Characterizing Magnetic Reconnection Regions Using Gaussian Mixture Models on Particle Velocity Distributions
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[1] David G. Sibeck,et al. On the electron diffusion region in planar, asymmetric, systems , 2014 .
[2] René Pellat,et al. Stability of a thick two‐dimensional quasineutral sheet , 1982 .
[3] E. Priest,et al. Magnetohydrodynamic evolution of magnetic skeletons , 2007, Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences.
[4] V. Titov,et al. Generalized Squashing Factors for Covariant Description of Magnetic Connectivity in the Solar Corona , 2007, astro-ph/0703671.
[5] S. Sheather. Density Estimation , 2004 .
[6] D. Rubin,et al. Maximum likelihood from incomplete data via the EM - algorithm plus discussions on the paper , 1977 .
[7] E. G. Harris. On a plasma sheath separating regions of oppositely directed magnetic field , 1962 .
[8] G. Lapenta,et al. Ion reflection and acceleration near magnetotail dipolarization fronts associated with magnetic reconnection , 2015 .
[9] Enrico Camporeale,et al. RECONNECTION AND ELECTRON TEMPERATURE ANISOTROPY IN SUB-PROTON SCALE PLASMA TURBULENCE , 2013, 1304.1444.
[10] H. Karimabadi,et al. Fundamental Concepts Associated with Magnetic Reconnection , 2016 .
[11] B. Ishak,et al. Statistics, data mining, and machine learning in astronomy: a practical Python guide for the analysis of survey data, by Željko Ivezić, Andrew J. Connolly, Jacob T. VanderPlas and Alexander Gray , 2017 .
[12] E. Priest,et al. Magnetic reconnection at three-dimensional null points , 1996, Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences.
[13] V. Vasyliūnas,et al. A survey of low-energy electrons in the evening sector of the magnetosphere with OGO 1 and OGO 3. , 1968 .
[14] S. M. Shaaban,et al. Temperature anisotropy instabilities stimulated by the interplay of the core and halo electrons in space plasmas , 2018 .
[15] M. Hesse,et al. The Diffusion Region in Collisionless Magnetic Reconnection , 1999 .
[16] David R. Anderson,et al. Model selection and multimodel inference : a practical information-theoretic approach , 2003 .
[17] Richard M. Thorne,et al. Variability of the pitch angle distribution of radiation belt ultrarelativistic electrons during and following intense geomagnetic storms: Van Allen Probes observations , 2015 .
[18] V. Vasyliūnas. Theoretical models of magnetic field line merging , 1975 .
[19] R. Torbert,et al. Highly structured electron anisotropy in collisionless reconnection exhausts , 2014 .
[20] A. Klimas,et al. New measure of the dissipation region in collisionless magnetic reconnection. , 2011, Physical review letters.
[21] Stefano Markidis,et al. Multi-scale simulations of plasma with iPIC3D , 2010, Math. Comput. Simul..
[22] M. Shay,et al. Energy partition in magnetic reconnection in Earth's magnetotail. , 2013, Physical review letters.
[23] N. Bessho,et al. Electron distribution functions in the diffusion region of asymmetric magnetic reconnection , 2016 .
[24] W. Newcomb. Motion of magnetic lines of force , 1958 .
[25] Adam Szabo,et al. Physics-based Tests to Identify the Accuracy of Solar Wind Ion Measurements: A Case Study with the Wind Faraday Cups , 2006 .
[26] Thomas E. Moore,et al. Magnetospheric Multiscale Overview and Science Objectives , 2016 .
[27] J. Finn,et al. Three-dimensional kinematic reconnection in the presence of field nulls and closed field lines , 1990 .
[28] Eric Ronald Priest,et al. Reconnection of magnetic fields : magnetohydrodynamics and collisionless theory and observations , 2007 .
[29] M. Shay,et al. Effect of inflow density on ion diffusion region of magnetic reconnection: Particle-in-cell simulations , 2011 .
[30] L. Fazendeiro,et al. Viriato: A Fourier-Hermite spectral code for strongly magnetized fluid-kinetic plasma dynamics , 2015, Comput. Phys. Commun..
[31] N. Buzulukova,et al. Spontaneous formation of dipolarization fronts and reconnection onset in the magnetotail , 2013 .
[32] Michael Hesse,et al. Electron nongyrotropy in the context of collisionless magnetic reconnection , 2013 .
[33] M. Hellberg,et al. Generalized plasma dispersion function for a plasma with a kappa-Maxwellian velocity distribution , 2002 .
[34] M. Lazar,et al. Kappa Distributions: Theory and Applications in Space Plasmas , 2010, 1003.3532.
[35] Eli Upfal,et al. Machine Learning in High Energy Physics Community White Paper , 2018, Journal of Physics: Conference Series.
[36] W. Dorland,et al. Fluidization of collisionless plasma turbulence , 2018, Proceedings of the National Academy of Sciences.
[37] Gaël Varoquaux,et al. Scikit-learn: Machine Learning in Python , 2011, J. Mach. Learn. Res..
[38] C. Russell,et al. Magnetospheric Multiscale Observation of Plasma Velocity-Space Cascade: Hermite Representation and Theory. , 2017, Physical review letters.
[39] D. Mccomas,et al. Characterizing the dayside magnetosheath using energetic neutral atoms: IBEX and THEMIS observations , 2013 .
[40] Nils-Bastian Heidenreich,et al. Bandwidth selection for kernel density estimation: a review of fully automatic selectors , 2013, AStA Advances in Statistical Analysis.
[41] S. Schwartz,et al. Electron Energy Partition across Interplanetary Shocks. I. Methodology and Data Product , 2019, The Astrophysical journal. Supplement series.
[42] Verena Heidrich-Meisner,et al. Solar Wind Classification Via k-Means Clustering Algorithm , 2018 .
[43] G. Lapenta,et al. On the origin of the crescent‐shaped distributions observed by MMS at the magnetopause , 2017, 1702.03550.
[44] Richard M. Thorne,et al. The modified plasma dispersion function , 1991 .
[45] M. Swisdak,et al. Quantifying gyrotropy in magnetic reconnection , 2015, 1509.00787.
[46] M. Hesse,et al. A theoretical foundation of general magnetic reconnection , 1988 .
[47] Geoffrey J. McLachlan,et al. Finite Mixture Models , 2019, Annual Review of Statistics and Its Application.
[48] M. Desai,et al. Generation of Kappa Distributions in Solar Wind at 1 au , 2018 .
[49] J. B. Blake,et al. Electron-scale measurements of magnetic reconnection in space , 2016, Science.
[50] Stefano Markidis,et al. On the electron agyrotropy during rapid asymmetric magnetic island coalescence in presence of a guide field , 2016, 1608.00725.
[51] P. Cassak,et al. Spacecraft Observations and Analytic Theory of Crescent-Shaped Electron Distributions in Asymmetric Magnetic Reconnection. , 2016, Physical review letters.
[52] R. Torbert,et al. Spatiotemporal evolution of electron characteristics in the electron diffusion region of magnetic reconnection: Implications for acceleration and heating , 2015 .
[53] G. Lapenta,et al. What Can We Learn about Magnetotail Reconnection from 2D PIC Harris-Sheet Simulations? , 2016 .
[54] Andrew J. Connolly,et al. Statistics, Data Mining, and Machine Learning in Astronomy , 2014 .
[55] Daniel N. Baker,et al. Classification of Magnetospheric Particle Distributions Via Neural Networks , 2018 .
[56] J. Scudder,et al. Electron diffusion region and thermal demagnetization , 2008 .
[57] D. Mccomas,et al. Understanding Kappa Distributions: A Toolbox for Space Science and Astrophysics , 2013 .
[58] G. Lapenta,et al. Multiscale study of electron energization during unsteady reconnection events , 2015 .
[59] Stefano Markidis,et al. Automated Classification of Plasma Regions Using 3D Particle Energy Distributions , 2019, Journal of Geophysical Research: Space Physics.
[60] H. Ji,et al. Conversion of magnetic energy in the magnetic reconnection layer of a laboratory plasma , 2014, Nature Communications.
[61] Stefano Markidis,et al. Progress towards physics-based space weather forecasting with exascale computing , 2017, Adv. Eng. Softw..
[62] Michael Hesse,et al. Geospace Environmental Modeling (GEM) magnetic reconnection challenge , 2001 .
[63] M. Gruntman. Anisotropy of the energetic neutral atom flux in the heliosphere , 1992 .