Member Since 2006
Lynn B. Wilson III
Plasma Physicist, NASA Goddard Space Flight Center
Member, Space Physics and Aeronomy Canvassing Committee
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
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
The Effect of Intermediate Frequency Waves on the Radial Evolution of Coronal Mass Ejections from ~1 au to ~5 au: Juno, Wind, STEREO and ARTEMIS
AGU 2024
spa-solar and heliospheric physics | 13 december 2024
Cynthia A. Cattell, Sadie Elliott, Elizabeth (Lily...
The evolution of interplanetary coronal mass ejections (ICMEs) from near the Sun to the outer heliosphere has been the focus of many studies utilizing...
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Determining The SNR Requirements For FETCH, A Novel Faraday Rotation Instrument
AGU 2024
spa-solar and heliospheric physics | 13 december 2024
Elizabeth A. Jensen, Nat Gopalswamy, Shing F. Fung...
The magnetic field within interplanetary plasma can only be reliably and regularly measured across broad swaths of space with the technique of Faraday...
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Properties of Ion-Scale Circularly-Polarized Waves in the Solar Wind
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Samuel Fordin, Michael A. Shay, Lynn B. Wilson
The solar wind is full of electromagnetic fluctuations at or near the characteristic ion scales. Many of these fluctuations can be identified as magne...
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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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