Member Since 2006
Lynn B. Wilson III
Plasma Physicist, NASA Goddard Space Flight Center
AGU Research
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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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Comparison of Waves Measured by Parker Solar Probe During Interplanetary Shocks at 15 Rs and 49Rs
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Elizabeth (Lily) Hanson, Cynthia A. Cattell, Keith...
During Encounter 13, Parker Solar Probe (PSP) was enveloped by an interplanetary coronal mass ejection (ICME) preceded by an interplanetary (IP) shock...
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Kinetic complexities of the near-Sun heliospheric current sheet observed by Parker Solar Probe
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Jaye Verniero, Kristoff W. Paulson, Adam Szabo, Ol...
The heliospheric current sheet (HCS), which separates the Suns magnetic field lines of opposite polarity in the solar wind, is a complex structure tha...
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Downstream Jets at Interplanetary and Planetary Shocks
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
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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Short-Wavelength Electric Field Fluctuations in Simulations of Collisionless Plasma Shocks
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Vadim Roytershteyn, Lynn B. Wilson, Li-Jen Chen, M...
Large-amplitude electrostatic fluctuations are routinely observed by spacecraft upon traversal of collisionless shocks in the heliosphere. Kinetic sim...
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Compound electron acceleration at planetary foreshocks
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Xiaofei Shi, Anton Artemyev, Vassilis Angelopoulos...
Shock waves, the interface of supersonic and subsonic plasma flows, are the primary region for charged particle acceleration in multiple space plasma ...
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