EVOLUTION OF FAST MAGNETOACOUSTIC PULSES IN RANDOMLY STRUCTURED CORONAL PLASMAS
Abstract
We investigate the evolution of fast magnetoacoustic pulses in randomly structured plasmas, in the context of largescale propagating waves in the solar atmosphere. We perform onedimensional numerical simulations of fast wave pulses propagating perpendicular to a constant magnetic field in a lowβ plasma with a random density profile across the field. Both linear and nonlinear regimes are considered. We study how the evolution of the pulse amplitude and width depends on their initial values and the parameters of the random structuring. Acting as a dispersive medium, a randomly structured plasma causes amplitude attenuation and width broadening of the fast wave pulses. After the passage of the main pulse, secondary propagating and standing fast waves appear. Width evolution of both linear and nonlinear pulses can be well approximated by linear functions; however, narrow pulses may have zero or negative broadening. This arises because narrow pulses are prone to splitting, while broad pulses usually deviate less from their initial Gaussian shape and form ripple structures on top of the main pulse. Linear pulses decay at an almost constant rate, while nonlinear pulses decay exponentially. A pulse interacts most efficiently with a random medium with a correlation length of about half of themore »
 Authors:
 Shandong Provincial Key Laboratory of Optical Astronomy and SolarTerrestrial Environment, Institute of Space Sciences, Shandong University, Weihai 264209 (China)
 Centre for Fusion, Space and Astrophysics, Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom)
 Centre for mathematical Plasma Astrophysics, Department of Mathematics, KU Leuven, Celestijnenlaan 200B bus 2400, B3001 Leuven (Belgium)
 Publication Date:
 OSTI Identifier:
 22364306
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Astrophysical Journal; Journal Volume: 799; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; AMPLITUDES; APPROXIMATIONS; ATTENUATION; COMPUTERIZED SIMULATION; CORRELATIONS; MAGNETIC FIELDS; MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; OSCILLATIONS; PLASMA; PULSES; RANDOMNESS; SOLAR ATMOSPHERE; STAR EVOLUTION; SUN; WAVE PROPAGATION
Citation Formats
Yuan, D., Li, B., Pascoe, D. J., Nakariakov, V. M., and Keppens, R., Email: Ding.Yuan@wis.kuleuven.be, Email: bbl@sdu.edu.cn. EVOLUTION OF FAST MAGNETOACOUSTIC PULSES IN RANDOMLY STRUCTURED CORONAL PLASMAS. United States: N. p., 2015.
Web. doi:10.1088/0004637X/799/2/221.
Yuan, D., Li, B., Pascoe, D. J., Nakariakov, V. M., & Keppens, R., Email: Ding.Yuan@wis.kuleuven.be, Email: bbl@sdu.edu.cn. EVOLUTION OF FAST MAGNETOACOUSTIC PULSES IN RANDOMLY STRUCTURED CORONAL PLASMAS. United States. doi:10.1088/0004637X/799/2/221.
Yuan, D., Li, B., Pascoe, D. J., Nakariakov, V. M., and Keppens, R., Email: Ding.Yuan@wis.kuleuven.be, Email: bbl@sdu.edu.cn. 2015.
"EVOLUTION OF FAST MAGNETOACOUSTIC PULSES IN RANDOMLY STRUCTURED CORONAL PLASMAS". United States.
doi:10.1088/0004637X/799/2/221.
@article{osti_22364306,
title = {EVOLUTION OF FAST MAGNETOACOUSTIC PULSES IN RANDOMLY STRUCTURED CORONAL PLASMAS},
author = {Yuan, D. and Li, B. and Pascoe, D. J. and Nakariakov, V. M. and Keppens, R., Email: Ding.Yuan@wis.kuleuven.be, Email: bbl@sdu.edu.cn},
abstractNote = {We investigate the evolution of fast magnetoacoustic pulses in randomly structured plasmas, in the context of largescale propagating waves in the solar atmosphere. We perform onedimensional numerical simulations of fast wave pulses propagating perpendicular to a constant magnetic field in a lowβ plasma with a random density profile across the field. Both linear and nonlinear regimes are considered. We study how the evolution of the pulse amplitude and width depends on their initial values and the parameters of the random structuring. Acting as a dispersive medium, a randomly structured plasma causes amplitude attenuation and width broadening of the fast wave pulses. After the passage of the main pulse, secondary propagating and standing fast waves appear. Width evolution of both linear and nonlinear pulses can be well approximated by linear functions; however, narrow pulses may have zero or negative broadening. This arises because narrow pulses are prone to splitting, while broad pulses usually deviate less from their initial Gaussian shape and form ripple structures on top of the main pulse. Linear pulses decay at an almost constant rate, while nonlinear pulses decay exponentially. A pulse interacts most efficiently with a random medium with a correlation length of about half of the initial pulse width. This detailed model of fast wave pulses propagating in highly structured media substantiates the interpretation of EIT waves as fast magnetoacoustic waves. Evolution of a fast pulse provides us with a novel method to diagnose the subresolution filamentation of the solar atmosphere.},
doi = {10.1088/0004637X/799/2/221},
journal = {Astrophysical Journal},
number = 2,
volume = 799,
place = {United States},
year = 2015,
month = 2
}

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