Direct Multipoint Observations Capturing the Reformation of a Supercritical Fast Magnetosonic Shock
D. L. Turner, L. B. Wilson III, K. A. Goodrich, H. Madanian, S. J., Schwartz, T. Z. Liu, A. Johlander, D. Caprioli, I. J. Cohen, D. Gershman, H., Hietala, J. H. Westlake, B. Lavraud, O. Le Contel, and J. L. Burch

TL;DR
This study uses multipoint MMS observations to analyze the detailed process of shock reformation at Earth's bow shock, revealing the roles of electron-scale physics, energy conversion, and cross-scale coupling during the reformation cycle.
Contribution
It provides the first multipoint measurements of shock reformation at a supercritical fast magnetosonic shock, highlighting electron-scale physics and cross-scale interactions.
Findings
Shock reformation cycle observed with new shock ramp formation.
Electron-scale physics significantly influence shock reformation.
Energy conversion processes exhibit cyclical periodicity.
Abstract
Using multipoint Magnetospheric Multiscale (MMS) observations in an unusual string-of-pearls configuration, we examine in detail observations of the reformation of a fast magnetosonic shock observed on the upstream edge of a foreshock transient structure upstream of Earth's bow shock. The four MMS spacecraft were separated by several hundred km, comparable to suprathermal ion gyro-radius scales or several ion inertial lengths. At least half of the shock reformation cycle was observed, with a new shock ramp rising up out of the "foot" region of the original shock ramp. Using the multipoint observations, we convert the observed time-series data into distance along the shock normal in the shock's rest frame. That conversion allows for a unique study of the relative spatial scales of the shock's various features, including the shock's growth rate, and how they evolve during the reformation…
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