Modeling of the 11-year Solar Cycle Response in Upper Atmospheric Hydroxyl Radicals Yuk Yung 3-1-2012 ESE.

Slides:



Advertisements
Similar presentations
Steve Rumbold Keith Shine, Lesley Gray Charlotte Pascoe (CASE, RAL) Picture: Strat Hour - July 05, 2006 The University.
Advertisements

Cassini UVIS Update: He 584  Dayglow at Saturn Christopher Parkinson Ian Stewart and Yuk Yung January 05, 2006.
Photochemistry in the Atmospheres of Hot Jupiters Yuk L. Yung 1, Mao-Chang Liang 2, Michael Line 1 and Giovanna Tinetti 3 1 Division of Geological and.
AGU 2010 Fall Meeting GC21B-0880 Modeling the Observed Atmospheric OH Response to the Solar Cycle Shuhui Wang, Stanley P. Sander, Nathaniel J. Livesey,
Observing OH Response to the Solar Cycle  Over 5-year Aura MLS OH Measurements in Combination With the 13-year Ground-based FTUVS OH Measurement Shuhui.
29 April 2011Viereck: Space Weather Workshop 2011 The Recent Solar Minimum: How Low Was It? What Were The Consequences? Rodney Viereck NOAA Space Weather.
By David Gray.  Background ozone  ozone present through natural or nonlocal sources  currently ranges from ppb in North America  Rising background.
SBUV/2 Observations of Atmospheric Response to Solar Variations Matthew DeLand Science Systems and Applications, Inc. (SSAI) Background -SBUV/2 instruments.
CHAPTER 10: STRATOSPHERIC CHEMISTRY. THE MANY FACES OF ATMOSPHERIC OZONE Troposphere Stratosphere: 90% of total In stratosphere: UV shield In middle/upper.
Observed decadal scale changes in polar ozone suggest solar influence through energetic electron precipitation Björn-Martin Sinnhuber Institute of Environmental.
Figure 3. The MJO-related vertical structures of MACC CO. CO are averaged between 15ºN – 15ºS. Rainfall is averaged between 5ºN – 5ºS. ABSTRACT. We report.
Distribution of H 2 O and SO 2 in the atmosphere of Venus Yung Y. 1, Zhang X. 1, Liang M.-C. 2 and Parkinson C. 3 1 California Institute of Technology.
Using global models and chemical observations to diagnose eddy diffusion.
By studying the case with QBO signal only, the model reproduces the previous observation that QBO signal of column ozone at equator is anti-correlated.
Modeling Carbon Species in the Atmosphere of Neptune and Comparison with Spitzer Observations Xi Zhang 1, Mao-Chang Liang 2, Daniel Feldman 1, Julianne.
FACTORS GOVERNING THE SEASONAL VARIABILITY OF ATMOSPHERIC CARBONYL SULFIDE Parv Suntharalingam Harvard/Univ. of East Anglia A.J. Kettle, S. Montzka, D.
Modelling studies of metallic layers in the mesosphere using a GCM model Wuhu Feng 1,2, John Plane 1, Martyn Chipperfield 2, Dan Marsh 3, Diego Jaches.
The Atmosphere: Oxidizing Medium In Global Biogeochemical Cycles EARTH SURFACE Emission Reduced gas Oxidized gas/ aerosol Oxidation Uptake Reduction.
Modeling of OCS in the Lower Atmosphere of Venus Yuk L. Yung M. C. Liang, X. Jiang, C. Lee, B. Bezard and E. Marq California Institute of Technology
AGU 2006 Highlights Le Kuai Dec. 19, 2006 Le Kuai Dec. 19, 2006.
Chemical Sources and Sinks of OCS in the Lower Atmosphere of Venus Yuk L. Yung M. C. Liang, California Institute of Technology EGU.
Observing the Transition From NO x -Limited to NO x -Saturated O 3 Production J. A. Thornton 1, P. J. Wooldridge 1, R. C. Cohen 1, M. Martinez 2, H. Harder.
Solar Forcing on Climate Through Stratospheric Ozone Change Le Kuai.
1 Pedagogical Review on Solar Cycles King-Fai Li Caltech GPS, YL Yung Group Jan 17, 2007.
(a)(b)(c) Simulation of upper troposphere CO 2 from two-dimensional and three-dimensional models Xun Jiang 1, Runlie Shia 2, Qinbin Li 1, Moustafa T Chahine.
Langematz, Oberländer, Kunze Ulrike Langematz, Sophie Oberländer and Markus Kunze Institut für Meteorologie, Freie Universität Berlin, Germany The effects.
Solar Irradiance Variability Rodney Viereck NOAA Space Environment Center Derived Total Solar Irradiance Hoyt and Schatten, 1993 (-5 W/m 2 ) Lean et al.,
Photochemical Distribution of Venusian Sulphur and Halogen Species AND Why Vulcanism cannot be the source for Venusian SO 2 above 80km C. D. Parkinson.
New Insights into the Atmospheric Chemistry of Venus from Venus Express Yuk L. Yung Caltech GISS Seminar, Mar
Ozone Layer in the 21 st Century Swagath Navin Manohar.
Chemistry of Venus’ Atmosphere Vladimir A. Krasnopolsky Photochemical model for km Photochemical model for km Chemical kinetic model for.
Response of Middle Atmospheric Hydroxyl Radical to the 27-day Solar Forcing King-Fai Li 1, Qiong Zhang 2, Shuhui Wang 3, Yuk L. Yung 2, and Stanley P.
Comparison of Solar EUV Irradiance Measurements from CDS and TIMED/EGS W. T. Thompson L3 Communications EER, NASA GSFC P. Brekke ESA Space Science Department.
Solar Cycle 24 Carl Luetzelschwab K9LA QCWA Chap 36 April 2012 K9LA.
Upper Stratospheric and Lower Mesospheric HO x :Theory and Observations Tim Canty 1, Herb Pickett 2, Brian Drouin 2, Ken Jucks 3, Ross Salawith 2 HO x.
The Standard Solar Model and Experiments Predictions versus experiments Uncertainties in predictions Challenges and open questions BP00: astro-ph/
Seasonal variability of UTLS hydrocarbons observed from ACE and comparisons with WACCM Mijeong Park, William J. Randel, Louisa K. Emmons, and Douglas E.
Comparison of Magnesium II Core-to-Wing Ratio Measurements J. Machol 1,2*, M. Snow 3, R. Viereck 4, M. Weber 5, E. Richard 3, L. Puga 4 1 NOAA/National.
Investigation of Atmospheric Recycling Rate from Observation and Model James Trammell 1, Xun Jiang 1, Liming Li 2, Maochang Liang 3, Jing Zhou 4, and Yuk.
Understanding the Observed Ozone and Thermal Response To 11-Year Solar Variability Lon Hood Lunar and Planetary Laboratory University of Arizona Tucson,
1 AISC Workshop May 16-18, 2006 Lesson Learned from CCSP 1.1: Temperature Trends in the Atmosphere Lesson Learned from CCSP 1.1 Temperature Trends in the.
IAC ETH, 26 October 2004 Sub-project: Effects of Solar irradiance variability on the atmosphere (steady-state sensitivity study) Progress report (final)
TOSCA workshop, Berlin, 15 May 2012 Comparison of the SSI data sets using observed and simulated evolution of the middle atmosphere during A.
Camp et al. (2003) illustrated that two leading modes of tropical total ozone variability exhibit structrures of the QBO and the solar cycle. Figure (1)
Multi-model intercomparison of the impact of SORCE measurements in climate models TOSCA WG1 Workshop May 2012, Berlin K. Matthes (1), J.D. Haigh.
SPEAKERS: Gabriele Pfister, Scientist III, National Center for Atmospheric Research (NCAR) Brad Pierce, Physical Scientist, NOAA Salient Questions: 1.What.
 We also investigated the vertical cross section of the vertical pressure velocity (dP/dt) across 70°W to 10°E averaged over 20°S-5°S from December to.
Validation of OMI NO 2 data using ground-based spectrometric NO 2 measurements at Zvenigorod, Russia A.N. Gruzdev and A.S. Elokhov A.M. Obukhov Institute.
SOLSTICE II -- Magnesium II M. Snow 1*, J. Machol 2,3, R. Viereck 4, M. Weber 5, E. Richard 1 1 Laboratory for Atmospheric and Space Physics, University.
Yuk Yung (Caltech), M. C. Liang (Academia Sinica), X. Zhang (Caltech),
Exploring Planets and Earth Yuk Ling Yung Caltech.
The impact of solar variability and Quasibiennial Oscillation on climate simulations Fabrizio Sassi (ESSL/CGD) with: Dan Marsh and Rolando Garcia (ESSL/ACD),
Spectroscopy and Radiative Transfer – Application to Martian atmosphere Helen Wang Smithsonian Astrophysical Observatory April 2012.
METO 621 CHEM Lesson 4. Total Ozone Field March 11, 1990 Nimbus 7 TOMS (Hudson et al., 2003)
(a)(b)(c) Simulation of upper troposphere CO 2 from two-dimensional and three-dimensional models Xun Jiang 1, Runlie Shia 2, Qinbin Li 1, Moustafa T Chahine.
Variability of CO 2 From Satellite Retrievals and Model Simulations Xun Jiang 1, David Crisp 2, Edward T. Olsen 2, Susan S. Kulawik 2, Charles E. Miller.
Night OH in the Mesosphere of Venus and Earth Christopher Parkinson Dept. Atmospheric, Oceanic, and Space Sciences University of Michigan F. Mills, M.
A global model of meteoric metals and smoke particles: An update  Model for metal layers and MSPs  Validation of model results  Sensitivities/uncertainties.
Fifth Workshop on Titan Chemistry April 2011, Kauai, Hawaii Organic Synthesis in the Atmosphere of Titan: Modeling and Recent Observations Yuk Yung.
Upgrade from SGP V5.02 to V6.00: Conclusions from delta-validation of Diagnostic Data Set D. Hubert, A. Keppens, J. Granville, F. Hendrick, J.-C. Lambert.
What Are the Implications of Optical Closure Using Measurements from the Two Column Aerosol Project? J.D. Fast 1, L.K. Berg 1, E. Kassianov 1, D. Chand.
Non-LTE atmosphere calculations of the solar spectrum
Updates on Solar Signal in the Stratospheric Ozone using a 3D CTM and SAGE v7.0 data Sandip Dhomse, Martyn Chipperfiield, Wuhu Feng, Ryan Hossaini, Graham.
Nowcasting of neutral and ion composition of the mesosphere:
Thermosphere-Ionosphere Issues for DASI - I:
Absolute calibration of sky radiances, colour indices and O4 DSCDs obtained from MAX-DOAS measurements T. Wagner1, S. Beirle1, S. Dörner1, M. Penning de.
Model Uncertainties: IPCC GCMs
Variability of CO2 From Satellite Retrievals and Model Simulations
大气圈地球化学及其环境效益.
Dr. Matthias Lüdeke, Potsdam Institut für Klimafolgenforschung
Presentation transcript:

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