Auswirkungen von Halogen-induzierten stratosphärischen Ozonänderungen auf den effektiven Strahlungsantrieb und das Oberflächenklima

2021 ◽  
Author(s):  
Katerina Kusakova ◽  
Björn-Martin Sinnhuber ◽  
Peter Braesicke

<p>   Emissionen von anthropogenen FCKW wurden infolge des Montrealer Abkommens von 1987 stark reduziert und entsprechend wird für das 21. Jahrhundert eine Erholung der Ozonschicht erwartet. Eine Änderung der Ozonkonzentration in der Stratosphäre verändert die Energiebilanz der Erde und wird, im Vergleich zum heutigen Tag, zu einem positiven Strahlungsantrieb führen. Daraus resultieren sowohl global als auch regional erwärmende oder abkühlende Einflüsse auf das Klima.</p> <p>    Der effektive Strahlungsantrieb (Effective radiative forcing - ERF) ist definiert als Änderung der Strahlungsflüsse am oberen Rand der Atmosphäre durch bestimmte „Treiber“, unter Berücksichtigung von Rückkopplungen des Klimasystems auf kurzen Zeitskalen, während Rückkopplungen auf langen Zeitskalen (insbesondere die Meeresoberflächentemperaturen) konstant gehalten werden.Einige Studien untersuchten bereits das ERF von troposphärischen Ozonäderungen, nur wenig ist aber bekannt über den Einfluss von stratosphärischem Ozonänderungen auf den effektiven Strahlungsantrieb und dessen Auswirkung auf das Oberflächenklima.</p> <p>    Um die Entwicklung der Ozonschicht und damit einhergehende Klimaänderung in die Zukunft zu projizieren führten wir so genannte Time-Slice Simulationen mit dem Klimamodell ICON-ART durch. Stratosphärische Ozonänderungen wurden mit dem linearisierten Ozonschema (LINOZ) berechnet, mit einem zusätzlichen Verlustterm, um die katalytische Ozonzerstörung in Polarregionen zu berücksichtigen. Das modellierte Ozon war interaktiv und mit der Strahlung gekoppelt.</p> <p>   In der Standardsimulation werden Meeresoberflächentemperatur und Meer-Eisbedeckung, Aerosole und Treibhausgase entsprechend für das Jahr 2000 fixiert. Für Sensitivitätssimulationen verwenden wir den gleichen Modellaufbau wie in der Standardsimulation, aber mit stratosphärischen Halogenkonzentrationen entsprechend dem 1960 Niveau. Unsere Ergebnisse zeigen, dass die Ozonabnahme zwischen den Jahren 1960 und 2000 zwar global zu keinem signifikantem ERF geführt hat. Regional, auf der Südhemisphäre, vor allem über der Antarktis, ist das ERF der Ozonabnahme aber durchaus signifikant. Unsere Ergebnisse zeigen, dass in hohen südlichen Breiten über der Antarktis das negative ERF durch die Ozonabnahme zwischen 1960 und 2000 zu einem wesentlichen Teil das positive ERF durch den CO2 Anstieg kompensiert hat.</p> <p> </p>

2020 ◽  
Author(s):  
Timothy Andrews ◽  
Christopher J Smith ◽  
Gunnar Myhre ◽  
Piers Forster ◽  
Robin Chadwick ◽  
...  

2016 ◽  
Vol 9 (8) ◽  
pp. 3477-3490 ◽  
Author(s):  
Nir Bluvshtein ◽  
J. Michel Flores ◽  
Lior Segev ◽  
Yinon Rudich

Abstract. Atmospheric aerosols play an important part in the Earth's energy budget by scattering and absorbing incoming solar and outgoing terrestrial radiation. To quantify the effective radiative forcing due to aerosol–radiation interactions, researchers must obtain a detailed understanding of the spectrally dependent intensive and extensive optical properties of different aerosol types. Our new approach retrieves the optical coefficients and the single-scattering albedo of the total aerosol population over 300 to 650 nm wavelength, using extinction measurements from a broadband cavity-enhanced spectrometer at 315 to 345 nm and 390 to 420 nm, extinction and absorption measurements at 404 nm from a photoacoustic cell coupled to a cavity ring-down spectrometer, and scattering measurements from a three-wavelength integrating nephelometer. By combining these measurements with aerosol size distribution data, we retrieved the time- and wavelength-dependent effective complex refractive index of the aerosols. Retrieval simulations and laboratory measurements of brown carbon proxies showed low absolute errors and good agreement with expected and reported values. Finally, we implemented this new broadband method to achieve continuous spectral- and time-dependent monitoring of ambient aerosol population, including, for the first time, extinction measurements using cavity-enhanced spectrometry in the 315 to 345 nm UV range, in which significant light absorption may occur.


2018 ◽  
Vol 10 (11) ◽  
pp. 2786-2805 ◽  
Author(s):  
J. P. Mulcahy ◽  
C. Jones ◽  
A. Sellar ◽  
B. Johnson ◽  
I. A. Boutle ◽  
...  

2018 ◽  
Author(s):  
Benjamin S. Grandey ◽  
Daniel Rothenberg ◽  
Alexander Avramov ◽  
Qinjian Jin ◽  
Hsiang-He Lee ◽  
...  

Abstract. We quantify the effective radiative forcing (ERF) of anthropogenic aerosols modelled by the aerosol–climate model CAM5.3-MARC-ARG. CAM5.3-MARC-ARG is a new configuration of the Community Atmosphere Model version 5.3 (CAM5.3) in which the default aerosol module has been replaced by the two-Moment, Multi-Modal, Mixing-state-resolving Aerosol model for Research of Climate (MARC). CAM5.3-MARC-ARG uses the default ARG aerosol activation scheme, consistent with the default configuration of CAM5.3. We compute differences between simulations using year-1850 aerosol emissions and simulations using year-2000 aerosol emissions in order to assess the radiative effects of anthropogenic aerosols. We compare the aerosol column burdens, cloud properties, and radiative effects produced by CAM5.3-MARC-ARG with those produced by the default configuration of CAM5.3, which uses the modal aerosol module with three log-normal modes (MAM3). Compared with MAM3, we find that MARC produces stronger cooling via the direct radiative effect, stronger cooling via the surface albedo radiative effect, and stronger warming via the cloud longwave radiative effect. The global mean cloud shortwave radiative effect is similar between MARC and MAM3, although the regional distributions differ. Overall, MARC produces a global mean net ERF of −1.75 ± 0.04 W m−2, which is stronger than the global mean net ERF of −1.57 ± 0.04 W m−2 produced by MAM3. The regional distribution of ERF also differs between MARC and MAM3, largely due to differences in the regional distribution of the cloud shortwave radiative effect. We conclude that the specific representation of aerosols in global climate models, including aerosol mixing state, has important implications for climate modelling.


2020 ◽  
Vol 20 (10) ◽  
pp. 6225-6241 ◽  
Author(s):  
Alyson Douglas ◽  
Tristan L'Ecuyer

Abstract. Aerosol–cloud interactions and their resultant forcing remains one of the largest sources of uncertainty in future climate scenarios. The effective radiative forcing due to aerosol–cloud interactions (ERFaci) is a combination of two different effects, namely how aerosols modify cloud brightness (RFaci, intrinsic) and how cloud extent reacts to aerosol (cloud adjustments CA; extrinsic). Using satellite observations of warm clouds from the NASA A-Train constellation from 2007 to 2010 along with MERRA-2 Reanalysis and aerosol from the SPRINTARS model, we evaluate the ERFaci in warm, marine clouds and its components, the RFaciwarm and CAwarm, while accounting for the liquid water path and local environment. We estimate the ERFaciwarm to be -0.32±0.16 Wm−2. The RFaciwarm dominates the ERFaciwarm contributing 80 % (-0.21±0.15 Wm−2), while the CAwarm enhances this cooling by 20 % (-0.05±0.03 Wm−2). Both the RFaciwarm and CAwarm vary in magnitude and sign regionally and can lead to opposite, negating effects under certain environmental conditions. Without considering the two terms separately and without constraining cloud–environment interactions, weak regional ERFaciwarm signals may be erroneously attributed to a damped susceptibility to aerosol.


2017 ◽  
Author(s):  
Yawen Liu ◽  
Kai Zhang ◽  
Yun Qian ◽  
Yuhang Wang ◽  
Yufei Zou ◽  
...  

Abstract. Aerosols from fire emissions can potentially have large impact on clouds and radiation. However, fire aerosol sources are often intermittent and their effect on weather and climate is difficult to quantify. Here we investigated the short-term effective radiative forcing of fire aerosols using the global aerosol-climate model Community Atmosphere Model Version 5 (CAM5). Different from previous studies, we used nudged hindcast ensembles to quantify the forcing uncertainty due to the chaotic response to small perturbations in the atmosphere state. Daily mean emissions from three fire inventories were used to consider the uncertainty in emission strength and injection heights. The simulated aerosol optical depth (AOD) and mass concentrations were evaluated against in-situ measurements and re-analysis data. Overall, the results show the model has reasonably good predicting skills. Short (10-day) nudged ensemble simulations were then performed with and without fire emissions to estimate the effective radiative forcing. Results show fire aerosols have large effects on both liquid and ice clouds over the two selected regions in April 2009. For the 10-day average, we found a large ensemble spread of regional mean shortwave cloud radiative effect over Southern Mexico (15.6 %) and the Central U.S. (64.3 %), despite that the regional mean AOD time series are almost indistinguishable during the 10-day period. Moreover, the ensemble spread is much larger when using daily averages instead of 10-day averages. For the case investigated here, a minimum of 9 ensemble members is necessary to get a reasonable estimate of the ensemble mean and spread of the forcing on individual days. This demonstrates the importance of using a large ensemble of simulations to estimate the short-term effective aerosol radiative forcing.


2020 ◽  
Author(s):  
Takuro Michibata ◽  
Kentaroh Suzuki ◽  
Toshihiko Takemura

Abstract. Complex aerosol–cloud–precipitation interactions lead to large differences in estimates of aerosol impacts on climate among general circulation models (GCMs) and satellite retrievals. Typically, precipitating hydrometeors are treated diagnostically in most GCMs, and their radiative effects are ignored. Here, we quantify how the treatment of precipitation influences the simulated effective radiative forcing due to aerosol–cloud interactions (ERFaci) using a state-of-the-art GCM with a two-moment prognostic precipitation scheme that incorporates the radiative effect of precipitating particles, and investigate how microphysical process representations are related to macroscopic climate effects. Prognostic precipitation substantially weakens the magnitude of ERFaci (by approximately 75 %) compared with the traditional diagnostic scheme, and this is the result of the increased longwave (warming) and weakened shortwave (cooling) components of ERFaci. The former is attributed to additional adjustment processes induced by falling snow, and the latter stems largely from riming of snow by collection of cloud droplets. The significant reduction in ERFaci does not occur without prognostic snow, which contributes mainly by buffering the cloud response to aerosol perturbations through depleting cloud water via collection. Prognostic precipitation also alters the regional pattern of ERFaci, particularly over northern mid-latitudes where snow is abundant. The treatment of precipitation is thus a highly influential controlling factor of ERFaci, contributing more than other uncertain tunable processes related to aerosol–cloud–precipitation interactions. This change in ERFaci caused by the treatment of precipitation is large enough to explain the existing difference in ERFaci between GCMs and observations.


2018 ◽  
Vol 18 (2) ◽  
pp. 621-634 ◽  
Author(s):  
Camilla W. Stjern ◽  
Helene Muri ◽  
Lars Ahlm ◽  
Olivier Boucher ◽  
Jason N. S. Cole ◽  
...  

Abstract. Here we show results from Earth system model simulations from the marine cloud brightening experiment G4cdnc of the Geoengineering Model Intercomparison Project (GeoMIP). The nine contributing models prescribe a 50 % increase in the cloud droplet number concentration (CDNC) of low clouds over the global oceans in an experiment dubbed G4cdnc, with the purpose of counteracting the radiative forcing due to anthropogenic greenhouse gases under the RCP4.5 scenario. The model ensemble median effective radiative forcing (ERF) amounts to −1.9 W m−2, with a substantial inter-model spread of −0.6 to −2.5 W m−2. The large spread is partly related to the considerable differences in clouds and their representation between the models, with an underestimation of low clouds in several of the models. All models predict a statistically significant temperature decrease with a median of (for years 2020–2069) −0.96 [−0.17 to −1.21] K relative to the RCP4.5 scenario, with particularly strong cooling over low-latitude continents. Globally averaged there is a weak but significant precipitation decrease of −2.35 [−0.57 to −2.96] % due to a colder climate, but at low latitudes there is a 1.19 % increase over land. This increase is part of a circulation change where a strong negative top-of-atmosphere (TOA) shortwave forcing over subtropical oceans, caused by increased albedo associated with the increasing CDNC, is compensated for by rising motion and positive TOA longwave signals over adjacent land regions.


2016 ◽  
Vol 48 (11-12) ◽  
pp. 3489-3505 ◽  
Author(s):  
Timothy Andrews ◽  
Richard A. Betts ◽  
Ben B. B. Booth ◽  
Chris D. Jones ◽  
Gareth S. Jones

Author(s):  
Donald P. Cummins ◽  
David B. Stephenson ◽  
Peter A. Stott

Abstract. Reliable estimates of historical effective radiative forcing (ERF) are important for understanding the causes of past climate change and for constraining predictions of future warming. This study proposes a new linear-filtering method for estimating historical radiative forcing from time series of global mean surface temperature (GMST), using energy-balance models (EBMs) fitted to GMST from CO2-quadrupling general circulation model (GCM) experiments. We show that the response of any k-box EBM can be represented as an ARMA(k, k−1) (autoregressive moving-average) filter. We show how, by inverting an EBM's ARMA filter representation, time series of surface temperature may be converted into radiative forcing. The method is illustrated using three-box EBM fits to two recent Earth system models from CMIP5 and CMIP6 (Coupled Model Intercomparison Project). A comparison with published results obtained using the established ERF_trans method, a purely GCM-based approach, shows that our new method gives an ERF time series that closely matches the GCM-based series (correlation of 0.83). Time series of estimated historical ERF are obtained by applying the method to a dataset of historical temperature observations. The results show that there is clear evidence of a significant increase over the historical period with an estimated forcing in 2018 of 1.45±0.504 W m−2 when derived using the two Earth system models. This method could be used in the future to attribute past climate changes to anthropogenic and natural factors and to help constrain estimates of climate sensitivity.


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