“…Martian “inverted channels” resemble terrestrial fossilized paleofluvial channels (Foix et al, ; Maizels ; Martinez et al, ; Pain & Ollier, ; Williams et al, ), and are identified by their sinuous and/or branching planimetric pattern, continuity relationships with valley networks, and geologic context (e.g., distributary channels on alluvial fans). FSRs on Mars range in scale from large‐scale landforms identified in Viking images (10–200 km long, 0.3 to 3 km wide; Howard, ; Kargel & Strom, ) to fine‐scale bifurcating ridges (few hundred meters long, few tens of meters wide; Burr et al, , ; Davis et al, ; Williams & Edgett, ; Williams et al, ).…”