Fig. 12From: Nanoscale analysis of noble gas in solidsSolar wind 4He distribution of asteroid Itokawa sample grain, RA-QD02-0169; olivine. a Backscattered electron image of the Itokawa sample. Red square: 4He mapping area. b x–y–z directions of the 4He mapping area. x, y: parallel to the surface, z: depth. c Three-dimensional map of 4He distribution. Color contours of red color: 1020 He cm−3, light gray color: 5 × 1019 He cm−3, and dark gray color: 1019 He cm−3. Cuboid size: (x, y, z) = (8 µm, 13 µm, 525 nm). d 4He distribution of x–y plane at z = 50 nm, e He distribution of the x–z cross-section at the line x1 shown in (d). f 4He distribution of the y–z cross-section at the line y1 shown in (d). Color contours of (d), (e), and (f) are shown in the figureBack to article page