“…Although atmospheric HONO has been measured for several decades [ Perner and Platt , ], sources of HONO to the atmosphere remain uncertain [e.g., Stutz et al ., ; Kleffmann , ; Zhou et al ., ; Li et al ., ; VandenBoer et al ., ; Gall et al ., ]. HONO sources include direct emission from combustion [ Kirchstetter et al ., ; Kurtenbach et al ., ; Stutz et al ., ; Wood et al ., ; Jurkat et al ., ; Burling et al ., ] and soils [ Oswald et al ., ], formation by gas phase reaction of OH and NO [ Calvert et al ., ], and production by surface reaction of nitrogen‐containing compounds [e.g., Stutz et al ., ; Stemmler et al ., ; Kleffmann , ; Zhou et al ., ; VandenBoer et al ., ; Baergen et al ., ]. During the day, rapid photolysis (11 min lifetime for solar zenith angle < 20°) [ Stockwell and Calvert , ] limits HONO mixing ratios.…”