BibTex format
@article{Kelly:2026:10.1029/2025GL120284,
author = {Kelly, H and Archer, M and Eastwood, J and Heyns, M and Eggington, J and Chittenden, J},
doi = {10.1029/2025GL120284},
journal = {Geophysical Research Letters},
title = {Superposition of doppler-shifting magnetopause Kelvin-Helmholtz modes through dynamic mode decomposition of a global MHD simulation},
url = {http://dx.doi.org/10.1029/2025GL120284},
volume = {53},
year = {2026}
}
RIS format (EndNote, RefMan)
TY - JOUR
AB - The Kelvin-Helmholtz instability (KHI) mediates the viscous-like solar-terrestrial interaction by generating magnetopause surface waves that quickly become non-linear. Basic theory predicts the locally most-unstable linear wave dominates. However, Kelvin-Helmholtz is a broad, convective instability that also amplifies waves originating upstream. We address this conundrum by applying dynamic mode decomposition to a Gorgon global magnetohydrodynamic simulation of the KHI. While distinct modes quickly grow at points along the magnetopause, signaling local generation, their energy continues to slowly grow downtail. Thus, a superposition is present along the magnetopause, where the dominant mode is not always the locally fastest-growing. Each mode's wavelength elongates downtail, correlating with the boundary layer flow speed due to the accelerating advective flow around the magnetosphere Doppler shifting the fixed-frequency waves. This may explain why longer wavelengths are observed in the tail than theory predicts and motivates further exploration of tangential inhomogeneities in basic Kelvin-Helmholtz theory.
AU - Kelly,H
AU - Archer,M
AU - Eastwood,J
AU - Heyns,M
AU - Eggington,J
AU - Chittenden,J
DO - 10.1029/2025GL120284
PY - 2026///
SN - 0094-8276
TI - Superposition of doppler-shifting magnetopause Kelvin-Helmholtz modes through dynamic mode decomposition of a global MHD simulation
T2 - Geophysical Research Letters
UR - http://dx.doi.org/10.1029/2025GL120284
UR - https://meetingorganizer.copernicus.org/EGU26/EGU26-21774.html
VL - 53
ER -