Abstract

Abstract. Ozone is an important greenhouse gas in terms of anthropogenic radiative forcing (RF). RF calculations for ozone were until recently entirely model based, and significant discrepancies were reported due to different model characteristics. However, new instantaneous radiative kernels (IRKs) calculated from hyperspectral thermal IR satellites have been able to help adjudicate between different climate model RF calculations. IRKs are defined as the sensitivity of the outgoing longwave radiation (OLR) flux with respect to the ozone vertical distribution in the full 9.6 μm band. Previous methods applied to measurements from the Tropospheric Emission Spectrometer (TES) on Aura rely on an anisotropy approximation for the angular integration. In this paper, we present a more accurate but more computationally expensive method to calculate these kernels. The method of direct integration is based on similar principles to the anisotropy approximation, but it deals more precisely with the integration of the Jacobians. We describe both methods and highlight their differences with respect to the IRKs and the ozone longwave radiative effect (LWRE), i.e., the radiative impact in OLR due to absorption by ozone, for both tropospheric and total columns, from measurements of the Infrared Atmospheric Sounding Interferometer (IASI) onboard MetOp-A. Biases between the two methods vary from −25 to +20 % for the LWRE, depending on the viewing angle. These biases point to the inadequacy of the anisotropy method, especially at nadir, suggesting that the TES-derived LWREs are biased low by around 25 % and that chemistry–climate model OLR biases with respect to TES are underestimated. In this paper we also exploit the sampling performance of IASI to obtain first daily global distributions of the LWRE, for 12 days (the 15th of each month) in 2011, calculated with the direct integration method. We show that the temporal variation of global and latitudinal averages of the LWRE shows patterns which are controlled by changes in the surface temperature and ozone variation due to specific processes, such as the ozone hole in the polar regions and stratospheric intrusions into the troposphere.

Highlights

  • Ozone in the atmosphere is a key substance for both atmospheric chemistry and climate

  • We calculated the longwave radiative effect of ozone due to absorption. These calculations were performed using two different methods: the anisotropy approximation, which is a simplified approach with a moderate requirement of computational resources, and the direct integration method, which follows more strictly the application of the instantaneous radiative kernels (IRKs) definition but demands more computational resources

  • A step-by-step comparison between the two methods was conducted for both the IRKs and the longwave radiative effect (LWRE), using global daily data from the Infrared Atmospheric Sounding Interferometer (IASI) instrument on the MetOp-A satellite

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Summary

Introduction

Ozone in the atmosphere is a key substance for both atmospheric chemistry and climate. In 2011, Worden et al (2011) used the measurements of Aura-TES (Tropospheric Emission Spectrometer) to calculate the longwave radiative effect (LWRE) due to ozone with respect to TOA radiative flux. This radiative effect is different from the radiative forcing defined in IPCC (Ramaswamy et al, 2001), as it is not calculated at the tropopause and does not refer to ozone concentration changes with respect to pre-industrial levels. Note that all zenith angles are converted to equivalent TOA nadir angles for IASI and will be used as such hereafter

IASI-FORLI radiance Jacobians
Angular integration of moments
Anisotropy approximation
Direct integration of Jacobians
IRK comparison
LWRE comparison
LWRE annual variation
15 Jan 15 Feb
Findings
Conclusions
Full Text
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