JS
Member Since 2010
Joshua E. Stawarz
Royal Society University Research Fellow, Northumbria University Newcastle
AGU Research
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Statistical Study of Energy Transport and Conversion in Electron Diffusion Regions at Earth's Dayside Magnetopause
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
03 october 2024
Naïs Fargette, Jonathan P. Eastwood, Martin V. Gol...
The electron diffusion region (EDR) is a key region for magnetic reconnection, but the typical energy transport and conversion in EDRs is still not...
Statistical Observations of Proton‐Band Electromagnetic Ion Cyclotron Waves in the Outer Magnetosphere: Full Wavevector Determination
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
15 may 2024
Sergio Toledo Redondo, Inmaculada F Albert, Mats A...
Electromagnetic Ion Cyclotron (EMIC) waves mediate energy transfer from the solar wind to the magnetosphere, relativistic electron precipitation, o...
Automatic Encoding of Unlabeled Two Dimensional Data Enabling Similarity Searches: Electron Diffusion Regions and Auroral Arcs
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
27 january 2024
Andrew W. Smith, Jonathan Rae, Julia E. Stawarz, W...
Critically important phenomena in Earth’s magnetosphere often occur briefly, or in small spatial regions. These processes are sampled with or...
Electron acceleration in magnetic flux ropes in shock turbulence
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA III ORAL
spa-solar and heliospheric physics | 15 december 2023
Naoki Bessho, Li-Jen Chen, Michael Hesse, Jonathan...
MMS observations of reconnecting current sheets in the shock transition and downstream regions of the Earths bow shock motivated this work. We carry o...
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Turbulent Plasmas in the Solar Wind and Earth’s Magnetosphere: What have we learned and where are we going?
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA III ORAL
spa-solar and heliospheric physics | 15 december 2023
Julia E. Stawarz, Alexandros Chasapis, Naoki Bessh...
Owing to the large dataset of high-quality in situ measurements from a fleet of current and previous spacecraft missions, the turbulent environments i...
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Reconnection-driven Agyrotropic Electron Velocity Distributions in Turbulent Plasmas
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA I POSTER
spa-solar and heliospheric physics | 14 december 2023
Luca Franci, Daniele Del Sarto, Emanuele Papini, A...
The inherently kinetic and collisionless nature of the solar wind plasma allows it to exist out of thermodynamical equilibrium for large time interval...
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Heating and Acceleration of the Solar Wind by Magnetic Switchbacks
FUNDAMENTAL PHYSICS OF THE SOLAR CORONA AND INNER HELIOSPHERE III POSTER
spa-solar and heliospheric physics | 14 december 2023
Yeimy Rivera, Samuel T. Badman, Michael L. Steven...
It is well established that the solar wind is actively heated and accelerated after it escapes the closed-field corona. Parker Solar Probe's close pro...
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The Energy Budget Associated with Turbulence-Driven Magnetic Reconnection
MAGNETIC RECONNECTION: CONNECTING IDEAS FROM OBSERVATIONS, EXPERIMENTS, MODELS, AND THEORY III ORAL
spa-magnetospheric physics | 13 december 2023
Julia E. Stawarz, Jonathan P. Eastwood, Tai D. Pha...
Magnetic reconnection and turbulence have long been thought to be fundamentally interrelated phenomena in the context of plasma systems, with the nonl...
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