Infrared radiation and planetary temperature

Physics Today AIP Publishing 64:1 (2011) 33-38

Multimodel climate and variability of the stratosphere

Journal of Geophysical Research Atmospheres 116:5 (2011)

Authors:

N Butchart, AJ Charlton-Perez, I Cionni, SC Hardiman, PH Haynes, K Krüger, PJ Kushner, PA Newman, SM Osprey, J Perlwitz, M Sigmond, L Wang, H Akiyoshi, J Austin, S Bekki, A Baumgaertner, P Braesicke, C Brhl, M Chipperfield, M Dameris, S Dhomse, V Eyring, R Garcia, H Garny, P Jöckel, JF Lamarque, M Marchand, M Michou, O Morgenstern, T Nakamura, S Pawson, D Plummer, J Pyle, E Rozanov, J Scinocca, TG Shepherd, K Shibata, D Smale, H Teyssèdre, W Tian, D Waugh, Y Yamashita

Abstract:

The stratospheric climate and variability from simulations of sixteen chemistry-climate models is evaluated. On average the polar night jet is well reproduced though its variability is less well reproduced with a large spread between models. Polar temperature biases are less than 5 K except in the Southern Hemisphere (SH) lower stratosphere in spring. The accumulated area of low temperatures responsible for polar stratospheric cloud formation is accurately reproduced for the Antarctic but underestimated for the Arctic. The shape and position of the polar vortex is well simulated, as is the tropical upwelling in the lower stratosphere. There is a wide model spread in the frequency of major sudden stratospheric warnings (SSWs), late biases in the breakup of the SH vortex, and a weak annual cycle in the zonal wind in the tropical upper stratosphere. Quantitatively, "metrics" indicate a wide spread in model performance for most diagnostics with systematic biases in many, and poorer performance in the SH than in the Northern Hemisphere (NH). Correlations were found in the SH between errors in the final warming, polar temperatures, the leading mode of variability, and jet strength, and in the NH between errors in polar temperatures, frequency of major SSWs, and jet strength. Models with a stronger QBO have stronger tropical upwelling and a colder NH vortex. Both the qualitative and quantitative analysis indicate a number of common and long-standing model problems, particularly related to the simulation of the SH and stratospheric variability. Copyright 2011 by the American Geophysical Union.

On the persistence and predictability properties of north atlantic climate variability

Journal of Climate 24:2 (2011) 466-472

Authors:

C Franzke, T Woollings

Abstract:

The persistence and climate noise properties of North Atlantic climate variability are of importance for trend identification and assessing predictability on all time scales from several days to many decades. Here, the authors analyze these properties by applying empirical mode decomposition to a time series of the latitude of the North Atlantic eddy-driven jet stream. In previous studies, it has been argued that a slow decay of the autocorrelation function at large lags suggests potential extended-range predictability during the winter season. The authors show that the increased autocorrelation time scale does not necessarily lead to enhanced intraseasonal predictive skill. They estimate the fraction of interannual variability that likely arises due to climate noise as 43%-48% in winter and 70%-71% in summer. The analysis also indentifies a significant poleward trend of the jet stream that cannot be explained as arising from climate noise. These findings have important implications for the predictability of North Atlantic climate variability. © 2011 American Meteorological Society.

Solar signal propagation: The role of gravity waves and stratospheric sudden warmings

Journal of Geophysical Research Atmospheres 116:2 (2011)

Authors:

I Cnossen, H Lu, CJ Bell, LJ Gray, MM Joshi

Abstract:

We use a troposphere-stratosphere model of intermediate complexity to study the atmospheric response to an idealized solar forcing in the subtropical upper stratosphere during Northern Hemisphere (NH) early winter. We investigate two conditions that could influence poleward and downward propagation of the response: (1) the representation of gravity wave effects and (2) the presence/absence of stratospheric sudden warmings (SSWs). We also investigate how the perturbation influences the timing and frequency of SSWs. Differences in the poleward and downward propagation of the response within the stratosphere are found depending on whether Rayleigh friction (RF) or a gravity wave scheme (GWS) is used to represent gravity wave effects. These differences are likely related to differences in planetary wave activity in the GWS and RF versions, as planetary wave redistribution plays an important role in the downward and poleward propagation of stratospheric signals. There is also remarkable sensitivity in the tropospheric response to the representation of the gravity wave effects. It is most realistic for GWS. Further, tropospheric responses are systematically different dependent on the absence/presence of SSWs. When only years with SSWs are examined, the tropospheric signal appears to have descended from the stratosphere, while the signal in the troposphere appears disconnected from the stratosphere when years with SSWs are excluded. Different troposphere-stratosphere coupling mechanisms therefore appear to be dominant for years with and without SSWs. The forcing does not affect the timing of SSWs, but does result in a higher occurrence frequency throughout NH winter. Quasi-Biennial Oscillation effects were not included. Copyright 2011 by the American Geophysical Union.

The solar influence on the probability of relatively cold UK winters in the future

Environmental Research Letters 6:3 (2011)

Authors:

M Lockwood, RG Harrison, MJ Owens, L Barnard, T Woollings, F Steinhilber

Abstract:

Recent research has suggested that relatively cold UK winters are more common when solar activity is low (Lockwood et al 2010 Environ.Res.Lett. 5 024001). Solar activity during the current sunspot minimum has fallen to levels unknown since the start of the 20th century (Lockwood 2010 Proc. R. Soc. A 466 303-29) and records of past solar variations inferred from cosmogenic isotopes (Abreu et al 2008 Geophys.Res.Lett. 35 L20109) and geomagnetic activity data (Lockwood et al 2009 Astrophys. J. 700 937-44) suggest that the current grand solar maximum is coming to an end and hence that solar activity can be expected to continue to decline. Combining cosmogenic isotope data with the long record of temperatures measured in central England, we estimate how solar change could influence the probability in the future of further UK winters that are cold, relative to the hemispheric mean temperature, if all other factors remain constant. Global warming is taken into account only through the detrending using mean hemispheric temperatures. We show that some predictive skill may be obtained by including the solar effect. © 2011 IOP Publishing Ltd.