Cross-validation of HIRDLS and COSMIC radio-occultation retrievals, particularly in relation to fine vertical structure

INFRARED SPACEBORNE REMOTE SENSING AND INSTRUMENTATION XVI SPIE-INT SOC OPTICAL ENGINEERING 7082 (2008)

Authors:

JJ Barnett, CL Hepplewhite, S Osprey, JC Gille, R Khosravi

Abstract:

The High Resolution Dynamics Limb Sounder (HIRDLS) instrument was launched oil the NASA Aura satellite in July 2004. HIRDLS is a joint project between the UK and USA, and is a mid-infrared limb emission sounder designed to measure the concentrations of trace species, Cloud and aerosol, and temperature and pressure variations in the Earth’s atmosphere front the upper troposphere to the mesophere. The instrument is intended to make measurements at both high vertical and horizontal spatial resolutions, but validating those measurements is difficult because few other measurements provide that vertical resolution sufficiently closely in time. However, the FOPMOSAT-3/COSMIC suite of radio occultation satellites that exploit the U.S. GPS transmitters to obtain high resolution (similar to 1 km) temperature profiles in the stratosphere does provide sufficient profiles nearly coincident with those from HIRDLS. Comparisons show a good degree intercorrelation between COSMIC and HIRDLS down to about 2 km resolution, with similar amplitudes for each, implying that HIRDLS and COSMIC are able to measure the same small scale features. The optical blockage that occurred within HIRDLS during launch does not seem to have affected this capability.

Axisymmetric, nearly inviscid circulations in non‐condensing radiative‐convective atmospheres

Quarterly Journal of the Royal Meteorological Society Wiley 134:634 (2008) 1269-1285

Authors:

Rodrigo Caballero, Raymond T Pierrehumbert, Jonathan L Mitchell

Coupled chemistry climate model simulations of the solar cycle in ozone and temperature

Journal of Geophysical Research Atmospheres 113:11 (2008)

Authors:

J Austin, K Tourpali, E Rozanov, H Akiyoshi, S Bekki, G Bodeker, C Brühl, N Butchart, M Chipperfield, M Deushi, VI Fomichev, MA Giorgetta, L Gray, K Kodera, F Lott, E Manzini, D Marsh, K Matthes, T Nagashima, K Shibata, RS Stolarski, H Struthers, W Tian

Abstract:

The 11-year solar cycles in ozone and temperature are examined using new simulations of coupled chemistry climate models. The results show a secondary maximum in stratospheric tropical ozone, in agreement with satellite observations and in contrast with most previously published simulations. The mean model response varies by up to about 2.5% in ozone and 0.8 K in temperature during a typical solar cycle, at the lower end of the observed ranges of peak responses. Neither the upper atmospheric effects of energetic particles nor the presence of the quasi biennial oscillation is necessary to simulate the lower stratospheric response in the observed low latitude ozone concentration. Comparisons are also made between model simulations and observed total column ozone. As in previous studies, the model simulations agree well with observations. For those models which cover the full temporal range 1960-2005, the ozone solar signal below 50 hPa changes substantially from the first two solar cycles to the last two solar cycles. Further investigation suggests that this difference is due to an aliasing between the sea surface temperatures and the solar cycle during the first part of the period. The relationship between these results and the overall structure in the tropical solar ozone response is discussed. Further understanding of solar processes requires improvement in the observations of the vertically varying and column integrated ozone. Copyright 2008 by the American Geophysical Union.

Decadal-scale changes in the effect of the QBO on the northern stratospheric polar vortex

Journal of Geophysical Research Atmospheres 113:10 (2008)

Authors:

H Lu, MP Baldwin, LJ Gray, MJ Jarvis

Abstract:

This study documents decadal-scale changes in the Holton and Tan (HT) relationship, i.e., the influence of the lower stratospheric equatorial quasi-biennial oscillation (QBO) on the northern hemisphere (NH) extratropical. circulation. Using a combination of ECMWF ERA-40 Reanalysis and Operational data from 1958-2006, we find that the Arctic stratosphere is indeed warmer under easterly QBO and colder under westerly QBO. During November to January, composite easterly minus westerly QBO signals in zonal wind extend from the lower stratosphere to the upper stratosphere and are centered at ∼5 hPa, 55-65°N with a magnitude of ∼10 m s-1. In temperature, the maximum signal is near ∼20-30 hPa at the pole with a magnitude of ∼4 K. During winter, the dominant feature is a poleward and downward transfer of wind and temperature anomalies from the midlatitude upper stratosphere to the high latitude lower stratosphere. For the first time, a statistically significant decadal scale change of the HT relationship during 1977-1997 is diagnosed. The main feature of the change is that the extratropical QBO signals reverse sign in late winter, resulting in fewer and delayed major stratospheric sudden warmings (SSWs), which occurred more often under westerly QBO. Consistent with earlier studies, it is found that the HT relationship is significantly stronger under solar minima overall, but the solar cycle does not appear to be the primary cause for the detected decadal-scale change. Possible mechanisms related to changes in planetary wave forcing are discussed. Copyright 2008 by the American Geophysical Union.

Data discrepancies in solar-climate link.

Science American Association for the Advancement of Science (AAAS) 320:5877 (2008) 746