Atmospheric Chemistry and Physics (Oct 2011)

Quantification of the unknown HONO daytime source and its relation to NO<sub>2</sub>

  • M. Martinez,
  • Z. Hosaynali-Beygi,
  • H. Harder,
  • A. Held,
  • H. Fischer,
  • F. Drewnick,
  • J.-M. Diesch,
  • H. Bozem,
  • E. Regelin,
  • M. Sörgel,
  • C. Zetzsch

DOI
https://doi.org/10.5194/acp-11-10433-2011
Journal volume & issue
Vol. 11, no. 20
pp. 10433 – 10447

Abstract

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During the DOMINO (Diel Oxidant Mechanism In relation to Nitrogen Oxides) campaign in southwest Spain we measured simultaneously all quantities necessary to calculate a photostationary state for HONO in the gas phase. These quantities comprise the concentrations of OH, NO, and HONO and the photolysis frequency of NO2, j(NO2) as a proxy for j(HONO). This allowed us to calculate values of the unknown HONO daytime source. This unknown HONO source, normalized by NO2 mixing ratios and expressed as a conversion frequency (% h−1), showed a clear dependence on j(NO2) with values up to 43% h−1 at noon. We compared our unknown HONO source with values calculated from the measured field data for two recently proposed processes, the light-induced NO2 conversion on soot surfaces and the reaction of electronically excited NO2* with water vapour, with the result that these two reactions normally contributed less than 10% (2 + soot + hν; and 2* + H2O) to our unknown HONO daytime source. OH production from HONO photolysis was found to be larger (by 20%) than the "classical" OH formation from ozone photolysis (O(1D)) integrated over the day.