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Investigating the Role of Magnetic Cohesion in Avalanching on 16-Psyche: A Discrete Element Modeling Approach

  • Authors: Anmol Sikka, Christine M. Hartzell

Anmol Sikka and Christine M. Hartzell 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Trends of mean angle of repose (﹩{\bar{\theta }}_{B}﹩), rms height (﹩\bar{\xi }﹩), and rms slope (﹩{\bar{\theta }}_{{\rm{r}}{\rm{m}}{\rm{s}}}﹩), with the increasing magnetic field strength (B) and the magnetic Bond numbers for different material compositions. The mean values are calculated as weighted averages, with R2 values as weights. The error bars are calculated as a weighted average of the standard errors for each parameter. The effects of magnetic cohesion are evident in the rms height and rms slope plots for the 500 and 1000 μT field strength, where the values are higher than those for the other field strengths in cases with a higher percentage of high-susceptible. All other cases remain similar across field strengths, as suggested by the angle-of-repose plot.

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