Anisotropic Magnetic Turbulence in the Inner Heliosphere—Radial Evolution of Distributions Observed by Parker Solar Probe

Authors: Rohit Chhiber (NASA GSFC and U Delaware) Observations from Parker Solar Probe’s first several orbits are used to investigate the helioradial evolution of probabilityView More

A Quantitative Comparison of Multipoint Magnetic Field Reconstruction Methods

Authors: Theodore Broeren (University of Arizona), Kristopher Klein (University of Arizona) The upcoming NASA mission HelioSwarm will use nine spacecraft to make simultaneous measurements ofView More

Does Big Heating Come in Small Sizes? Chromospheric Turbulence and Heating Due to the Thermal Farley-Buneman Instability

Authors: Samuel Evans (Boston University Center for Space Physics), Meers Oppenheim (Boston University Center for Space Physics), Juan Martínez-Sykora (Lockheed Martin Solar & Astrophysics Laboratory),View More

Phase-space turbulence in electrostatic plasmas

Authors: Michael Nastac (University of Oxford), Michael Barnes (University of Oxford), Robert Ewart (University of Oxford), James Juno (Princeton Plasma Physics Laboratory), Alexander Schekochihin (UniversityView More

Elemental abundance variations across coronal hole boundaries

Authors: Alexandros Koukras (Columbia University), Michael Hahn (Columbia University), Daniel W. Savin (Columbia University) The fast solar wind originates from regions of open magnetic fieldView More

Identifying the phase of magnetic reconnection using the temporal evolution of pressure-strain interaction

Authors: Hasan Barbhuiya (West Virginia University), Paul Cassak (West Virginia University) Energy conversion in collisionless space plasmas has garnered significant attention in recent years. KineticView More

Comparing Landau and Cyclotron Damping Rates Constrained by PSP Observations

Authors: Niranjana Shankarappa (University of Arizona), Kristopher Klein (University of Arizona), Mihailo Martinovic (University of Arizona) Solar wind heating and acceleration is a long-standing problemView More

Extended magnetic reconnection in kinetic plasma turbulence

Authors: Tak Chu Li (Dartmouth College), Yi-Hsin Liu (Dartmouth College), Yi Qi (University of Colorado Boulder), and Muni Zhou (Institute for Advanced Study) Magnetic reconnectionView More

Decomposing the global solar magnetic field to understand the IMF evolution: a new suggestion for the open flux problem

Authors: Minami Yoshida (The University of Tokyo, ISAS/JAXA), Toshifumi Shimizu (ISAS/JAXA, The University of Tokyo), Shin Toriumi (ISAS/JAXA) The “open” magnetic field extending from theView More

Theoretical Developments on Energy Conversion via the Pressure-Strain Interaction and Applications to Magnetic Reconnection

Authors: Paul Cassak (West Virginia University), Hasan Barbhuiya (West Virginia University) Energy conversion between bulk kinetic and thermal energy in weakly collisional and collisionless plasmas,View More

Analysis of Faraday Cup measurements using Artificial Neural Networks

Authors: Lidiya Y. Ahmed1,2 , Michael L. Stevens1, Kristoff Paulson1, Anthony Case1 1 Smithsonian Astrophysical Observatory 2 Harvard University Solar wind parameters such as density,View More

This plot shows the relationship between Mean Solar Brightness and CME velocity in kilometers per second.

The Relationship between Coronal Mass Ejections and Brightness of the Corona

Authors: Kelly Victor-French (NRL), Karl Battams (NRL), Brian Wood (NRL) We present our investigation into the relationship between coronal brightness and the eruptivity of solarView More

Exploring the effect of turbulent fluctuations on the onset of reconnection

Authors: Jeffersson Agudelo Rueda, (Department of Physics and Astronomy, Dartmouth College, Hanover, NH, USA), Yi-Hsin Liu (Department of Physics and Astronomy, Dartmouth College, Hanover, NH,View More

Nonequilibrium Ionization Modeling of Petschek-type Shocks in Reconnecting Current Sheets in Solar Eruptions

Authors: Chengcai Shen (CfA), John C. Raymond (CfA), Nicholas A. Murphy (CfA) Nonequilibrium ionization (NEI) is essentially required for astrophysical plasma diagnostics once the plasmaView More

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