Fig. 1
From: Reiner Gamma albedo features reproduced by modeling solar wind standoff
Comparison of the relative brightness of Reiner Gamma with the simulated surface flux patterns after the simulation has reached steady state. a LRO-WAC empirically normalised reflectance image for the Reiner Gamma region60,61. b Normalised proton charge density profile below 1.35 km above the lunar surface from simulation. c Normalised proton number flux profile below 1.35 km above the lunar surface from simulation. d Normalised proton energy flux profile below 1.35 km above the lunar surface from simulation. All panels share the same spatial scale and linear colour scale
