Fig. 2
From: Reiner Gamma albedo features reproduced by modeling solar wind standoff
Close-up of the Reiner Gamma albedo pattern and simulated energy flux to the surface after the simulation has reached steady state. a LRO-WAC empirically normalised reflectance image for the Reiner Gamma region60,61. b Normalised proton energy flux profile below 1.35 km above the lunar surface from simulation. Both panels are extracted from Fig. 1 and share the same colour scale; a, b do not share the same spatial scale, a is zoomed 2.5 times compared to b
