S. Oberländer and co-authors investigate the different processes affecting the Brewer Dobson Circulation in future using the EMAC chemistry-climate model in a new JGR article. Using several sensitivity simulations they isolate the effects of external forcings such as greenhouse gases, sea surface temperatures (SSTs) and ozone-depleting substances. They find that in boreal winter the tropical upward mass flux increases by about 1%/decade (2%/decade) in the upper (lower) stratosphere until the end of the 21^st century. The mean stratospheric age of air decreases by up to 60 and 30 days/decade, respectively. Changes in transient planetary and synoptic waves account for the strengthening of the BDC in the lower stratosphere, whereas upper stratospheric changes are due to improved propagation properties for gravity waves in future climate. The radiative impact of increasing GHG concentrations is detected only in the upper stratosphere, whereas the effect of increasing SSTs dominates the lower stratospheric signal. Changes in tropical SSTs influence not only the shallow but also the deep branch of the BDC as confirmed from both changes in residual circulation and mixing. Declining ODSs were found to slightly counteract the BDC increase in the Southern Hemisphere. The full abstract can be found here.

Some of the first results from the SPARC Data Initiative to be published, this new article by M.I. Hegglin and co-authors in JGR compares the water vapour climatologies from various satellite limb sounders for the period 1978-2010. Monthly zonal means from LIMS, SAGE II, UARS-MLS, HALOE, POAM III, SMR, SAGE III, MIPAS, SCIAMACHY, ACE-FTS, and Aura-MLS were calculated on a common latitude-pressure grid and then compared with the multi-instrument mean. Evaluations include comparisons of monthly or annual zonal mean cross-sections and seasonal cycles in the tropical and extra-tropical upper troposphere and stratosphere, comparisons of interannual variability, and the study of features such as the water vapour tape recorder. The instruments agree best in the mid-latitude and tropical middle and lower stratosphere, with a relative uncertainty of ±2–6% (as quantified by the standard deviation of the instruments’ multi-annual means). The uncertainty increases toward the polar regions (±10–15%), the mesosphere (±15%), and the upper troposphere/lower stratosphere below 100 hPa (±30–50%), where sampling issues add uncertainty due to large gradients and high natural variability in water vapour. The knowledge gained from these comparisons and regarding the quality of the individual data sets in different regions of the atmosphere will help to improve model-measurement comparisons (e.g., for diagnostics such as the tropical tape recorder or seasonal cycles), data merging activities, and studies of climate variability. The full abstract can be found here.

Using high-precision measurements of the isotopic ratios of N2, O2, and Ar, as well as the mole fraction of Ar, S. Ishidoya and co-authors show that gravitational separation occurs in the stratosphere below the turbopause. Observed vertical profiles agree well with those expected theoretically from molecular mass differences. Simulations with a 2D model of the middle atmosphere indicate that a relationship between gravitational separation and stratospheric age-of-air would be significantly affected if the Brewer Dobson Circulation was enhanced. Therefore they suggest that gravitational separation could serve as a new indicator of changes in stratospheric circulation. The full abstract can be found here.

At a press conference held today in Stockholm, Sweden, the Summary for Policymakers of the Working Group I contribution of AR5 on Climate Change 2013: The Physical Science Basis was presented by the Co-Chairs Dahe Qin and Thomas Stocker.

Find the presentation by Dahe Qin and Thomas Stocker, IPCC Working Group I Co-Chairs.

Find the Summary for Policy Makers and approved final draft of the Scientific-technical Report; of particular interest to the SPARC community are Chapter 2 on Observations: Atmosphere and Surface, and Chapter 7 on Clouds and Aerosols.

Find online registration and programme at http://royalsociety.org/events/2013/climatescience-next-steps/

Find full report at http://www.ncdc.noaa.gov/bams-state-of-the-climate/2012.php.

A new ACP article by N.A. Kramarova and co-authors presents a validation of ozone profiles from the Solar Backscatter Ultraviolet (SBUV and SBUV/2) instruments that were recently reprocessed using an updated (version 8.6) algorithm. The SBUV data record covers the period 1970-2011, with a 5 year gap in the 1970s. Validation with MLS (on board the UARS and Aura satellites) and SAGE-II satellite observations, as well as ground-based observations from microwave spectrometers, lidars, Umkehr instruments and balloon-borne ozonesondes. They find that in the stratosphere, between 25 and 1 hPa, the mean biases and standard deviations are mostly within 5% for monthly zonal mean ozone profiles. Above and below this layer the vertical resolution of the SBUV algorithm decreases. In order to account for the lower resolution in the troposphere/lower stratosphere, they combine several layers of data. The drift of the SBUV instruments is also estimated, as well as its potential effect on the long-term stability of the combined data record. The features of individual SBUV(/2) instruments are discussed and recommendations for creating a merged SBUV data set are provided. The full abstract can be found here.

A recent JGR article by J. Hsu and co-authors uses the NCAR Community Atmosphere Model to evaluate the sensitivity of stratospheric dynamics to the uncertainty in ozone production related to uncertainty in O2 cross-sections in the Hertzberg Continuum. Reducing the O2 cross-sections by 30% is found to increase ozone abundances in the lower stratosphere, which as a result warms between 60°S -60°N (2K maximum at the equator) and lowers the tropopause height by 100-200m between 30°S -30°N. The study points to the important role of ozone in the lower tropical stratosphere in determining the physical characteristics of the tropical tropopause layer. The full abstract can be found here.

The effects of imposed stratospheric cooling on the maximum intensity of tropical cyclones

Using a cloud-resolving model, H. Ramsay presents results that elucidate the effect of stratospheric cooling and sea surface warming on the potential intensity (PI) of tropical cyclones in a recent article in the Journal of Climate. With fixed sea surface temperatures, cooling near and above the tropopause (~90hPa) is shown to increase PI at a rate of 1m/s per degree cooling. With fixed stratospheric temperatures, sea surface warming increases the PI by approximately twice as much, as a rate of about 2m/s per degree warming. These results have significant implications in terms of global tropical cyclone PI trends in response to climate change. Tropical sea surface temperatures have warmed by about 0.15K/decade since the 1970s, while the stratosphere has cooled anywhere from 0.3K/decade to over 1K/decade, depending on the data set used. Therefore, global PI trends in recent decades appear to have been driven more by stratospheric cooling than by surface warming. Find the full abstract here.

Drivers of hemispheric differences in return dates of mid-latitude stratospheric ozone

In a new ACP paper, H. Garny and co-authors investigate the main factors driving the hemispherical asymmetry in ozone return dates. They find that the hemispherical return date differences, which range between 0-30 years across the CCM projections analysed, are affected by both the sensitivity of ozone to Cly (ozone trends have a larger effect on return dates when sensitivity is lower) and the difference in ozone trends between hemispheres. An attribution analysis performed with two CCMs shows that chemically-induced changes in ozone are the major driver of the earlier return of ozone to 1980 levels in northern mid-latitudes. The causes for chemically-induced asymmetric ozone trends relevant for the total column ozone return date differences are found to be (i) stronger increases in ozone production due to enhanced NOx concentrations in the Northern Hemisphere lowermost stratosphere and troposphere, (ii) stronger decreases in the destruction rates of ozone by the NOx cycle in the Northern Hemisphere lower stratosphere linked to effects of dynamics and temperature on NOx concentrations, and (iii) an increasing efficiency of heterogeneous ozone destruction by Cly in the Southern Hemisphere mid-latitudes as a result of decreasing lower stratospheric temperatures. The full abstract can be found here.