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Published byLynn Marshall Modified over 9 years ago
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Solar Variability and Climate: From Mechanisms to Models
Terry Nathan Atmospheric Science Program University of California, Davis OUTLINE SUN-CLIMATE CONNECTIONS CHALLENGES 11-YEAR SOLAR FORCING KEY CIRCULATION COMPONENTS OF CLIMATE SYSTEM SOLAR VARIABILITY, OZONE AND WAVES PATHWAYS AND INTERFACES FUTURE ILWS 2009, Brazil
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SUN-CLIMATE CONNECTIONS
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Global Average Radiative Forcing (RF) Estimates
LOSU Level of Scientific Understanding IPCC 4th Assessment Report 2007
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Paleo Sun–Climate Synopsis
…when solar activity is high…. increased temperature & moisture SW Alaska Sheng et al., 2003 drought Western US Cookl et al., 2001 warming North Atlantic Bond et al., 2000 stronger monsoon Wangxiang cave Zhang et al., 2008 high rainfall Oman Neff et al., 2001 drought Equatorial East Africa Verschuren et al., 2000 Mayan drought Cariaco Basin Hodell et al., 2001 Haug et al., 2003 weakened upwelling and trade winds (warmer SSTs) Cariaco Basin Black et al., 1999 warming Beijing Tan et al., 2004 streamflow Parana River Mauas et al., 2008. tree-rings Chile Roig et al., 2001 Nordemann et al. warming Tasmania Hill et al., 2007 Courtesy J. Lean significant local changes do not imply global changes of equal magnitude
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Natural and Anthropogenic Change in Earth’s Atmosphere
2km LOWER TROPOSPHERE 5km MID TROPOSPHERE 19km LOWER STRAT Courtesy of Judith Lean 5
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11-YEAR SOLAR FORCING - Total solar irradiance (TSI) changes
Solar spectral irradiance (SSI) changes - 11-year solar cycle modulation in high energy particles (e.g., solar protons, galactic cosmic rays)
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CHALLENGES - TSI Variations <0.1%
- Identification of pathways that communicate and amplify solar variability throughout the atmosphere and oceans Address discrepancies between models and observations
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Total Solar Irradiance (TSI) changes
<0.1% YEAR From Lean, Ann. Rev of Astron. & Astrophys., 1997
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Solar Spectral Irradiance (SSI) changes
Variations in SSI over the Solar Cycle 8% 4% 20% 0.5% From Lean, Ann. Rev of Astron. & Astrophys., 1997 Stratospheric Ozone Heating Rates Adapted from Strobel (1978) JGR
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KEY CIRCULATION COMPONENTS OF CLIMATE SYSTEM
Quasi-biennial oscillation (QBO) Hadley circulation, subtropical jets… - Stratospheric polar vortex Brewer-Dobson circulation Planetary waves ……..
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Quasi-biennial Oscillation (QBO)
Time–height plot of equatorial zonal wind (u) in m/s between about 20 and 35 km altitude above sea level over a ten-year period. Positive values denote westerly winds and the contour line is at 0 m/s. After Holton et al
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Hadley Circulation, Subtropical Jets …
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Stratospheric Polar Vortex
Pole 660
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Brewer-Dobson Circulation
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Stratospheric Polar Vortex Vertically Propagating Planetary Waves
Brewer-Dobson Vertically Propagating Planetary Waves WAVE DRAG
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SOLAR VARIABILITY, OZONE AND WAVES
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Connection between SSI and PWD
Variations in Solar Spectral Irradiance PWD Zonal-Mean Variations in Ozone Heating “TRADITIONAL” Longitudinal Variations in Ozone Heating “NEW” Planetary Wave Drag (propagation / attenuation) Why is PWD so important? Zonal-Mean Flow Residual Mean Meridional Circulation, PWD Vertically Propagating Wave EP-Flux Divergence F = Fyj Fzk momentum flux heat flux
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WKB Solution for EP-Flux Divergence (1-D)
SSI-Modified Vertical Wavenumber (Refractive Index) SSI-Modified Planetary Wave Drag Zonal-Mean Flow Equation Nonlinear function of SSI
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Ozone-Modified Downward Control
Residual Vertical Velocity “Downward Control” To what extent is the divergence of Eliassen-Palm flux (i.e., PWD) affected by the solar-modulated, planetary wave induced ozone heating? Adapted from Holton 2004
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PATHWAYS AND INTERFACES
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Variations in SSI and TSI - Solar Proton Events – Cosmic Rays
Impacts on Upper Atmospheric Chemistry and Dynamics Direct RF of the Lower Atmosphere Tropical Upwelling Downwelling Quasi-biennial Oscillation QBO Polar Vortex Middle Atmosphere OZONE OZONE Vertically Propagating Planetary Waves PWD Vertically Propagating Tropical Waves WD 450 latitude clouds HADLEY clouds clouds clouds Surface Troposphere EQUATOR POLE
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FUTURE
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