activity
20052026
most citedWhy does steady-state magnetic reconnection have a maximum local rate of order 0.1?

186 citations · 2.5k across the 62 of their papers we have counts for

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Showing 2023Show all

7 papers · 1 filter

physics.space-ph2023

Unveiling plasma energization and energy transport in the Earth Magnetospheric System: the need for future coordinated multiscale observations

A. Retino, L. Kepko, H. Kucharek +31

Energetic plasma is everywhere in the Universe. The terrestrial Magnetospheric System is a key case where direct measures of plasma energization and energy transport can be made in…

physics.plasm-ph2023

Scale Filtering Analysis of Kinetic Reconnection and its Associated Turbulence

Subash Adhikari, Yan Yang, William H. Matthaeus +3

Previously, using an incompressible von Kármán-Howarth formalism, the behavior of cross-scale energy transfer in magnetic reconnection and turbulence was found to be essentially id…

physics.plasm-ph2023★ 1 cited

The Importance of Heat Flux in Quasi-Parallel Collisionless Shocks

Colby C. Haggerty, Damiano Caprioli, Paul A. Cassak +3

Collisionless plasma shocks are a common feature of many space and astrophysical systems and are sources of high-energy particles and non-thermal emission, channeling as much as 20…

astro-ph.IM2023

Multi-point Assessment of the Kinematics of Shocks (MAKOS): A Heliophysics Mission Concept Study

Katherine A. Goodrich, Lynn B. Wilson, Steven Schwartz +6

Collisionless shocks are fundamental processes that are ubiquitous in space plasma physics throughout the Heliosphere and most astrophysical environments. Earth's bow shock and int…

physics.plasm-ph2023★ 27 cited

Quantifying Energy Conversion in Higher Order Phase Space Density Moments in Plasmas

Paul A. Cassak, M. Hasan Barbhuiya, Haoming Liang +1

Weakly collisional and collisionless plasmas are typically far from local thermodynamic equilibrium (LTE), and understanding energy conversion in such systems is a forefront resear…

astro-ph.IM2023★ 3 cited

Magnetic Energy Powers the Corona: How We Can Understand its 3D Storage & Release

Amir Caspi, Daniel B. Seaton, Roberto Casini +12

The coronal magnetic field is the prime driver behind many as-yet unsolved mysteries: solar eruptions, coronal heating, and the solar wind, to name a few. It is, however, still poo…