exploring the stratospheric/tropospheric response to solar forcing

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Exploring the stratospheric/tropospher ic response to solar forcing D. Rind et al. 2010/03/30 Pei-Yu Chueh

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Exploring the stratospheric/tropospheric response to solar forcing. D. Rind et al. 2010/03/30 Pei-Yu Chueh. Introduction. Higher values in the upper troposphere are reported, seen most clearly during June-August although present on the annual average. - PowerPoint PPT Presentation

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Page 1: Exploring the stratospheric/tropospheric response to solar forcing

Exploring the stratospheric/tropospheric response to solar forcing

D. Rind et al.

2010/03/30 Pei-Yu Chueh

Page 2: Exploring the stratospheric/tropospheric response to solar forcing

Introduction

• Higher values in the upper troposphere are reported, seen most clearly during June-August although present on the annual average.

• There are disagreements as to whether the tropical region warms, or primarily the subtropical through mid-latitudes.

• Precipitation increased in July and August in the tropical western Pacific, and the various monsoon regions.

Page 3: Exploring the stratospheric/tropospheric response to solar forcing

Introduction1. Meehl et al. reported that in their model increased solar irradiance

over land during summer solar maximum conditions helped intensify the monsoons, and more solar radiation over cloud free regions increased evaporation and moisture convergence.(atmospheric response)

2. Van Loon et al. suggested that TSI forcing in the subtropics created temperature gradients and wind conditions that excite an ocean dynamical response, particularly that associated with La nina during Northern Hemisphere winter.(ocean dynamical heating)

3. The influence of UV variations in the stratosphere, which is known to respond to solar forcing with warming and increased ozone during solar maximum conditions.

Page 4: Exploring the stratospheric/tropospheric response to solar forcing

Model experiments

• Calculated SST• Historical SST• Climatological Average SST

Page 5: Exploring the stratospheric/tropospheric response to solar forcing

Do the Standard Runs Reproduce the ObservedStratospheric and Tropospheric Temperature

Changes?

+0.7

+0.2

0.2C, are about half that derived from NCEP reanalysis.

(right) warming similar to that in the annual average occurs in the stratosphere, although now all three models also show more cooling at Southern Hemisphere upper mid-latitudes in the low stratosphere to mid-stratosphere, in agreement with NCEP reanalysis observations.

Page 6: Exploring the stratospheric/tropospheric response to solar forcing

Do the DSST in the Calculated Ocean Runs MatchThose in the Historical Data?

• They all show warming in the North Pacific.

• There is greater widespread warming with the historical SST.

• Greater warming north of the equator

Page 7: Exploring the stratospheric/tropospheric response to solar forcing

Do the Standard Runs Produce the ObservedOzone Difference, and if Not, What Difference

Does It Make?

• with peak ozone change of close to 2% in the mid-stratosphere, not in the upper stratosphere as suggested by observations.

• Interestingly, this run did show ozone increases in the extratropical lower stratosphere of both hemispheres, associated with altered dynamical transports, although not in the tropical lower stratosphere as observed

no photochemical response

Page 8: Exploring the stratospheric/tropospheric response to solar forcing

Does Model Resolution Make a Difference?

• high correlations of ozone and solar UV radiation above the stratopause, minimum correlation (though still positive) around 50 km, and greater correlation in the mid-stratosphere.

• maximum correlation in the subtropical lower stratosphere• the negative correlation in the tropical lower stratosphere

We find no evidence of this in our simulations.

Page 9: Exploring the stratospheric/tropospheric response to solar forcing

Do the Other Forcings Make a Difference?

• The tropospheric response is clearly larger with anthropogenic forcing as expected, but the stratospheric response has been largely erased, as increasing CO2 acts to cool the stratosphere.

Page 10: Exploring the stratospheric/tropospheric response to solar forcing

Do the Circulation Changes Match Those Claimedfor Solar Forcing?

• Extratropical cooling in the Southern Hemisphere stratosphere increased thermal gradient strengthens west winds, consistent with observations.

In general, the changes in dynamics associated with solar forcing are weak, and in the troposphere usually not statistically significant.

Page 11: Exploring the stratospheric/tropospheric response to solar forcing

Do the Circulation Changes Match Those Claimedfor Solar Forcing?

• Relative rising air can be seen around 50S in all the cases.

• Descent occurs at high southern latitudes, and, in the stratosphere during JJA.

• On the annual average, the most consistent descent in the NH occurs around 45N, extending down into the troposphere.

The annual average descent in the Northern mid-latitudes should impact precipitation.

Page 12: Exploring the stratospheric/tropospheric response to solar forcing

Do the Precipitation Changes Match ThoseClaimed for Solar Forcing?

• Precipitation increases in this region north of the equator, and decreases in the vicinity of the equator, although again the magnitudes are small.

• The precipitation increase occurs not only in the western Pacific region, but also at latitudes 10N-18N across the globe.

• Similarly there is a small precipitation decrease near the equator.

Page 13: Exploring the stratospheric/tropospheric response to solar forcing

Do the Precipitation Changes Match ThoseClaimed for Solar Forcing?

• During solar maximum conditions, precipitation preferentially shifts north of the equator, with a corresponding decrease to the south.

• on the annual average, especially with climatological SST, reduced precipitation at northern midlatitudes (at solar maximum) is apparent in the majority of cases, although this is not true with historical SST.

Page 14: Exploring the stratospheric/tropospheric response to solar forcing

Discussion-Stratosphere

• Upper Stratosphere : Reanalysis data in the upper stratosphere suggest some solar-driven warming, but the magnitude vary among the different studies.

• Midstratosphere : Model change max, but satellite data indicate should have min.→ different ozone profiles

• Lower Stratosphere : Reanalysis data in the lower stratosphere suggest some solar-driven warming, although the magnitude and actual location vary among the different studies, ranging from small to substantial, and from tropical to subtropical.

• SST Influence : SST doesn’t play a significant role, probably because in the solar case, the forcing is greatest in the stratosphere and the SST response is small.

Page 15: Exploring the stratospheric/tropospheric response to solar forcing

Discussion-Tropospheric Response

• Temperature : The reports of solar-driven tropospheric warming estimated from observations are somewhat inconsistent among the various studies.

• Precipitation : 1. reduction of precipitation near and to the south of the equator, with

increases off the equator, especially to the north over Southern Asia during solar cycle maximum.

2. precipitation reduction at northern midlatitudes.

• Circulation : Consistent with the precipitation changes, greater subsidence south of the equator does occur in association with increased solar activity.