The uptake of HNO3 on meteoric smoke analogues

The uptake of HNO3, H2O, NO2 and NO was studied on meteoric smoke particle analogues using a low-pressure Knudsen cell operating at 295K. The analogues used were olivine (MgFeSiO4) and a haematite/goethite (Fe2O3/FeO(OH)) mixture synthesised by the sol-gel process. For uptake on MgFeSiO4, the following uptake coefficients were obtained: γ(HNO3)=(1.8±0.3)×10-3, γ(H2O)=(4.0±1.3)×10-3, γ(NO2)=(5.7±0.2)×10-4 and γ(NO)<3×10-4. γ(HNO3) did not show a dependence on the mass of MgFeSiO4 in the Knudsen cell (when varied by a factor of 6) implying that, because of relatively efficient uptake, HNO3 is removed only by near-surface particles. This was corroborated by application of a surface uptake model. Saturating the MgFeSiO4 particles with water vapour before exposing them to NO2 increased γ(NO2) to (2.1±0.7)×10-3, but had a very small effect on γ(HNO3). For uptake on Fe2O3/FeO(OH), γ(HNO3)=(1.5±0.2)×10-3. These results were then included in a whole atmosphere chemistry-climate model, which shows that the heterogeneous removal on meteoric smoke particles in the winter polar vortex between 30 and 60km appears to provide an important sink for HNO3.