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Modeling the isotopic composition of H 2 with the TM5 model using a new photochemical scheme for production from CH 4 and VOCs. Gerben Pieterse, Maarten Krol and Thomas Röckmann
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Modeling the isotopic composition of H2 with the TM5 model using a new photochemical scheme for production from CH4 and VOCs Gerben Pieterse, Maarten Krol and Thomas Röckmann Atmospheric Physics and Chemistry Group, Institute for Marine and Atmospheric research (IMAU), Utrecht, The Netherlands. MODEL SETUP The TM5 model is a global offline chemistry–transport model with two-way nested zooming capability (Krol et al. 2005). The model is operated on a basic horizontal resolution of 6°- 4° globally with the possibility to zoom to 1°- 1° over regions of interest. We have recently included molecular hydrogen (H2) into the model, including its isotopologue HD. Surface emissions are used from EDGAR/HYDA datasets where possible. Photochemical sources are calculated based on the modified carbon bond mechanism (CBM). The deposition scheme is based on Sanderson et al., 2003. Isotope signatures for the surface sources are taken similar to the model study by Price et al., 2007. For the photochemical sources, we use either the bulk number given by Price et al., 2007, or the full photochemical mechanism based on functional group theory as described in the companion poster. Table 1 presents the budget of H2 and the isotope signatures used in the model. Note that in the explicit photochemistry run, the average of the two photochemical pathways for formaldehyde destruction from Feilberg et al., 2007 is used. The budget cannot be closed at present using the individual rate constants. RESULTS Figure 3 and 4 show the very first results of the new global H2 and HD modeling with TM5. Concentrations and isotope values are in a reasonable range, the interhemispheric gradient is modeled roughly correctly. Nevertheless, some unexpected features indicate that there are still some model errors (concentration minima in South America, Africa and the maritime continent up to Japan. Isotope minima over the VOC production regions. The latter indicate that isotope scheme as implemented at present has deficiencies and the investigation of such features will actually lead to interesting scientific results. Note that at the moment it is too early to draw scientific conclusions, because many aspects of the code still have to be checked, for example the VOC source field (see below). ADDITIONAL FUTURE POSSIBILITIES Model results will soon be compared to new data from the EUROHYDROS project. Since isotope chemistry of intermediate species is explicitly included, it will also be possible to model the isotope content of H2CO. SOURCE FIELDS Figures 5 and 6 show the global average fields of the main H2 precursors CH4 and isoprene (as indicator for VOC). The former is well validated and has been used in a recent inverse modeling study, the latter is very speculative and still has to be investigated. All VOC sources are initialized with the isotopic composition of CH4. STABILITY OF THE FIRST MODEL VERSION AND DEVELOPMENT OF THE PHOTOCHEMICAL CODE When the bulk number (Price et al., 2007) for the isotopic composition of the photochemical source is used, the global D values increase slightly, but not dramatically at the two stations Cape Grim, Tasmania and Barrow, Alasca(blue curve). The red and black curve show two implementations of a photochemical code. In the preliminary version, peroxy acetyl chemistry is not modeled correctly, global D values drop (red curve). in the full version (black curve), the D values stay approximately stable. References Feilberg, K. L., Johnson, M. S., and Nielsen, C. J.: Relative reaction rates of hcho, hcdo, dcdo, (hcho)-13c, and (hcho)-18o with oh, cl, br, and no3 radicals, J. Phys. Chem. A, 108, 7393-7398, 2004; Feilberg, K. L., Johnson, M. S., Bacak, A., Röckmann, T., and Nielsen, C. 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M., and Röckmann, T.: Hydrogen isotope fractionation in the photolysis of formaldehyde, Atm. Chem. Phys., 8, 1353-1366, 2008.; Röckmann, T., Rhee, T. S., and Engel, A.: Heavy hydrogen in the stratosphere, Atmos. Chem. Phys., 3, 2015-2023, 2003.