Mercury's Eccentric Orbit as a Driver of Significant “Seasonal” Change in Upstream Solar Wind Forcing

Abstract Mercury experiences the most intense and variable solar wind (SW) conditions in the solar system due to its close, eccentric orbit about the Sun. In addition to variation driven by coronal source and solar cycle, the SW arriving at Mercury varies periodically as the planet's heliocentric distance changes by over 50% per orbit. We use 30 years of SW measurements near Earth and scale them to Mercury's orbital distance to determine the importance of this “seasonal” change in the SW. We find the seasonal change to be substantial, systematic, and significant, and that it dominates over other sources of variability (e.g., fast vs. slow SW) and even exceeds the relative change at Earth from ICMEs compared to the ambient SW. As a result, Mercury's magnetosphere is expected to exhibit substantial seasonal effects.

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Publication Details

Journal
Geophysical Research Letters
Published
2026-06-19
DOI
https://doi.org/10.1029/2026gl123323
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
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article

Mercury's Eccentric Orbit as a Driver of Significant “Seasonal” Change in Upstream Solar Wind Forcing

A. D. Shane, Jesse T. Coburn, Yeimy J. Rivera, W. Sun et al.
Geophysical Research Letters
Planetary Science and Exploration
article

Mercury's Eccentric Orbit as a Driver of Significant “Seasonal” Change in Upstream Solar Wind Forcing

A. D. Shane, Jesse T. Coburn, Yeimy J. Rivera, W. Sun, Daragh M. Hollman, Beatriz Sánchez‐Cano, Jim M. Raines, J. A. Slavin, S. Livi, Jiutong Zhao, C. F. Bowers, C. M. Jackman, Mathias Rojo, Daniel Heyner, Lina Hadid, Sae Aizawa, S. T. Lepri, R. M. Dewey
article en

Abstract

Abstract Mercury experiences the most intense and variable solar wind (SW) conditions in the solar system due to its close, eccentric orbit about the Sun. In addition to variation driven by coronal source and solar cycle, the SW arriving at Mercury varies periodically as the planet's heliocentric distance changes by over 50% per orbit. We use 30 years of SW measurements near Earth and scale them to Mercury's orbital distance to determine the importance of this “seasonal” change in the SW. We find the seasonal change to be substantial, systematic, and significant, and that it dominates over other sources of variability (e.g., fast vs. slow SW) and even exceeds the relative change at Earth from ICMEs compared to the ambient SW. As a result, Mercury's magnetosphere is expected to exhibit substantial seasonal effects.

Geophysical Research LettersVol. 53(12)
Southwest Research Institute (US), Centre National de la Recherche Scientifique (FR), Dublin Institute For Advanced Studies (IE), Université Toulouse III - Paul Sabatier (FR), École Polytechnique (FR), University of Leicester (GB), University of Colorado Boulder (US), Université Paris-Saclay (FR), University of Michigan (US), Sorbonne Université (FR), Center for Astrophysics Harvard & Smithsonian (US), Laboratoire de Physique des Plasmas (FR), Institut de Recherche en Astrophysique et Planétologie (FR), Technische Universität Braunschweig (DE), University of California, Berkeley (US)
National Aeronautics and Space Administration, Science and Technology Facilities Council, Planetary Science Division, Research Ireland
Openalex Percentile: Top 7%
Planetary Science and Exploration
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