Modeling of the 11-year Solar Cycle Response in Upper Atmospheric Hydroxyl Radicals Yuk Yung ESE
The solar-cycle modulation recently reported by Shuhui Wang et al. (2011) OH column shows 10±3 % Modeled OH column response using previous solar model predicts 3.7 % only Recent satellite UV measurements show unexpectedly large 11-year solar-cycle variability Motivation NRL FluxSORCE Flux
An “Error Estimation” (Conservative) 5% SOLSTICE 2% SIM Error estimates are as important as the measured means Spectral uncertainty should also propagate in the models Very very conservative uncertainty limits will be tested
Backward Extrapolation Extrapolate to the solar max in Jan 2002 using Mg-II index Uncertainty = regression error + instrument uncertainty
OH Photochemistry A A BB C C D A: H 2 O photolysis B: OH + O( 3 P) → H + O 2 O( 3 P) comes from photolysis of O 2 and O 3. C. H 2 O + O( 1 D) → OH + O 2 O( 1 D) comes from the photolysis of O 3 + h → O 2 + O( 1 D). D. Shielding effect due to the increased overhead O 3 opacity
Modeled Response (1D) (Blue) Solar-cycle modulation using the extrapolated UV changes (Shade) Uncertainty related to extrapolation (Black) Simulation using Lean’s spectrum (Orange) Canty and Minschwaner (2007). OH column = 6.4 ± 2.5 % versus obs 10 ± 3%
Modeled Response (3D)
Simulated solar response of the mid-latitude OH column abundance is much closer to observations when the latest satellite solar UV measurements are used. Nevertheless, the observed solar response is still slightly greater than the simulated value. Future OH measurements through the next solar maximum (expected in 2013) will be extremely valuable for investigating these differences further. Summary
Daytime Merkel et al. (2011) How about O 3 ? Merkel et al. examined the effect in the lower mesosphere Stratosphere ??? Continuous satellite measurements too short
Ground-based measurements LIDAR O 3 measurement over Mauna Loa, Hawaii (MLO) MLO agrees with 1D/2D photochemical models Max level of WACCM is wrong WACCM zero level too low
O 3 chemistry is much simpler
Acknowledgements NASA and ESA Yung’s Group at Caltech Fai Li, Stan Sander, Shuhui Wang Yung and DeMore (1999) Book