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Possible Magnetic Perturbations Associated with Starship Lunar Landings

  • Authors: William M. Farrell, Stefano Boccelli, Orenthal J. Tucker

William M. Farrell et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 9.

The geometry of the current region used to calculate the B-field in Figure 8. The current flowing through a 200 km × 200 km region in the XY-plane located at a height of 50 km was divided up onto a set of smaller distributed line currents, I, each located in 100 × 100 grids having 2 km × 2 km in cross-sectional size. The width of the current region is 20 km. The B-field at any observation point is then calculated by summing the contributions from each of the smaller line currents I = I (xs, ys, zs).

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