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Abstract:

The acceleration of charged particles is relevant to the solar corona over a broad range of scales and energies. High-energy particles are usually detected in concomitance with large energy release events like solar eruptions and flares. Nevertheless, acceleration can occur at smaller scales, characterized by dynamical activity near current sheets. To gain insight into the complex scenario of coronal charged particle acceleration, we investigate the properties of acceleration with a test-particle approach using three-dimensional magnetohydrodynamic (MHD) models. These are obtained from direct solutions of the reduced MHD equations, well suited for a plasma embedded in a strong axial magnetic field, relevant to the inner heliosphere. A multi-box, multiscale technique is used to solve the equations of motion for protons. This method allows us to resolve an extended range of scales present in the system, namely, from the ion inertial scale of the order of a meter up to macroscopic scales of the order of 10 km (1/100th of the outer scale of the system). This new technique is useful to identify the mechanisms that, acting at different scales, are responsible for acceleration to high energies of a small fraction of the particles in the coronal plasma. We report results that describe acceleration at different stages over a broad range of time, length, and energy scales. © 2014. The American Astronomical Society. All rights reserved.

Registro:

Documento: Artículo
Título:Test-particle acceleration in a hierarchical three-dimensional turbulence model
Autor:Dalena, S.; Rappazzo, A.F.; Dmitruk, P.; Greco, A.; Matthaeus, W.H.
Filiación:Bartol Research Institute, Department of Physics and Astronomy, University of Delaware, DE 19716, United States
Dipartimento di Fisica, Università della Calabria, I-87036 Cosenza, Italy
Departamento de Fisica, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, 1428 Buenos Aires, Argentina
Palabras clave:acceleration of particles; magnetic reconnection; Sun: corona; turbulence
Año:2014
Volumen:783
Número:2
DOI: http://dx.doi.org/10.1088/0004-637X/783/2/143
Título revista:Astrophysical Journal
Título revista abreviado:Astrophys. J.
ISSN:0004637X
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v783_n2_p_Dalena

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Citas:

---------- APA ----------
Dalena, S., Rappazzo, A.F., Dmitruk, P., Greco, A. & Matthaeus, W.H. (2014) . Test-particle acceleration in a hierarchical three-dimensional turbulence model. Astrophysical Journal, 783(2).
http://dx.doi.org/10.1088/0004-637X/783/2/143
---------- CHICAGO ----------
Dalena, S., Rappazzo, A.F., Dmitruk, P., Greco, A., Matthaeus, W.H. "Test-particle acceleration in a hierarchical three-dimensional turbulence model" . Astrophysical Journal 783, no. 2 (2014).
http://dx.doi.org/10.1088/0004-637X/783/2/143
---------- MLA ----------
Dalena, S., Rappazzo, A.F., Dmitruk, P., Greco, A., Matthaeus, W.H. "Test-particle acceleration in a hierarchical three-dimensional turbulence model" . Astrophysical Journal, vol. 783, no. 2, 2014.
http://dx.doi.org/10.1088/0004-637X/783/2/143
---------- VANCOUVER ----------
Dalena, S., Rappazzo, A.F., Dmitruk, P., Greco, A., Matthaeus, W.H. Test-particle acceleration in a hierarchical three-dimensional turbulence model. Astrophys. J. 2014;783(2).
http://dx.doi.org/10.1088/0004-637X/783/2/143