentes tipos de instalação e aterramentos. Comparações entre valores analíticos e valores de medições de campo magnético de linhas subterrâneas de alta tensão existentes em operação também são abordadas neste trabalho. As principais técnicas de mitigação de campo magnético utilizadas em linhas subterrâneas de alta tensão...

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## PARALLEL ELECTRIC FIELD ON AURORAL MAGNETIC FIELD LINES

Fonte: Universidade Rice
Publicador: Universidade Rice

Tipo: Thesis; Text
Formato: application/pdf

ENG

Relevância na Pesquisa

66%

The interaction of Birkeland (magnetic-field-aligned) current carriers and the Earth's magnetic field results in electrostatic potential drops along magnetic field lines. The statistical distributions of the field-aligned potential difference (phi)(,(PARLL)) were determined from the energy spectra of electron inverted "V" events observed at ionospheric altitude for different conditions of geomagnetic activity as indicated by the AE index. Data of 1270 electron inverted "V"'s were obtained from Low-Energy Electron measurements of the Atmosphere Explorer-C and -D Satellite (despun mode) in the interval January 1974-April 1976.
In general, (phi)(,(PARLL)) is largest in the dusk to pre-midnight sector, smaller in the post-midnight to dawn sector, and smallest in the near noon sector during quiet and disturbed geomagnetic conditions; there is a steady dusk-dawn-noon asymmetry of the global (phi)(,(PARLL)) distribution. As the geomagnetic activity level increases, the (phi)(,(PARLL)) pattern expands to lower invariant latitudes, and the magnitude of (phi)(,(PARLL)) in the 13-24 magnetic local time sector increases significantly. The spatial structure and intensity variation of the global (phi)(,(PARLL)) distribution are statistically more variable...

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## Las fulguraciones solares como manifestación de reconexión magnética; Solar flares as a manifestation of magnetic reconnection

Fonte: Facultad de Ciencias Exactas y Naturales. Universidad de Buenos Aires
Publicador: Facultad de Ciencias Exactas y Naturales. Universidad de Buenos Aires

Tipo: info:eu-repo/semantics/doctoralThesis; tesis doctoral; info:eu-repo/semantics/publishedVersion
Formato: application/pdf

Publicado em //1997
SPA

Relevância na Pesquisa

56.02%

#SOLAR PHYSICS#SOLAR FLARES#ASTROPHYSYCAL PLASMAS#MAGNETIC RECONNECTION#MAGNETIC FIELD TOPOLOGY#IMAGE PROCESSING AND ANALYSIS OF ASTRONOMICAL DATA#FISICA SOLAR#FULGURACIONES SOLARES#PLASMAS ASTROFISICOS#RECONEXION MAGNETICA#TOPOLOGIA DEL CAMPO MAGNETICO

Se acepta generalmente que el campo magnético juega un rol fundamental en la física del Sol y de otros objetos astrofísicos, confinando el plasma y acumulando enormes cantidades de energia que luego será liberada en los llamados eventos catastróficos. Las fulguraciones solares son fenómenos que nos brindan una gran oportunidad para comprender cómo actúa el campo magnético durante estos eventos. La comparación entre las manifestaciones de estos fenómenos impulsivos y el modelado del campo magnético de la región activa donde tuvieron lugar, es uno de los tópicos fundamentales de la física solar. Este trabajo nos lleva a analizar las diferentes señales de la actividad de la fulguración, usando observaciones simultáneas en un amplio rango del espectro electromagnético como rayos X, ultravioleta (UV), y diferentes lineas espectrales en el visible, así como magnetogramas vectoriales. Para entender las condiciones que conducen a una dada región activa a producir una fulguración, hemos considerado en esta Tesis el modelado del campo magnético, analizando luego la relación entre su topología y las emisiones radiativas en las diferentes regiones espectrales. La visión convencional de la reconexión magnética está basada principalmente en el estudio en dos dimensiones (2-D) de un punto neutro del tipo X...

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## Algorithms for real time magnetic field tracing and optimization

Fonte: Elsevier
Publicador: Elsevier

Tipo: Artigo de Revista Científica

Relevância na Pesquisa

75.81%

#Keywords: Algorithms#Interpolation#Optimization#Perturbation techniques#Simulated annealing#Surface properties#Vacuum#Magnetic field tracing#Magnetic fields Field line tracing#Fusion#Magnetic coil design

We describe algorithms for tracing vacuum magnetic field lines in complex geometries at interactive speeds (∼50,000 steps/s on a personal computer), and a post-processing perturbation method for optimization of magnetic surface properties. Algorithms in

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## Confinement Efficiency and Stability of a Toroidal Magnetized Plasma Device with Sheared Magnetic Field Lines using an Internal Ring Conductor

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Relevância na Pesquisa

65.86%

In a new toroidal laboratory plasma device including a poloidal magnetic
field created by an internal circular conductor, the confinement efficiency of
the magnetized plasma and the turbulence level are studied in different
situations. The plasma density is greatly enhanced when a sufficient poloidal
magnetic field is established. Moreover, the instabilities and the turbulence
usually found in toroidal devices without shear of the magnetic field lines are
suppressed when the rotational transform is present. The measurement of the
plasma decay time allows to determine the confinement time of the particles
which is compared to the Bohm diffusion time and to the value predicted by
different diffusion models, especially the neoclassical diffusion.; Comment: 3 figures

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## Study of the interplay between magnetic shear and resonances using Hamiltonian models for the magnetic field lines

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Publicado em 18/03/2011

Relevância na Pesquisa

65.99%

The issue of magnetic confinement in magnetic fusion devices is addressed
within a purely magnetic approach. Using some Hamiltonian models for the
magnetic field lines, the dual impact of low magnetic shear is shown in a
unified way. Away from resonances, it induces a drastic enhancement of magnetic
confinement that favors robust internal transport barriers (ITBs) and
stochastic transport reduction. When low-shear occurs for values of the winding
of the magnetic field lines close to low-order rationals, the amplitude
thresholds of the resonant modes that break internal transport barriers by
allowing a radial stochastic transport of the magnetic field lines may be quite
low. The approach can be applied to assess the robustness versus magnetic
perturbations of general (almost) integrable magnetic steady states, including
non-axisymmetric ones such as the important single helicity steady states. This
analysis puts a constraint on the tolerable mode amplitudes compatible with
ITBs and may be proposed as a possible explanation of diverse experimental and
numerical signatures of their collapses.

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## Compressible dynamics of magnetic field lines for incompressible MHD flows

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Publicado em 01/10/2003

Relevância na Pesquisa

65.9%

It is demonstrated that the deformation of magnetic field lines in
incompressible magnetohydrodynamic flows results from a compressible mapping.
Appearance of zeroes for the mapping Jacobian correspond to the breaking of
magnetic field lines, associated with local blowup of the magnetic field. The
possibility of such events is found to be unlikely in two dimensions but not in
three dimensions.; Comment: 13 pages

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## On the significance of polarization charge and isomagnetic surface in the interaction between conducting fluid and magnetic field

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Relevância na Pesquisa

56.04%

From the frozen-in field lines concept, a highly conducting fluid can move
freely along, but not traverse to, magnetic field lines. We discuss this topic
and find that in the study of the frozen-in field lines concept, the effects of
inductive and capacitive reactance have been omitted. When admitted, the
relationships among the motional electromotive field, the induced electric
field, the eddy electric current, and the magnetic field becomes clearer and
the frozen-in field line concept can be reconsidered. We emphasize the
importance of isomagnetic surfaces and polarization charges, and show
analytically that whether a conducting fluid can freely traverse magnetic field
lines or not depends solely on the magnetic gradient in the direction of fluid
motion. If a fluid does not change its density distribution and shape (can be
regarded as a quasi-rigid body), and as long as it is moving along an
isomagnetic surface, it can freely traverse magnetic field lines without any
magnetic resistance no matter how strong the magnetic field is. When our
analysis is applied, the origin of the magnetic field of sunspots can be
interpreted easily. In addition, we also present experimental results to
support our analysis.; Comment: 12 pages, 12 figures...

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## Coronal heating through braiding of magnetic field lines

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Publicado em 21/09/2004

Relevância na Pesquisa

65.82%

Cool stars like our Sun are surrounded by a million degree hot outer
atmosphere, the corona. Since more than 60 years the physical nature of the
processes heating the corona to temperatures well in excess of those on the
stellar surface remain puzzling. Recent progress in observational techniques
and numerical modeling now opens a new window to approach this problem. We
present the first coronal emission line spectra synthesized from
three-dimensional numerical models describing the evolution of the dynamics and
energetics as well as of the magnetic field in the corona. In these models the
corona is heated through motions on the stellar surface that lead to a braiding
of magnetic field lines inducing currents which are finally dissipated. These
forward models enable us to synthesize observed properties like (average)
emission line Doppler shifts or emission measures in the outer atmosphere,
which until now have not been understood theoretically, even though many
suggestions have been made in the past. As our model passes these observational
tests, we conclude that the flux braiding mechanism is a prime candidate for
being the dominant heating process of the magnetically closed corona of the Sun
and solar-like stars.; Comment: 4 pages...

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## Asymmetric Diffusion of Magnetic Field Lines

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Publicado em 13/03/2013

Relevância na Pesquisa

65.96%

#Astrophysics - High Energy Astrophysical Phenomena#Astrophysics - Astrophysics of Galaxies#Astrophysics - Solar and Stellar Astrophysics

Stochasticity of magnetic field lines is important for particle transport
properties. Magnetic field lines separate faster than diffusively in turbulent
plasma, which is called superdiffusion. We discovered that this superdiffusion
is pronouncedly asymmetric, so that the separation of field lines along the
magnetic field direction is different from the separation in the opposite
direction. While the symmetry of the flow is broken by the so-called imbalance
or cross-helicity, the difference between forward and backward diffusion is not
directly due to imbalance, but a non-trivial consequence of both imbalance and
non-reversibility of turbulence. The asymmetric diffusion perpendicular to the
mean magnetic field entails a variety of new physical phenomena, such as the
production of parallel particle streaming in the presence of perpendicular
particle gradients. Such streaming and associated instabilities could be
significant for particle transport in laboratory, space and astrophysical
plasmas.; Comment: 4 pages 3 figures

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## Acceleration of charged particles due to chaotic scattering in the combined black hole gravitational field and asymptotically uniform magnetic field

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Publicado em 09/11/2015

Relevância na Pesquisa

56.02%

To test the role of large-scale magnetic fields in accretion processes, we
study dynamics of charged test particles in vicinity of a black hole immersed
into an asymptotically uniform magnetic field. Using the Hamiltonian formalism
of charged particle dynamics, we examine chaotic scattering in the effective
potential related to the black hole gravitational field combined with the
uniform magnetic field. Energy interchange between the translational and
oscillatory modes od the charged particle dynamics provides mechanism for
charged particle acceleration along the magnetic field lines. This energy
transmutation is an attribute of the chaotic charged particle dynamics in the
combined gravitational and magnetic fields only, the black hole rotation is not
necessary for such charged particle acceleration. The chaotic scatter can cause
transition to the motion along the magnetic field lines with small radius of
the Larmor motion or vanishing Larmor radius, when the speed of the particle
translational motion is largest and can be ultra-relativistic. We discuss
consequences of the model of ionization of test particles forming a neutral
accretion disc, or heavy ions following off-equatorial circular orbits, and we
explore the fate of heavy charged test particles after ionization where no kick
of heavy ions is assumed and only switch-on effect of the magnetic field is
relevant. We demonstrate that acceleration and escape of the ionized particles
can be efficient along the Kerr black hole symmetry axis parallel to the
magnetic field lines. We show that strong acceleration of ionized particles to
ultra-relativistic velocities is preferred in the direction close to the
magnetic field lines. Therefore...

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## How to use magnetic field information for coronal loop identification?

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Publicado em 30/01/2008

Relevância na Pesquisa

56.03%

The structure of the solar corona is dominated by the magnetic field because
the magnetic pressure is about four orders of magnitude higher than the plasma
pressure. Due to the high conductivity the emitting coronal plasma (visible
e.g. in SOHO/EIT) outlines the magnetic field lines. The gradient of the
emitting plasma structures is significantly lower parallel to the magnetic
field lines than in the perpendicular direction. Consequently information
regarding the coronal magnetic field can be used for the interpretation of
coronal plasma structures. We extrapolate the coronal magnetic field from
photospheric magnetic field measurements into the corona. The extrapolation
method depends on assumptions regarding coronal currents, e.g. potential fields
(current free) or force-free fields (current parallel to magnetic field). As a
next step we project the reconstructed 3D magnetic field lines on an EIT-image
and compare with the emitting plasma structures. Coronal loops are identified
as closed magnetic field lines with a high emissivity in EIT and a small
gradient of the emissivity along the magnetic field.; Comment: 14 pages, 3 figures

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## Observation of magnetic field lines in the vicinity of a superconductor with the naked eye

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Relevância na Pesquisa

65.82%

Meissner effect and pinning effect are clearly observed with the naked eye. A
GdBaCuO high-temperature superconductor (HTS) disk fabricated by Nippon Steel
Corporation, a 100mm cubic NdFeB sintered magnet, and iron wires coated by
colored are used. When the HTS is put in the magnetic field of the magnet, it
can be observed by the wires that the magnetic field lines are excluded from
the superconductor (Meissner effect) as well as are pinned in the
superconductor (pinning effect).; Comment: 14 pages, 13 figures
http://www.sci-museum.kita.osaka.jp/~saito/superconduct.html

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## The covariant description of electric and magnetic field lines of null fields: application to Hopf-Ranada solutions

Fonte: Universidade Cornell
Publicador: Universidade Cornell

Tipo: Artigo de Revista Científica

Relevância na Pesquisa

66.01%

The concept of electric and magnetic field lines is intrinsically
non-relativistic. Nonetheless, for certain types of fields satisfying certain
geometric properties, field lines can be defined covariantly. More precisely,
two Lorentz-invariant 2D surfaces in spacetime can be defined such that
magnetic and electric field lines are determined, for any observer, by the
intersection of those surfaces with spacelike hyperplanes. An instance of this
type of field is constituted by the so-called Hopf-Ranada solutions of the
source-free Maxwell equations, which have been studied because of their
interesting topological properties, namely, linkage of their field lines. In
order to describe both geometric and topological properties in a succinct
manner, we employ the tools of Geometric Algebra (aka Clifford Algebra) and use
the Clebsch representation for the vector potential as well as the Euler
representation for both magnetic and electric fields. This description is
easily made covariant, thus allowing us to define electric and magnetic field
lines covariantly in a compact geometric language. The definitions of field
lines can be phrased in terms of 2D surfaces in space. We display those
surfaces in different reference frames, showing how those surfaces change under
Lorentz transformations while keeping their topological properties. As a
byproduct we also obtain relations between optical helicity...

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## Evidence of Confinement of Solar-energetic Particles to Interplanetary Magnetic Field Lines

Fonte: American Astronomical Society
Publicador: American Astronomical Society

Tipo: Article; PeerReviewed
Formato: application/pdf

Publicado em 10/02/2011

Relevância na Pesquisa

65.94%

We present new observations of solar-energetic particles (SEPs) associated with impulsive solar flares that show
evidence for their confinement to interplanetary magnetic field lines. Some SEP events exhibit intermittent intensity
dropouts becausemagnetic field lines filledwith and empty of particle flux mix together. The edges of these dropouts
are observed to be very sharp, suggesting that particles cannot easily move from a filled to an empty field line in
the time available during their transport from the Sun. In this paper, we perform high time-resolution observations
of intensity fall-off at the edges of observed SEP dropouts in order to look for signatures of particle motion off
field lines. However, the statistical study is dominated by one particularly intense event. The inferred length scale
of the intensity decay is comparable to the gyroradii of the particles, suggesting that particles only rarely scatter off magnetic field lines during interplanetary transport.

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## The Parker instability in axisymmetric filaments: final equilibria with longitudinal magnetic field

Fonte: Instituto de Astronomía, UNAM
Publicador: Instituto de Astronomía, UNAM

Tipo: Artigo de Revista Científica
Formato: text/html

Publicado em 01/04/2011
EN

Relevância na Pesquisa

65.91%

We study the final equilibrium states of the Parker instability arising from an initially unstable cylindrical equilibrium configuration of gas in the presence of a radial gravitational field and a longitudinal magnetic field. The aim of this work is to compare the properties of the nonlinear final equilibria with those found in a system with Cartesian geometry. Maps of the density and magnetic field lines, when the strength of the gravitational field is constant, are given in both geometries. We find that the magnetic buoyancy and the drainage of gas along field lines are less efficient under axial symmetry than in a Cartesian atmosphere. As a consequence, the column density enhancement arising in gas condensations in the axially-symmetric model is smaller than in a Cartesian geometry. The magnetic-to-gas pressure ratio in the final equilibrium state takes more extreme values in the Cartesian model. Models with non-uniform radial gravity are also discussed.

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