LW
Member Since 2006
Lynn B. Wilson III
Plasma Physicist, NASA Goddard Space Flight Center
Professional Experience
St. John's University
2022 - Present
NASA Goddard Space Flight Center
Plasma Physicist
2010 - Present
Education
College of Saint Benedict
Bachelors
2005
St Johns University
Bachelors
2005
University of Minnesota Twin Cities
Doctorate
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Honors & Awards
Outstanding Reviewer Award - Geophysical Research Letters
Received December 2022
Outstanding Reviewer Award - JGR-Space Physics
Received December 2016
Current Roles
Member
Space Physics and Aeronomy Canvassing Committee
Publications
Shocklets and Short Large Amplitude Magnetic Structures (SLAMS) in the High Mach Foreshock of Venus
Shocklets and short large‐amplitude magnetic structures (SLAMS) are steepened magnetic fluctuations commonly found in Earth's upstream foresh...
September 26, 2023
Decadal and Annual Variations in Meteoric Flux From Ulysses,...
October 18, 2022
Energy Partition at Collisionless Supercritical Quasi‐Perpen...
October 13, 2022
A Revised Understanding of the Structure of the Venusian Mag...
January 04, 2022
Evaluating the deHoffmann‐Teller Cross‐Shock Potential at Re...
August 01, 2021
AGU Abstracts
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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Downstream Jets at Interplanetary Shocks
TURBULENCE, MAGNETIC RECONNECTION, PARTICLE ENERGIZATION, AND FUNDAMENTAL PLASMA PROCESSES IN SPACE PLASMA III ORAL
spa-solar and heliospheric physics | 15 december 2023
Heli Hietala, Domenico Trotta, Annamaria Fedeli, L...
Localised dynamic pressure enhancements - jets - are regularly observed downstream of the Earths bow shock. They drive enhanced particle acceleration,...
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A Statistical Study of Circularly-Polarized Waves in the Solar Wind Using Machine Learning
MAGNETIC STRUCTURES AND WAVES IN SOLAR WIND TURBULENCE I POSTER
spa-solar and heliospheric physics | 14 december 2023
Samuel Fordin, Michael A. Shay, Lynn B. Wilson
The Wind spacecraft has yielded several decades of high-resolution magnetic field data, a large fraction of which displays small-scale structures. In ...
View Abstract
Volunteer Experience
2023 - 2025
Member
Space Physics and Aeronomy Canvassing Committee
Check out all of Lynn B. Wilson’s AGU Research!
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