Infrared spectroscopy of halogen-containing species for atmospheric remote sensing Jeremy J. Harrison University of York Atmospheric Chemistry Experiment (ACE) FTS: 750 to 4400 cm-1 Radiance of sun gives high S/N Long pathlengths ~ 300 km (limb sounding) Measurements at many altitudes ACE detects more trace organic molecules than any other satellite instrument. Halocarbons Strong greenhouse gases Many are ozone depleting substances – Regulated by the Montreal Protocol Many are increasing in the atmosphere Many have long atmospheric lifetimes Laboratory Spectroscopy GEISA and HITRAN contain a number of absorption cross section datasets for Cl- and F-containing molecules Dataset requirements for remote sensing: – – – – Accurate band intensities Accurate wavenumber scale Wide P-T coverage for best interpolation Appropriate resolution (Doppler-limited) A number of GEISA / HITRAN datasets fail in many of these respects. MSF at RAL Bruker IFS 125 HR 26-cm absorption cell CFC-12 (CCl2F2) Most abundant anthropogenic halocarbon in the atmosphere Was used in refrigeration and air conditioning Banned under the Montreal Protocol Atmospheric lifetime ~ 100 years MIPAS: Kellmann et al., ACP, 12, 11857–11875, 2012 CFC-12 absorption cross sections in HITRAN / GEISA CCl2F2 cross sections CCl2F2 (CFC-12) Main problems with old dataset: – Strong Q branch near 1160 cm-1 often saturated. – Wavenumber calibration error CCl2F2 cross sections CCl2F2 cross sections Carbon tetrachloride CCl4 accounted for 359 ppt (about 11%) of total tropospheric Cl in 2008 CCl4 tropospheric abundances have declined less rapidly than expected Atmospheric lifetime 26 years Top-down emissions 40–80 Gg/yr (2005–2008) Bottom-up emissions 0–30 Gg/yr (2005–2008) Errors in reporting, errors in the analysis of reported data, and/or unknown sources? ACE-FTS CCl4 data product biased ~20% high CCl4 absorption cross sections in HITRAN / GEISA CCl4 cross sections CCl4 Main problems with old dataset: – Spectra under-resolved – Wavenumber calibration error CCl4 cross sections CCl4 cross sections HCFC-22 (CHClF2) Most abundant HCFC (substitutes for long-lived ozone-depleting substances) Lifetime 11.9 years HCFC-22 increased at a rate of about 8 ppt/yr (4.3%/yr) during 2007–2008, more than 50% faster than observed in 2003–2004 – Rapidly increasing HCFC-22 production in developing countries Emissions are projected to begin to decline during the coming decade due to measures already agreed to under the Montreal Protocol HCFC-22 absorption cross sections in HITRAN / GEISA CHClF2 cross sections CHClF2 (HCFC-22) Main problems with old dataset: – Poor P-T coverage – Wavenumber calibration error CHClF2 cross sections Hydrofluorocarbons (HFCs) Hydrofluorocarbons (HFCs) are replacements for CFCs and HCFCs – Not regulated by Montreal Protocol Trifluoromethane (HFC-23, CHF3) – – – – Second most abundant HFC in atmosphere Lifetime of 222 years 100-year GWP of 14,200 Formed as a by-product of HCFC-22 (CHClF2) production 1,1,1,2-Tetrafluoroethane (HFC-134a, CF3CH2F) – – – – Most abundant HFC in atmosphere Lifetime of 13.4 years 100-year GWP of 1,370 The preferred refrigerant in refrigeration and mobile air conditioning (replacement for CFC-12) Previous HFC-23 absorption cross sections Remote-sensing observations of HFC-23 Harrison et al., First remote-sensing observations of trifluoromethane (HFC-23) in the upper troposphere and lower stratosphere, J. Geophys. Res., 2012, 117, D05308, doi:10.1029/2011JD016423. CHF3 cross sections New dataset: Harrison, JQSRT 130, 359-364 (2013) Main problems with old dataset: CHF3 (HFC-23) – – – – Very poor P-T coverage Spectra under-resolved Inconsistent baselines Wavenumber calibration error Remote-sensing observations of HFC-134a Nassar et al., J. Geophys. Res., 2006, 111, D22313, doi:10.1029/2006JD007395. HFC-134a absorption cross sections in HITRAN / GEISA CF3CH2F cross sections Main problems with old dataset: – Poor P-T coverage – Wavenumber calibration error CF3CH2F (HFC-134a) CF3CH2F cross sections Acknowledgements Funding from NERC (UK) & NCEO RAL – Gary Williams & Robert McPheat NCEO – John Remedios ACE – Chris Boone & Peter Bernath
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