SH51E:
Fundamental Physics of the Solar Corona and Inner Heliosphere Posters


Submit an Abstract to this Session


Session ID#: 50153

Session Description:
The solar corona and wind provide a natural laboratory where magnetic fields guide and energize the plasma. Structured over a wide range of time and spatial scales, the coronal plasma is heated and accelerated giving rise to the turbulent, super-Alfvénic wind filling the heliosphere. With the launch of Parker Solar Probe, inner heliospheric research should reach a new level of understanding. This session explores the many facets of physical processes involved in heliospheric origins: from the sources of different wind types and their connection to coronal structures, to the micro-physics of distribution functions, anisotropies, to the role of turbulence and wave-particle interactions in heating and acceleration, to the energization associated with structures, such as shocks, current sheets and magnetic reconnection. What specific observables derived from models, what fundamental observations from Parker Solar Probe and Solar Orbiter should drive theoretical developments? Solicited contributions include theoretical, numerical simulation, and observational papers.
Primary Convener:  Chadi S Salem, SSL, University of California Berkeley, Berkeley, United States
Conveners:  Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States, Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States and Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
Primary Liaison:  Chadi S Salem, University of California, Berkeley, United States
Chairs:  Chadi S Salem, University of California, Berkeley, United States and Yannis Zouganelis, European Space Agency, Villanueva De La Can, Spain
OSPA Liaison:  Olga Panasenco, Advanced Heliophysics Inc., Pasadena, CA, United States
Index Terms:

2164 Solar wind plasma [INTERPLANETARY PHYSICS]
2169 Solar wind sources [INTERPLANETARY PHYSICS]
7509 Corona [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]
7524 Magnetic fields [SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY]

Abstracts Submitted to this Session:

A Study of Coronal Holes in Emission at Low Frequencies by the Murchison Widefield Array (358274)
Md Mozibur Rahman, University of Sydney, Sydney, NSW, Australia, Patrick I. McCauley, University of Sydney, Sydney, Australia and Iver Hugh Cairns, University of Sydney, School of Physics, Sydney, NSW, Australia
Observations of Condensations at Coronal Hole Boundaries: Dynamics and Implications (370262)
Emily Irene Mason, Catholic University of America, Washington, DC, United States, Spiro K Antiochos, NASA GSFC, Greenbelt, United States, Adrian Nigel Daw, NASA Goddard Space Flight Center, Greenbelt, United States and Michael Schlenker, Drexel University, Philadelphia, PA, United States
Coronal Hole Lifespans at Lower Latitudes Studied with the McIntosh Archive (370382)
Ian McDonald Hewins1, Sarah E Gibson2, David F Webb3, Robert McFadden1, Barbara A Emery4 and Thomas A Kuchar3, (1)ISR, Boston College at HAO/NCAR, Boulder, CO, United States, (2)National Center for Atmospheric Research, High Altitude Observatory, Boulder, CO, United States, (3)Boston College, ISR, Chestnut Hill, MA, United States, (4)HAO/NCAR, Boulder, CO, United States
Very Large Array Measurements of Coronal Angular Broadening (457895)
Jason Earl Kooi, US Naval Research Laboratory, Washington, United States, Avni Singh, George Mason University Fairfax, Volgenau School of Engineering, Fairfax, VA, United States, Prateek Bardhan, University of Texas at Austin, Department of Astronomy, Austin, TX, United States and Ian Sutcliffe, University of Virginia, Computer Science Department, Charlottesville, VA, United States
Measurement of Equatorial Coronal Magnetic Fields Using Faraday Rotation (374909)
Megan Noelle Kenny, University of Virginia, Charlottesville, VA, United States, Jason Earl Kooi, US Naval Research Laboratory, Washington, United States and Madison Grace Allen, Spelman College, Atlanta, GA, United States
Using Thomson-Scattering Brightness to Enhance Coronal Magnetic Field Measurements (375197)
Madison Grace Allen, Spelman College, Atlanta, GA, United States, Jason Earl Kooi, US Naval Research Laboratory, Washington, United States and Megan Noelle Kenny, University of Virginia, Charlottesville, VA, United States
In Situ Categorization and Coronal Origins of Different Slow Solar Wind Types (449453)
Olga Panasenco1, Marco C M Velli2, Aram Panasenco2, Roberto Lionello3 and Raffaella D'Amicis4, (1)Advanced Heliophysics Inc., Pasadena, CA, United States, (2)University of California Los Angeles, Los Angeles, CA, United States, (3)Predictive Science Inc., San Diego, United States, (4)INAF-Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy
The Onset of Magnetic Reconnection in the Solar Corona (400293)
Lars K. S. Daldorff, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, James Edward Leake, NASA Goddard Space Flight Center, Greenbelt, United States, James A Klimchuk, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Kalman Joshua Knizhnik, US National Research Council of the National Academies, Washington, DC, United States
Scattering Effects on Type II and Type III Bursts (414815)
Vratislav Krupar, Universities Space Research Association Columbia, Columbia, United States, Milan Maksimovic, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, Adam Szabo, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Ondrej Santolik, Institute of Atmospheric Physics, Czech Academy of Sciences, Prague, Czech Republic, Eduard Kontar, University of Glasgow, Glasgow, G12, United Kingdom, Jan Soucek, Inst. of Atmospheric Physics, Praha 4, Czech Republic and Oksana Kruparova, NASA/GSFC & UMBC/GPHI, Greenbelt, United States
New Evidence for Third Harmonic Radiation in Interplanetary Type III Solar Radio Bursts (395466)
Michael J Reiner, Catholic University of America, Washington, DC, United States; Catholic Univ & GSFC, Greenbelt, MD, United States and Robert J MacDowall, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Pseudostreamer Signatures in the Solar Corona and Inner Heliosphere (443693)
Mari Paz Miralles, Center for Astrophysics, Harvard & Smithsonian, Cambridge, United States
Differences in the elemental fractionation of Mg, Si, and Fe in the solar wind (367995)
Verena Heidrich-Meisner, Lars Berger and Robert F Wimmer-Schweingruber, University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany
A Three-Dimensional MHD Simulation of the Solar Corona and Solar Wind with Turbulence Transport and Heating (377181)
Arcadi V. Usmanov1, Prof. William H Matthaeus1, Melvyn L Goldstein2 and Dr. Rohit Chhiber, BSc (Honours), MSc, PhD3, (1)University of Delaware, Department of Physics and Astronomy, Newark, DE, United States, (2)Space Science Institute Boulder, Boulder, United States, (3)University of Delaware, Department of Physics and Astronomy, Newark, United States
Onset and evolution of fast reconnection including the Hall effect (410097)
Chen Shi, Auburn University, Department of Physics, Auburn, United States, Anna Tenerani, California Institute of Technology, Pasadena, CA, United States and Marco C M Velli, University of California Los Angeles, Los Angeles, CA, United States
The Electric Fields of the Sun and Solar Wind (361117)
Charles Fred Driscoll, University of California San Diego, Physics, La Jolla, CA, United States
A new approach to identify interplanetary Alfvénic fluctuations (370794)
Jin Liu, Yunnan University, Kunming, China and ChuanBing Wang, Univ. Sci. & Tech. China, Hefei, Anhui Province, China
The Effect of Turbulence on the Evolution of Magnetic Field Magnitude Fluctuations in the Solar Wind (394125)
D Aaron Roberts, NASA Goddard Space Flight Center, Greenbelt, MD, United States
investigating the temporal decorrelation of the incompressible MHD turbulence (465889)
Sofiane Bourouaine, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, United States and Jean Carlos Perez, Florida Institute of Technology, Aerospace, Physics and Space Sciences, Melbourne, FL, United States
Effect of turbulent cascade partitioning among ion species on the solar wind formation (401783)
Dmitry Borovikov, University of New Hampshire, Durham, MI, United States, Kris Klein, University of Michigan Ann Arbor, Ann Arbor, United States, Bart van der Holst, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, Daniel Verscharen, University College London, Mullard Space Science Laboratory, London, United Kingdom and Benjamin D G Chandran, University of New Hampshire, Durham, United States
Numerical Simulations of Kinetic Turbulence in the Low Beta Regime: Predictions for Observations by Parker Solar Probe (446933)
David Burgess1, Luca Franci1, Christopher H K Chen2, Emanuele Papini3, Simone Landi4, Petr Hellinger5, Lorenzo Matteini6 and Andrea Verdini3, (1)Queen Mary, University of London, London, United Kingdom, (2)Queen Mary University of London, Department of Physics and Astronomy, London, United Kingdom, (3)Università di Firenze, Dipartimento di Fisica e Astronomia, Firenze, Italy, (4)Università degli Studi di Firenze, Florence, Italy, (5)Astronomical Institute, CAS, Ondrejov/Prague, Czech Republic, (6)Observatoire De Paris, LESIA, Meudon, FRANCE
The Field-Particle Correlation Technique: A Method for Determining Particle Energization in the Inner Heliosphere (432018)
Gregory G Howes, University of Iowa, Physics and Astronomy, Iowa City, IA, United States, Prof. Kristopher Gregory Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, Jason M TenBarge, Princeton University, Princeton, NJ, United States, Christopher H K Chen, Queen Mary University of London, Department of Physics and Astronomy, London, United Kingdom, Jaye Verniero, University of California Berkeley, Berkeley, United States, Andrew J McCubbin, University of Iowa, Physics and Astronomy, Iowa City, United States and Francesco Valentini, University della Calabria, Rende, Italy
How Solar Orbiter will observe small-scale time variations of the solar wind and identify characteristic structures (369384)
Georgios Nicolaou, IRF Swedish Institute of Space Physics Kiruna, Kiruna, Sweden, Christopher John Owen, UCL, Mullard Space Science Laboratory, Dorking, United Kingdom, Daniel Verscharen, University College London, Mullard Space Science Laboratory, London, United Kingdom and Robert T Wicks, University of Maryland College Park, College Park, United States
Inertial Kinetic-Alfven Turbulence in a Space Plasma (383576)
Stanislav Boldyrev, University of Wisconsin Madison, Madison, WI, United States, Vadim Roytershteyn, Space Science Institute Boulder, Boulder, United States and Christopher H K Chen, Queen Mary University of London, Department of Physics and Astronomy, London, United Kingdom
Solar Wind Turbulence From MHD Down to Electron Kinetic Scales: Artemis Observations (418075)
Chadi S Salem, SSL, University of California Berkeley, Berkeley, United States, John W Bonnell, University of California, Berkeley, Space Sciences Laboratory, Berkeley, United States, Elizabeth (Lily) Hanson, University of California Berkeley, Berkeley, CA, United States, Christopher Carew Chaston, University of California Berkeley, Space Sciences Laboratory, Berkeley, United States, Prof. Kristopher Gregory Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, Daniel Verscharen, University College London, Mullard Space Science Laboratory, London, United Kingdom, Catherine Lacombe, LESIA, Observatoire de Paris, Meudon, France and David J Sundkvist, UC Berkeley, Berkeley, CA, United States
Whistler waves in the inner heliosphere from 0.3 to 1 AU (368161)
Vamsee Krishna Jagarlamudi1,2, Olga Alexandrova3, Laura Bercic2, Thierry Dudok de Wit1, Federico Fraternale4 and Milan Maksimovic3, (1)LPC2E, CNRS and University of Orléans, Orléans, France, (2)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université Paris Diderot, Sorbonne Paris Cité, Meudon, France, (3)LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France, (4)University of Alabama in Huntsville, Huntsville, AL, United States
A Statistical Study of Parametric Decay Instability of Alfvén Waves in the Inner-Heliosphere (414679)
Trevor Bowen1, Alfred Mallet2, David Stansby3 and Stuart D Bale1, (1)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (2)University of New Hampshire, Durham, NH, United States, (3)Imperial College London, London, SW7, United Kingdom
Modeling the Composition and Properties of Solar Wind (412853)
Michael Lavarra1, Alexis P Rouillard2 and Pierre-Louis Blelly1, (1)Université Toulouse III - Paul Sabatier, Observatoire Midi–Pyrénées, CNRS, CNES, IRAP, Toulouse, France, (2)IRAP, Toulouse, France
The statistical properties of solar wind temperature parameters near 1 AU observed by Wind (342039)
Lynn B Wilson III1, Michael Louis Stevens2, Justin Christophe Kasper3, Prof. Kristopher Gregory Klein4, Bennett Maruca5, Stuart D Bale6, Trevor Bowen6, Marc Pulupa6 and Chadi S Salem7, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Smithsonian Astrophysical Observatory, Cambridge, MA, United States, (3)University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, (4)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (5)Center for Astrophysics, Berkeley, CA, United States, (6)University of California Berkeley, Space Sciences Laboratory, Berkeley, CA, United States, (7)University of California, Berkeley, United States
An Analysis of the Solar Wind Angular Momentum Using WIND Data (415079)
Michael McManus, University of California Berkeley, Space Sciences Laboratory, Berkeley, United States
Unexpected Structures in the Slow Wind near the Stream Interface (424866)
Yong Liu1, Jia Huang2, Zhaohui Qi1, Chi Wang3 and Berndt Klecker4, (1)NSSC National Space Science Center, CAS, Beijing, China, (2)NSSC National Space Science Center, CAS, State Key Laboratory of Space Weather, Beijing, China, (3)NSSC, CAS, Beijing, China, (4)Max Planck Institut for Extraterrestrial Physics, Garching, Germany
Simple Dependence of Proton Density and Temperature on Solar Wind Speed and Compression (451177)
Christopher Mark Bert, University of Michigan, Ann Arbor, United States, Justin Christophe Kasper, University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, United States, Prof. Kristopher Gregory Klein, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, Anthony W Case, Smithsonian Astrophysical Observatory, Cambridge, MA, United States, Milan Maksimovic, LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Université de Paris, Meudon, France and Arnaud Zaslavsky, CNRS, Observatoire de Paris, LESIA, Meudon, France
Solar wind Suprathermal Electrons around the Corotating Interaction Regions at 1 AU (409397)
Jiawei Tao1, Linghua Wang2, Gang Li3, Robert F Wimmer-Schweingruber4, Lan Jian5 and Jiansen He1, (1)Peking University, Beijing, China, (2)Peking University, Institute of Space Physics and Applied Technology, Beijing, China, (3)University of Alabama in Huntsville, Huntsville, United States, (4)University of Kiel, Institute for Experimental and Applied Physics, Kiel, Germany, (5)NASA Goddard Space Flight Center, Greenbelt, MD, United States

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