sparc volcano meeting zurich 8-9th july 2009 participants:

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SPARC Volcano Meeting Zurich 8-9th July 2009 Participants: Debra Weisenstein, Larry Thomason, Gera Stenchikov, Rene Hommel, Claudia Timmreck, Stephan Fueglistaler, Mike Mills, Stefan Brönnimann, Florian Arfeuille, Tom Peter, Eugene Rozanov, Beiping Luo, Patricia Heckendorn-Kenzelmann, Hans Graf, Ulrike Niemeier, Terry Deshler, Mahesh Mundakkara Kovilakam, Ana Cirisan, Perrine Lemennais, Julien Jumelet

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SPARC Volcano Meeting Zurich 8-9th July 2009 Participants: Debra Weisenstein, Larry Thomason, Gera Stenchikov, Rene Hommel, Claudia Timmreck, Stephan Fueglistaler, Mike Mills, Stefan Brönnimann, Florian Arfeuille, Tom Peter, Eugene Rozanov, Beiping Luo, - PowerPoint PPT Presentation

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Page 1: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

SPARC Volcano Meeting Zurich 8-9th July 2009

Participants:

Debra Weisenstein, Larry Thomason, Gera Stenchikov, Rene Hommel,Claudia Timmreck, Stephan Fueglistaler, Mike Mills, Stefan Brönnimann, Florian Arfeuille, Tom Peter, Eugene Rozanov, Beiping Luo,Patricia Heckendorn-Kenzelmann, Hans Graf, Ulrike Niemeier,Terry Deshler, Mahesh Mundakkara Kovilakam, Ana Cirisan, Perrine Lemennais, Julien Jumelet

Page 2: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

Program

Introduction Welcome Tom Peter Uncertainties in modeling volcanic eruptions Patricia Heckendorn

Part I: Observation of Mt. Pinatubo eruption in 1991

Issues related to developing a global long-term Larry Thomason stratospheric aerosol climate data set

Retrieval of size distribution from SAGE Beiping Luo extinction data

Injection height and efficiency Hans Graf

Comparison of stratospheric aerosol surface Mahesh Kovilakam densities from SAGE II and OPC measurements

Optical particle counter measurements Terry Deshler of stratospheric aerosols

Discussion Part I

Page 3: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

Program cont

Part II: Modeling of stratospheric aerosols formed after volcanic eruptions

Sensitivity studies with sulphur model AER Debra Weisenstein of Mt. Pinatubo eruption

The aerosol cloud of large volcanic eruptions: Ulrike Niemeier Simulations with MAECHAM5/HAM

Sulfate aerosol studies with WACCM/CARMA Mike Mills

Stratospheric aerosol modeling: Rene Hommel Scenarios in 3-D and 1-D

Discussion Part II

Page 4: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

Program cont

Part III: Modeling historic/paleo volcanic eruptions

Understanding the climate impact of past Claudia Timmreck volcanic eruptions: "Simulations, Observations, Challenges”

Modeling past volcanism: Florian Arfeuille The Mt Tambora 1815 eruption case study.

Observation-based data and model simulations Stefan Brönnimann of climate effects of major eruptions during the past 125 years”

Discussion Part III

Part IV: Radiative, chemical and dynamical response to volcanic eruptions

Coupled climate model simulations of the Gera Stenchikov Pinatubo and Tambora Impacts.

Mt. Pinatubo eruption modeled by CCM SOCOL Eugene Rozanov

Volcanoes and their impact on atmospheric Claudia Timmreck chemistry and dynamics

Page 5: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

Program cont

Do we understand stratospheric temperatures Stephan Fueglistaler in the Pinatubo period?

Are the models ready for the volcanic forcing? Hans Graf

Effect of geoengineering aerosols on cirrus Ana Cirisan

Discussion Part IV & Final Discussion

Friday 10th July 2009

Splinter Meetings SAGE-OPC intercomparison in volcanically quiescent periodsGeoengineering applications

Page 6: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:
Page 7: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

1980 1990 2000

3

2

1

0

-1

-2

Ano

mal

y (K

)

Sorted according to magnitude of anomalySOCOL calculated on line using aerosol data from ASAPCMAM calculated on line with climate model radiation schemeE39C precalculated net heating rates Kirchner et al. (1999)UMETRAC precalculated heating rates (Stenchikov, pers. communication, 2005)MAECHAM4C precalculated net heating rates Kirchner et al. (1999)MRI calc. on line from OD and reff based on data by Sato et al. (1993)ERA40 observations, global annual mean, 50 hPaULAQ calculated on line Pitari (1993)AMTRAC calculated on line with climate model radiation schemeCCSRNIES calculated on line using aerosol data from Sato et al. (1993)

T, global annual mean, 50 hPa

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Page 10: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

nominal OPC uncertainty

uncertainty SAGE extinction

uncertainty SAGE SAD assuming n = 20 cm-3

unlimited SAGE uncertainty w/o additional assumption

From the ASAP-Report (Assessment of Stratospheric Aerosol Properties)

Page 11: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

Very last slide:

Low clouds, cirrus and volcanic aerosol above northern midlatitudes, Sept 2009

Zurich, 16 September 2009

Page 12: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:

Highlight:New Instrument development

COBALD LightweightBackscatter Sonde

Feature Specification Remark

wavelengths 455 nm & 870 nm color index 1-15

Backscatter 104 from unperturbed dynamic range stratosph. aerosol to

thick anvil outflow

time resolution 1 s 0.05-3 s selectable

dimensions 17 × 14 × 12 cm3 incl. 3 cm insulation

total weight 540 g suited for piggyback

power supply 8 × LR61 (1.5V AA) for > 3 h of operation

2 × 6LR61 (9V)

data interface 19.2 kbit/s, settings for SRS-C34,logic level RS232 adaptable to telemetry

altitude range ground to > 30 km cp. weather sondes

More on this: Cirisan et al., future work

Page 13: SPARC Volcano Meeting Zurich 8-9th July 2009  Participants:
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Part I: Observation of Mt. Pinatubo eruption in 1991

1.1. How much S emitted by Mt. Pinatubo eruption? 4 – 9 – 13 MT S Vertical distribution of the initial SO2

cloud?

1.2. What is the vertical distribution of aerosol after gas to particle conversion?

1.3. How good are the extinction measurements of the different instruments?

1.4. Which is the best method to retrieve the aerosol size distribution from extinction measurements?

Part II: Modeling of stratospheric aerosols formed after volcanic eruptions

2.1. How good is the performance of different aerosol models?

2.2. Which micro-physical processes are most important for the formation of aerosols after Mt. Pinatubo eruptions?

2.3. Which process dominates at what altitude? To what degree does the answer depend on the type and strength of the volcanic eruption? What does the answer mean of geoengineering applications in comparison to eruptions? Again, what does this mean especially for the tropical tropopause? 2.3. How important is the correct vertical, horizontal and temporal distribution of the aerosol cloud? (HG/MH, DW, CT, KK, LT, MS, PH, ER) In the SPARC stratospheric aerosol report (Thomason and Peter , 2006) the Pinatubo simulation with AER aerosol model injected SO2 in a broad layer (16-29 km altitude, 5°S-14°N). Results from volcanic plume model studies emphasize the importance of the vertical distribution of the sulphur cloud, which is evidently not homogeneous (Herzog & Graf). Would the results of the plume model serving as initial condition for AER 2D model actually lead to an improvement of the aerosol modeling. Part III: Modeling historic/paleo volcanic eruptions 3.1. What information do we have on volcanic eruptions of the last millennium? What are the uncertainties in ice cores volcanic aerosols estimates? (FA, SB, KK/MT, GS) 3.2. How could we model the aerosol distribution of historic eruptions with only a few constraints? (GS, CT, KK/MT, HG/MH, SB/FA) What do we know about spatial and temporal injections of sulphur to the stratosphere? What is the most credible column height for Tambora (Sigurdsson and Carey, 1989: 43km)? What could have been the SO2 vertical distribution of the Tambora cloud? Incidences of the height on aerosol formation. 3.3. For past eruptions as that of Tambora, could a volcanic plume model provide realistic source parameters for the AER 2D model? (HG/MH, DW) 3.4. Did the injection of halogens by past volcanic eruptions have a significant impact on stratospheric ozone and climate? (HG/MH, FA, SB, KK, MT) What are the main mechanisms regulating the percentages of HCl and HBr reaching the stratosphere? The literature ranges from more than 25% reaching the stratosphere (Textor et al 2003) to almost nothing (Tabazadeh&Turco 1993). Would a drastic perturbation of the ozone layer after the Tambora eruption have been documented in terms of significantly increased skin diseases? 3.5. What do we know about aerosol size distributions of very large eruptions? (HG/MH, DW, BL) Is there an upper bound on the mode radius of the aerosol distribution after large volcanic eruptions, as particles with larger radius than such an upper bound are lost due to gravitational settling and washout in the troposphere? Part IV: Radiative, chemical and dynamical response to volcanic eruptions Many CCMs overestimate the lower stratospheric heating after Mt. Pinatubo eruption. If the optical properties are correct (this question should be answered by Sections 1 and 2), there must be a problem either in the radiative transfer code, the cloud scheme or the dynamical response of the model. 4.1. How reliable are the radiative transfer codes of different models? (PH, GS, ER, BL, KK, CT/UN) The heating rates modelled in the lower tropical stratosphere after volcanic eruptions calculated by ECHAM4 and ECHAM5 differ significantly from the ones calculated by Libradtran (pseudospectral model) (Kenzelmann, 2009). Is Libradtran a good reference model? Are there other, better reference models? 4.2. Is there any evidence that the tropical tropopause was heated after volcanic eruptions? (SF, KK) Many modeling studies show a warming of the tropical tropopause. This would presumably lead to a moistening of the stratosphere. Some studies suggest a moistening of the stratosphere (e.g. Oltmans et al., 2000; Joshi and Shine, 2003) some don’t (e.g. ERA interim Randel et al., 2004). 4.3. Which chemical processes lead to the depletion of the ozone layer after volcanic eruptions? (MT, CT, KK, ER, TP, PH) The NOx/NOy and the ClOx/Cly fraction are changed after volcanic eruption with elevated halogen concentrations. Which reactions are responsible for that? Mainly N2O5 hydrolysis or also heterogenous Cl activation? 4.4. How is the stratospheric circulation influenced by volcanic eruptions? (HG/MH/RH, SF, CT/UN, KK, MG, PH, SB)

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