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Title: Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona

Abstract

Single-pulse, globally propagating coronal fronts, called Extreme-ultraviolet (EUV) waves, were first confirmed in 1995 by the Extreme-ultraviolet Imaging Telescope and every observed EUV wave since has been associated with a coronal mass ejection (CME). The physical mechanism underlying these waves has been debated for two decades with wave or pseudo-wave theories being advocated. We introduce a hybrid model where EUV waves are compressional fronts driven by a reverse electric current layer induced by the time-dependent CME core current. The reverse current layer flows in a direction opposite to the CME core current and is an eddy current layer necessary to maintain magnetic flux conservation above the layer. Repelled by the core current, the reverse current layer accelerates upward so it acts as a piston that drives a compressional perturbation in the coronal regions above. Given a sufficiently fast piston speed, the compressional perturbation becomes a shock that separates from the piston when the piston slows down. Since the model relates the motion of the EUV front to CME properties, the model provides a bound for the core current of an erupting CME. The model is supported and motivated by detailed results from both laboratory experiments and ideal 3D magnetohydrodynamic simulations.more » Overlaps and differences with other models and spacecraft observations are reported on.« less

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [1]
  1. California Inst. of Technology (CalTech), Pasadena, CA (United States). Applied Physics
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States). Theoretical Division
Publication Date:
Research Org.:
California Institute of Technology (CalTech), Pasadena, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
Contributing Org.:
Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
OSTI Identifier:
1574940
Grant/Contract Number:  
FG02-04ER54755
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 874; Journal Issue: 2; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; magnetohydrodynamics (MHD); methods: laboratory: atomic; methods: numerical; plasmas; Sun: coronal mass ejections (CMEs)

Citation Formats

Wongwaitayakornkul, Pakorn, Haw, Magnus A., Li, Hui, and Bellan, Paul M. Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona. United States: N. p., 2019. Web. doi:10.3847/1538-4357/ab09f2.
Wongwaitayakornkul, Pakorn, Haw, Magnus A., Li, Hui, & Bellan, Paul M. Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona. United States. https://doi.org/10.3847/1538-4357/ab09f2
Wongwaitayakornkul, Pakorn, Haw, Magnus A., Li, Hui, and Bellan, Paul M. Mon . "Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona". United States. https://doi.org/10.3847/1538-4357/ab09f2. https://www.osti.gov/servlets/purl/1574940.
@article{osti_1574940,
title = {Magnetically Induced Current Piston for Generating Extreme-ultraviolet Fronts in the Solar Corona},
author = {Wongwaitayakornkul, Pakorn and Haw, Magnus A. and Li, Hui and Bellan, Paul M.},
abstractNote = {Single-pulse, globally propagating coronal fronts, called Extreme-ultraviolet (EUV) waves, were first confirmed in 1995 by the Extreme-ultraviolet Imaging Telescope and every observed EUV wave since has been associated with a coronal mass ejection (CME). The physical mechanism underlying these waves has been debated for two decades with wave or pseudo-wave theories being advocated. We introduce a hybrid model where EUV waves are compressional fronts driven by a reverse electric current layer induced by the time-dependent CME core current. The reverse current layer flows in a direction opposite to the CME core current and is an eddy current layer necessary to maintain magnetic flux conservation above the layer. Repelled by the core current, the reverse current layer accelerates upward so it acts as a piston that drives a compressional perturbation in the coronal regions above. Given a sufficiently fast piston speed, the compressional perturbation becomes a shock that separates from the piston when the piston slows down. Since the model relates the motion of the EUV front to CME properties, the model provides a bound for the core current of an erupting CME. The model is supported and motivated by detailed results from both laboratory experiments and ideal 3D magnetohydrodynamic simulations. Overlaps and differences with other models and spacecraft observations are reported on.},
doi = {10.3847/1538-4357/ab09f2},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 874,
place = {United States},
year = {Mon Apr 01 00:00:00 EDT 2019},
month = {Mon Apr 01 00:00:00 EDT 2019}
}

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Works referenced in this record:

The Kinematics of a Globally Propagating Disturbance in the Solar Corona
journal, May 2008

  • Long, David M.; Gallagher, Peter T.; McAteer, R. T. James
  • The Astrophysical Journal, Vol. 680, Issue 1
  • DOI: 10.1086/589742

Imaging and Spectroscopic Investigations of a Solar Coronal Wave: Properties of the Wave Front and Associated Erupting Material
journal, April 2003

  • Harra, Louise K.; Sterling, Alphonse C.
  • The Astrophysical Journal, Vol. 587, Issue 1
  • DOI: 10.1086/368079

Simple magnetohydrodynamic waves
journal, February 1995


First Soft X-Ray Observations of Global Coronal Waves with the G O E S Solar X-Ray Imager
journal, May 2005

  • Warmuth, A.; Mann, G.; Aurass, H.
  • The Astrophysical Journal, Vol. 626, Issue 2
  • DOI: 10.1086/431756

Early life of coronal mass ejections
journal, November 2000


NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO
journal, October 2009


Coronal Response to an euv wave from dem Analysis
journal, October 2015


A Catalog of Coronal “eit Wave” Transients
journal, July 2009


Loop Density Enhancement by Nonlinear Magnetohydrodynamic Waves
journal, July 2004

  • Terradas, J.; Ofman, L.
  • The Astrophysical Journal, Vol. 610, Issue 1
  • DOI: 10.1086/421514

On Cylindrical Magnetohydrodynamic Shock Waves
journal, January 1961

  • Greifinger, Carl; Cole, Julian D.
  • Physics of Fluids, Vol. 4, Issue 5
  • DOI: 10.1063/1.1706358

Criteria for Scaled Laboratory Simulations of Astrophysical MHD Phenomena
journal, April 2000

  • Ryutov, D. D.; Drake, R. P.; Remington, B. A.
  • The Astrophysical Journal Supplement Series, Vol. 127, Issue 2
  • DOI: 10.1086/313320

Understanding the Physical Nature of Coronal “EIT Waves”
journal, December 2016


“EXTREME ULTRAVIOLET WAVES” ARE WAVES: FIRST QUADRATURE OBSERVATIONS OF AN EXTREME ULTRAVIOLET WAVE FROM STEREO
journal, July 2009


EIT Waves: A Changing Understanding over a Solar Cycle
journal, December 2009


Coronal "Wave": Magnetic Footprint of a Coronal Mass Ejection?
journal, January 2007

  • Attrill, Gemma D. R.; Harra, Louise K.; van Driel-Gesztelyi, Lidia
  • The Astrophysical Journal, Vol. 656, Issue 2
  • DOI: 10.1086/512854

Apex Dips of Experimental Flux Ropes: Helix or Cusp?
journal, October 2017

  • Wongwaitayakornkul, Pakorn; Haw, Magnus A.; Li, Hui
  • The Astrophysical Journal, Vol. 848, Issue 2
  • DOI: 10.3847/1538-4357/aa8990

Evidence of EIT and Moreton Waves in Numerical Simulations
journal, June 2002

  • Chen, P. F.; Wu, S. T.; Shibata, K.
  • The Astrophysical Journal, Vol. 572, Issue 1
  • DOI: 10.1086/341486

The Energetics of a Global Shock wave in the low Solar Corona
journal, January 2015


Three-Dimensional mhd Simulation of the Caltech Plasma jet Experiment: First Results
journal, July 2014


Solar Phenomena Associated with “EIT Waves”
journal, April 2002

  • Biesecker, D. A.; Myers, D. C.; Thompson, B. J.
  • The Astrophysical Journal, Vol. 569, Issue 2
  • DOI: 10.1086/339402

Cylindrical and Spherical Pistons as Drivers of MHD Shocks
journal, April 2008


A multiwavelength study of solar flare waves: II. Perturbation characteristics and physical interpretation
journal, April 2004


Plasma Beta Stratification in the Solar Atmosphere: A Possible Explanation for the Penumbra Formation
journal, November 2017


SOHO /EIT observations of an Earth-directed coronal mass ejection on May 12, 1997
journal, July 1998

  • Thompson, B. J.; Plunkett, S. P.; Gurman, J. B.
  • Geophysical Research Letters, Vol. 25, Issue 14
  • DOI: 10.1029/98GL50429

Observations and Interpretation of a low Coronal Shock wave Observed in the euv by the Sdo/Aia
journal, August 2011


The Flux‐Rope Scaling of the Acceleration of Coronal Mass Ejections and Eruptive Prominences
journal, September 2006

  • Chen, J.; Marque, C.; Vourlidas, A.
  • The Astrophysical Journal, Vol. 649, Issue 1
  • DOI: 10.1086/506466

ANALYSIS OF CHARACTERISTIC PARAMETERS OF LARGE-SCALE CORONAL WAVES OBSERVED BY THE SOLAR-TERRESTRIAL RELATIONS OBSERVATORY /EXTREME ULTRAVIOLET IMAGER
journal, September 2011


Statistical Analysis of Large-Scale EUV Waves Observed by STEREO/EUVI
journal, September 2014


Investigation of the Formation and Separation of an Extreme-Ultraviolet wave from the Expansion of a Coronal mass Ejection
journal, December 2011


Origin of Coronal Shock Waves: Invited Review
journal, July 2008


FIRST EVIDENCE OF COEXISTING EIT WAVE AND CORONAL MORETON WAVE FROM SDO /AIA OBSERVATIONS
journal, April 2011


Magnetically Driven Flows in Arched Plasma Structures
journal, August 2012


Quasiperiodic acceleration of electrons by a plasmoid-driven shock in the solar atmosphere
journal, October 2013

  • Carley, Eoin P.; Long, David M.; Byrne, Jason P.
  • Nature Physics, Vol. 9, Issue 12
  • DOI: 10.1038/nphys2767

A New Model for Propagating Parts of EIT Waves: A Current Shell in a CME
journal, November 2007


Observable Properties of the Breakout Model for Coronal Mass Ejections
journal, December 2004

  • Lynch, B. J.; Antiochos, S. K.; MacNeice, P. J.
  • The Astrophysical Journal, Vol. 617, Issue 1
  • DOI: 10.1086/424564

Are “EIT Waves” Fast‐Mode MHD Waves?
journal, July 2007

  • Wills‐Davey, M. J.; DeForest, C. E.; Stenflo, J. O.
  • The Astrophysical Journal, Vol. 664, Issue 1
  • DOI: 10.1086/519013

Laboratory demonstration of slow rise to fast acceleration of arched magnetic flux ropes: LABORATORY FLUX ROPES
journal, September 2016

  • Ha, Bao N.; Bellan, Paul M.
  • Geophysical Research Letters, Vol. 43, Issue 18
  • DOI: 10.1002/2016GL069744

Catalogue of the 1997 SOHO–EIT coronal transient waves and associated type II radio burst spectra
journal, February 2000

  • Klassen, A.; Aurass, H.; Mann, G.
  • Astronomy and Astrophysics Supplement Series, Vol. 141, Issue 3
  • DOI: 10.1051/aas:2000125

OFF-LIMB SOLAR CORONAL WAVEFRONTS FROM SDO /AIA EXTREME-ULTRAVIOLET OBSERVATIONS—IMPLICATIONS FOR PARTICLE PRODUCTION
journal, May 2011


EIT wave observations and modeling in the STEREO era
journal, June 2011


Reverse Current Model for Coronal Mass Ejection Cavity Formation
journal, July 2018

  • Haw, Magnus A.; Wongwaitayakornkul, Pakorn; Li, Hui
  • The Astrophysical Journal, Vol. 862, Issue 2
  • DOI: 10.3847/2041-8213/aad33c

Interaction of EIT Waves with Coronal Active Regions
journal, July 2002

  • Ofman, L.; Thompson, B. J.
  • The Astrophysical Journal, Vol. 574, Issue 1
  • DOI: 10.1086/340924

Three‐dimensional Model of the Structure and Evolution of Coronal Mass Ejections
journal, March 2002

  • Tokman, M.; Bellan, P. M.
  • The Astrophysical Journal, Vol. 567, Issue 2
  • DOI: 10.1086/338699

FIRST SDO AIA OBSERVATIONS OF A GLOBAL CORONAL EUV “WAVE”: MULTIPLE COMPONENTS AND “RIPPLES”
journal, October 2010


High-Cadence Observations of a Global Coronal Wave by STEREO EUVI
journal, June 2008

  • Veronig, Astrid M.; Temmer, Manuela; Vršnak, Bojan
  • The Astrophysical Journal, Vol. 681, Issue 2
  • DOI: 10.1086/590493

Plasma Physics
August 2014


A multiwavelength study of solar flare waves: I. Observations and basic properties
journal, April 2004


The Kinematics of a Globally Propagating Disturbance in the Solar Corona
text, January 2008


Quasiperiodic acceleration of electrons by a plasmoid-driven shock in the solar atmosphere
text, January 2014


Three-Dimensional MHD Simulation of Caltech Plasma Jet Experiment: First Results
text, January 2014


Statistical Analysis of Large-scale EUV Waves Observed by STEREO/EUVI
text, January 2014


The energetics of a global shock wave in the low solar corona
text, January 2014


Coronal response to an EUV wave from DEM analysis
text, January 2015


Works referencing / citing this record:

Self-similar Piston-Shock and CME
journal, September 2019