Fast plasmoid-mediated reconnection in a solar flare
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E. Priest | C. Jiang | Z. Xue | Xiaoli Yan | D. Kong | B. Kliem | Liheng Yang | Yongliang Song | Jincheng Wang | Zhong Liu | Xueshang Feng
[1] E. Priest,et al. Three-dimensional magnetic reconnection in astrophysical plasmas , 2021, Proceedings of the Royal Society A.
[2] L. Glesener,et al. Electron Acceleration during Macroscale Magnetic Reconnection. , 2021, Physical review letters.
[3] A. Warmuth,et al. Thermal-nonthermal energy partition in solar flares derived from X-ray, EUV, and bolometric observations , 2020, Astronomy & Astrophysics.
[4] B. Pontieu,et al. Observations and Modeling of the Onset of Fast Reconnection in the Solar Transition Region , 2020, The Astrophysical Journal.
[5] D. Gary,et al. Magnetic Reconnection during the Post-impulsive Phase of a Long-duration Solar Flare: Bidirectional Outflows as a Cause of Microwave and X-Ray Bursts , 2020, The Astrophysical Journal.
[6] A. Lazarian,et al. Onset of Turbulent Fast Magnetic Reconnection Observed in the Solar Atmosphere , 2020, The Astrophysical Journal.
[7] P. Judge,et al. Spectropolarimetric Insight into Plasma Sheet Dynamics of a Solar Flare , 2019, The Astrophysical Journal.
[8] Peter R. Young,et al. CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines , 2019, The Astrophysical Journal Supplement Series.
[9] A. Veronig,et al. The birth of a coronal mass ejection , 2018, Science Advances.
[10] E. Priest,et al. Evidence for Downflows in the Narrow Plasma Sheet of 2017 September 10 and Their Significance for Flare Reconnection , 2018, The Astrophysical Journal.
[11] X. Cheng,et al. Observations of Turbulent Magnetic Reconnection within a Solar Current Sheet , 2018, The Astrophysical Journal.
[12] C. Russell,et al. Electron magnetic reconnection without ion coupling in Earth’s turbulent magnetosheath , 2018, Nature.
[13] Lu Yang,et al. Simultaneous Observation of a Flux Rope Eruption and Magnetic Reconnection during an X-class Solar Flare , 2018, 1801.02738.
[14] Q. Hu,et al. Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with a Homologous X-shaped Flare , 2017, 1710.02775.
[15] Z. Xue,et al. Observing Formation of Flux Rope by Tether-cutting Reconnection in the Sun , 2017 .
[16] Y. Kawabata,et al. Non-potential Field Formation in the X-shaped Quadrupole Magnetic Field Configuration , 2017, 1705.02560.
[17] W. Fisher,et al. Rationale and Methods , 2016 .
[18] Zhong Liu,et al. High resolution reconstruction of solar prominence images observed by the New Vacuum Solar Telescope , 2016 .
[19] Yuming Wang,et al. Investigating Energetic X-Shaped Flares on the Outskirts of A Solar Active Region , 2016, Scientific Reports.
[20] Kai Yang,et al. Observing the release of twist by magnetic reconnection in a solar filament eruption , 2016, Nature Communications.
[21] S. Wu,et al. Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption , 2016, Nature Communications.
[22] Jun Zhang,et al. Magnetic reconnection between a solar filament and nearby coronal loops , 2016, Nature Physics.
[23] J. B. Blake,et al. Electron-scale measurements of magnetic reconnection in space , 2016, Science.
[24] D. Innes,et al. IRIS Si iv LINE PROFILES: AN INDICATION FOR THE PLASMOID INSTABILITY DURING SMALL-SCALE MAGNETIC RECONNECTION ON THE SUN , 2015, 1509.08837.
[25] X. Cheng,et al. Extreme ultraviolet imaging of three-dimensional magnetic reconnection in a solar eruption , 2015, Nature Communications.
[26] B. Kliem,et al. FAST MAGNETIC RECONNECTION IN THE SOLAR CHROMOSPHERE MEDIATED BY THE PLASMOID INSTABILITY , 2015, 1509.06895.
[27] Jun Zhang,et al. MAGNETIC RECONNECTION BETWEEN SMALL-SCALE LOOPS OBSERVED WITH THE NEW VACUUM SOLAR TELESCOPE , 2014, 1412.1314.
[28] Bin Chen,et al. IMAGING AND SPECTROSCOPIC OBSERVATIONS OF MAGNETIC RECONNECTION AND CHROMOSPHERIC EVAPORATION IN A SOLAR FLARE , 2014, 1411.2301.
[29] J. T. Hoeksema,et al. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches , 2014, 1404.1879.
[30] Bo Zhang,et al. New vacuum solar telescope and observations with high resolution , 2014, 1403.6896.
[31] Y. Liu,et al. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Optimization of the Spectral Line Inversion Code , 2014, Solar Physics.
[32] R. Centeno,et al. The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Optimization of the Spectral Line Inversion Code , 2014, 1403.3677.
[33] S. Krucker,et al. PARTICLE DENSITIES WITHIN THE ACCELERATION REGION OF A SOLAR FLARE , 2013 .
[34] Yang Liu,et al. Horizontal Flows in the Photosphere and Subphotosphere of Two Active Regions , 2013 .
[35] Xudong Sun,et al. On the Coordinate System of Space-Weather HMI Active Region Patches (SHARPs): A Technical Note , 2013, 1309.2392.
[36] M. Temmer,et al. Imaging coronal magnetic-field reconnection in a solar flare , 2013, Nature Physics.
[37] C. J. Wolfson,et al. Design and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO) , 2012 .
[38] Kazunari Shibata,et al. SIMULTANEOUS OBSERVATION OF RECONNECTION INFLOW AND OUTFLOW ASSOCIATED WITH THE 2010 AUGUST 18 SOLAR FLARE , 2011, 1112.1398.
[39] D. McKenzie,et al. LOW-ALTITUDE RECONNECTION INFLOW–OUTFLOW OBSERVATIONS DURING A 2010 NOVEMBER 3 SOLAR ERUPTION , 2011, 1111.1945.
[40] X. Sun,et al. SHARP: Space-Weather HMI Active Region Patches , 2011 .
[41] H. Ji,et al. Phase Diagram for Magnetic Reconnection in Heliophysical, Astrophysical and Laboratory Plasmas , 2011, 1109.0756.
[42] M. Temmer,et al. An Observational Overview of Solar Flares , 2011, 1109.5932.
[43] William Daughton,et al. Role of electron physics in the development of turbulent magnetic reconnection in collisionless plasmas , 2011 .
[44] J. Schou,et al. VFISV: Very Fast Inversion of the Stokes Vector for the Helioseismic and Magnetic Imager , 2009, 0901.2702.
[45] C. J. Wolfson,et al. The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO) , 2011 .
[46] Astronomy,et al. Physics of Solar Prominences: I—Spectral Diagnostics and Non-LTE Modelling , 2010, 1001.1620.
[47] Thomas R. Metcalf,et al. Resolving the 180° Ambiguity in Solar Vector Magnetic Field Data: Evaluating the Effects of Noise, Spatial Resolution, and Method Assumptions , 2009 .
[48] Yi-Min Huang,et al. Fast reconnection in high-Lundquist-number plasmas due to the plasmoid Instability , 2009, 0906.5599.
[49] A. Benz,et al. Flare Observations , 2016, Living Reviews in Solar Physics.
[50] Andrzej Galat,et al. Technical note , 2008, Comput. Biol. Chem..
[51] T. Kosugi,et al. The Hinode (Solar-B) Mission: An Overview , 2007 .
[52] J. Qiu,et al. Direct Observation of High-Speed Plasma Outflows Produced by Magnetic Reconnection in Solar Impulsive Events , 2007, 0709.2329.
[53] A. M. James,et al. The EUV Imaging Spectrometer for Hinode , 2007 .
[54] P. Mahadevan,et al. An overview , 2007, Journal of Biosciences.
[55] T. Sakurai,et al. Preprocessing of Vector Magnetograph Data for a Nonlinear Force-Free Magnetic Field Reconstruction , 2006, astro-ph/0612641.
[56] M. Shay,et al. Electron acceleration from contracting magnetic islands during reconnection , 2006, Nature.
[57] P. Schuck. Tracking Magnetic Footpoints with the Magnetic Induction Equation , 2006 .
[58] Peter R. Young,et al. CHIANTI—An Atomic Database for Emission Lines. VII. New Data for X-Rays and Other Improvements , 2006 .
[59] T. Török,et al. Confined and Ejective Eruptions of Kink-unstable Flux Ropes , 2005, astro-ph/0507662.
[60] J. Raymond,et al. Direct Observations of the Magnetic Reconnection Site of an Eruption on 2003 November 18 , 2005 .
[61] T. Wiegelmann. Optimization code with weighting function for the reconstruction of coronal magnetic fields , 2008, 0802.0124.
[62] Haimin Wang,et al. Observations of the Failed Eruption of a Filament , 2003 .
[63] G. Holman,et al. Evidence for the Formation of a Large-Scale Current Sheet in a Solar Flare , 2003 .
[64] G. J. Hurford,et al. RHESSI Data Analysis Software: Rationale and Methods , 2002 .
[65] G. Hornig,et al. Theory of magnetic connectivity in the solar corona , 2002 .
[66] E. Priest,et al. The magnetic nature of solar flares , 2002 .
[67] J. Brown,et al. Nonsolar astronomy with the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) , 2003, SPIE Astronomical Telescopes + Instrumentation.
[68] Takaaki Yokoyama,et al. Clear Evidence of Reconnection Inflow of a Solar Flare , 2001 .
[69] M. Karlický,et al. Solar flare radio pulsations as a signature of dynamic magnetic reconnection , 2000, astro-ph/0006324.
[70] T. Forbes,et al. Effects of reconnection on the coronal mass ejection process , 2000 .
[71] K. Shibata. Evidence of Magnetic Reconnection in Solar Flares and a Unified Model of Flares , 1998 .
[72] Saku Tsuneta,et al. Structure and Dynamics of Magnetic Reconnection in a Solar Flare , 1996 .
[73] E. Priest,et al. Three‐dimensional magnetic reconnection without null points: 1. Basic theory of magnetic flipping , 1995 .
[74] Thomas R. Metcalf,et al. Resolving the 180-degree ambiguity in vector magnetic field measurements: The ‘minimum’ energy solution , 1994 .
[75] T. Kosugi,et al. A loop-top hard X-ray source in a compact solar flare as evidence for magnetic reconnection , 1994, Nature.
[76] B. Kliem. Particle Orbits, Trapping, and Acceleration in a Filamentary Current Sheet Model , 1994 .
[77] S. Tsuneta. Observation of a Solar Flare at the Limb with the Yohkoh Soft X-Ray Telescope (Initial Results from Yohkoh) , 1992 .
[78] R. Kopp,et al. Magnetic reconnection in the corona and the loop prominence phenomenon , 1976 .
[79] P. Sturrock. Model of the High-Energy Phase of Solar Flares , 1966, Nature.
[80] H. Carmichael,et al. A process for flares , 1964 .
[81] George E. Hale,et al. The Magnetic Polarity of Sun-Spots , 1919 .