Long-Term Halogen Measurements at Cape Verde

Similar documents
ACTRIS TNA Activity Report

Long term DOAS measurements at Kiruna

Arctic Oxidation Chemistry

Daytime OIO in the Gulf of Maine

Halogens in the Troposphere

Multi axis differential optical absorption spectroscopy (MAX-DOAS)

CU Airborne Multi AXis DOAS

Remote Measurement of Tropospheric NO 2 by a Dual MAX-DOAS over Guangzhou During the 2008 PRD Campaign

Reactive iodine species in a semi-polluted environment

Trace gases, aerosols & clouds analysed from GOME, SCIAMACHY and GOME-2. Recommendations for TROPOMI. Thomas Wagner. Satellite Group Mainz Heidelberg

Remote Sensing of Atmospheric Trace Gases Udo Frieß Institute of Environmental Physics University of Heidelberg, Germany

Arctic Halogen Chemistry Part II

RETRIEVAL OF STRATOSPHERIC TRACE GASES FROM SCIAMACHY LIMB MEASUREMENTS

Algorithm Document HEIDOSCILI

Atmospheric Measurements from Space

Atmospheric Gas Phase Reactions. U. Platt

ClO + O -> Cl + O 2 Net: O 3 + O -> O 2 + O 2

Lecture 15 Antarctic Ozone Hole ATOC/CHEM 5151

Monitoring of trace gas emissions from space: tropospheric abundances of BrO, NO 2, H 2 CO, SO 2, H 2 O, O 2, and O 4 as measured by GOME

CREATE Summer School. Tim Canty

Autonomous "OBuoy" observations of the Arctic atmosphere

Supplement of Iodine oxide in the global marine boundary layer

MODEL SIMULATION OF BrO CHEMISTRY AT THE DEAD SEA, ISRAEL

Halogen Chemistry in CAM-CHEM & CCMVal

Reactive halogens and their measurements in the troposphere

CONTENTS 1 MEASURES OF ATMOSPHERIC COMPOSITION

DOAS: Yesterday, Today, and Tomorrow

Reactive and organic halogen species in three different European coastal environments

Atmospheric Chemistry III

BrO PROFILING FROM GROUND-BASED DOAS OBSERVATIONS: NEW TOOL FOR THE ENVISAT/SCIAMACHY VALIDATION

BIRA-IASB, Brussels, Belgium: (2) KNMI, De Bilt, Netherlands.

Tropospheric bromine in GEOS- Chem: Impact on preindustrial and present-day ozone

Dynamics and chemistry of tropospheric bromine explosion events in the Antarctic coastal region

Measurements of Ozone. Why is Ozone Important?

PROBLEMS Sources of CO Sources of tropospheric ozone

2. Sketch a plot of R vs. z. Comment on the shape. Explain physically why R(z) has a maximum in the atmospheric column.

What are Aerosols? Suspension of very small solid particles or liquid droplets Radii typically in the range of 10nm to

MAX-DOAS observations of NO 2 in NDACC: status and perspectives

7.5-year global trends in GOME cloud cover and humidity - a signal of climate change? Institut für Umweltphysik, Uni-Heidelberg, Germany

Chemistry 471/671. Atmospheric Chemistry III: Stratospheric Ozone Depletion

Chapman. 4. O + O 3 2 O 2 ; k 4 5. NO + O 3 NO 2 + O 2 ; k 5 6. NO 2 + O NO + O 2 ; k 6 7. NO 2 + hν NO + O; k 7. NO X Catalytic.

SCIAMACHY book. Ozone variability and long-term changes Michel Van Roozendael, BIRA-IASB

On the vertical distribution of boundary layer halogens over coastal Antarctica: implications for O 3, HO x, NO x and the Hg lifetime

MAX-DOAS air quality observations at Phimai,

Recent Climate History - The Instrumental Era.

A one dimensional model study of the mechanism of halogen liberation and vertical transport in the polar troposphere

Spatially resolved measurements of nitrogen dioxide in an urban environment using concurrent multi-axis differential optical absorption spectroscopy

Long Path (active) DOAS

From the measurement of halogenated species to iodine particle formation

Scattered-light DOAS Measurements

Retrieval and Monitoring of atmospheric trace gas concentrations in nadir and limb geometry using the space-borne SCIAMACHY instrument

Chemical sources and sinks of Hg(II) in the remote atmospheric marine boundary layer

Car MAX-DOAS measurements around entire cities: quantification of NO x emissions from the cities of Mannheim and Ludwigshafen (Germany)

Longtime Satelite Observation of Atmospheric Trace Gases

Longtime Satelite Observation of Atmospheric Trace Gases

Progress of total ozone data retrieval from Phaeton - REG(AUTH)

8.2 Tropospheric ozone

UV-Vis Nadir Retrievals

Tananyag fejlesztés idegen nyelven

CAM-Chem Chemical Forecasts

MAX-DOAS observations of NO 2 in NDACC: status and perspectives

Tropospheric NO 2 column densities deduced from zenith-sky DOAS measurements in Shanghai, China, and their application to satellite validation

Emission Limb sounders (MIPAS)

WATER VAPOUR RETRIEVAL FROM GOME DATA INCLUDING CLOUDY SCENES

Algorithms/Results (SO 2 and ash) based on SCIAMACHY and GOME-2 measurements

UKCA_RADAER Aerosol-radiation interactions

MAX-DOAS measurements of atmospheric trace gases in Ny-Ålesund - Radiative transfer studies and their application

Inaugural University of Michigan Science Olympiad Tournament

Aircraft Observations of the Lower Atmosphere and Surface Exchange Processes. Jennifer Murphy Department of Chemistry, University of Toronto

Stratosphere and Ozone

Stratospheric O 3 : Overview

Sensitivity of Ozone to Bromine in the Lower Stratosphere

Physical and Optical Properties of the Stratospheric Aerosol Layer

Ozone: Earth s shield from UV radiation

Aerosols and climate. Rob Wood, Atmospheric Sciences

MEASURING TRACE GAS PROFILES FROM SPACE

BrO measurements over the Eastern North-Atlantic

Chapter 4 Nadir looking UV measurement. Part-I: Theory and algorithm

Observations of high concentrations of I 2 and IO in coastal air supporting iodine-oxide driven coastal new particle formation

Differential Optical Absorption Spectroscopy (DOAS)

Aerosols AP sizes AP types Sources Sinks Amount and lifetime Aerosol radiative effects. Aerosols. Trude Storelvmo Aerosols 1 / 21

Comparison of Results Between the Miniature FASat-Bravo Ozone Mapping Detector (OMAD) and NASA s Total Ozone Mapping Spectrometer (TOMS)

CHEM/ENVS 380 S14, Midterm Exam ANSWERS 1 Apr 2014

Retrieval of stratospheric and tropospheric BrO columns from multi-axis DOAS measurements at Reunion Island (21 S, 56 E)

Spectral surface albedo derived from GOME-2/Metop measurements

Relation of atmospheric humidity and cloud properties to surface-near temperatures derived from GOME satellite observations

The Structure and Motion of the Atmosphere OCEA 101

Stratospheric Chemistry: Polar Ozone Depletion AOSC 433/633 & CHEM 433/633. Ross Salawitch

Review of Lectures 9 to 16 AOSC 433/633 & CHEM 433. Ross Salawitch

Overview on UV-Vis satellite work

UV-visible observations of atmospheric O 4 absorptions using direct moonlight and zenith-scattered sunlight for clear-sky and cloudy sky conditions

The Atmosphere. All of it. In one hour. Mikael Witte 10/27/2010

Introduction to HadGEM2-ES. Crown copyright Met Office

Earth s Heat Budget. What causes the seasons? Seasons

On the importance of aqueous-phase chemistry on the oxidative capacity of the troposphere: A 3-dimensional global modeling study

Aerosol. Challenge: Global Warming. Observed warming during 20 th century, Tapio. 1910s. 1950s. 1990s T [Kelvin]

Supplement of Cloud and aerosol classification for 2.5 years of MAX-DOAS observations in Wuxi (China) and comparison to independent data sets

Chapter 3. Multiple Choice Questions

ATOC 3500/CHEM 3151 Week 9, 2016 The Game Changer. Some perspective The British Antarctic Survey The Ozone Hole International Regulations

What is a Sudden Stratospheric Warming?

Transcription:

Long-Term Halogen Measurements at Cape Verde Ulrich Platt, Udo Frieß, Jessica Balbo Institut for Environmental Physics, University of Heidelberg, Germany Reactive Halogen Species in the Troposphere Previous Work of IUP Heidelberg DOAS and MAX-DOAS Expectations and Plans University of Heidelberg Institute for Environmental Physics

Reactive Halogens in the Atmosphere Stratosphere: Known since Lovelock, Global Strat. Ozone Depletion, Ozone Hole,... Sources: Longe lived organo-halogens Stratospheric Ozone destruction I Cl + O 3 ClO + O 2 ClO + O Cl + O 2 II Cl + O 3 ClO + O 2 Br + O 3 BrO + O 2 ClO + BrO Cl + Br + O 2 III ClO + ClO Cl 2 O 2 Cl 2 O 2 + hν Cl 2 + O 2 Troposphere: Known only since late 1980ies,... Sources: Short lived organohalogens, Sea salt, Volcanoes,... Consequences Ozone destruction, Reduction of Ozone formation, Modification of oxidation capacity Br (ng m -3 ), O 3 (ppbv) 100 80 60 40 20 O3 Br Barrie et al. 1988 0 0 5 10 15 20 April 1986

Simplified Outline of the Tropospheric XO X -Cycles XO X = X + XO Primary Emission (Algae, etc.) CH 3 X CHX 3 CH 2 X 2 etc. OH, hν X = I, Br, Cl HX RH,HO 2 OH XNO 2 X YO hν O 3, NO 2 XO NO 2 hν, hν YO hν hν HO 2 hν, HOX OXO XY, X 2 [ ] [ X] XO 1000 X = Cl, ( ) ( ) ( ) 100 X= Br, 10 X= I XONO 2 X 2 O 2 N 2 O 5 HX XONO 2 X 2 O 2 HOX Y - H + + X - Sea-Salt (Snow Pack or Aerosol)

Halogen Catalysed Destruction of Tropospheric O 3 Homogeneous reactions 1) XO + XO X + X + O 2 (rate determining) X 2 + O 2 X 2 + hν X + X 2 (X + O 3 XO + O 2 ) net: 2 O 3 3 O 2 2) XO + YO X + Y + O 2 (rate determining) XY + O 2 XY + hν X + Y ( Y + OXO + O 2 ) 2 nd order in RHS X + O 3 XO + O 2 Y + O 3 YO + O 2 net: 2 O 3 3 O 2 3) XO + HO 2 HOX + O 2 (rate determining) HOX + hν X + OH OH + AO HO 2 + A (AO = O 3, CO,...) net: 2 O 3 3 O 2 1 st order in RHS

Impediment of NO X and HO X Catalysed Tropospheric Ozone Production by Halogen Oxides XO + HO 2 HOX+O 2 HOX + hν OH + X XO XO + NO NO 2 + X X + O 3 XO + O 2 The product: [HO 2 ]x[no] and thus the rate of O 3 formation is reduced XO

Tropospheric Halogen Domains From: v. Glasow & Platt, HitT Description

IO Precursor: CH 2 I 2 or I 2? Data from Mace Head 1998, and Brittany, France, 2003 CH 2 I 2 [ppt] Date 1998 13.9 14.9 15.9 16.9 17.9 80 0.2 60 40 0.1 photopic [klx] IO concentration [ppt] 2 Jun 3 Jun 4 Jun 5 Jun 6 Jun 7 Jun 10 6 8 6 4 4 2 2 0 0-2 Tidenhöhe [m] TH [m] 20 0.0 0 13.9 14.9 15.9 16.9 17.9 6 4-2 -4 2 Jun 3 Jun 4 Jun 5 Jun 6 Jun 7 Jun Date IO at Lilia, Brittany, France, Atlantic Coast 06.5.2003-13.6.2003, C. Peters et al. 2005 2 0 CH 2 I 2 by Lucy Carpenter, taken from Kai Hebestreit Ph. D. Thesis, Univ. of Heidelberg, 2001

DOAS Measurements of I 2 at Mace Head, Oct. 1998 Data from Hönninger et al., re-evaluation by C. Peters Molecular Iodine is only seen at very low tide Forest of Laminaria Digitata

I 2, IO, OIO, and BrO during NAMBLEX at Mace Head, 2002 Saiz-Lopez et al., ACP 6, 2006 BrO at August 3, 4, 10 of 2002

Summary: Consequences of RHS in the Troposphere Catalytic destruction of ozone Reduction of the HO 2 /OH ratio XO Enhancement of the NO 2 /NO ratio Potentially strong influence on the global tropospheric ozone budget XO Change of oxidation capacity (e.g. reduction of DMS) Primary particle formation (IO X ) Particle formation: [Hoffmann et al. 2001, Jimenez et al. 2003, Burkholder et al. 2004]: Precursor (org. or I 2 ) + hν I + I + O 3 IO + O 2 IO + IO OIO + I OIO + OIO I 2 O 4 + O 2 I 2 O 4 + OIO particle

Preceding Work of our Laboratory Related to RHS in General Our Group has been involved in Investiations of most experimental aspects of tropospheric RHS including: Studies in polar regions (first identification of BrO in the Arctic and Antarctic Boundary Layers) Studies at Salt Lakes (first identification of BrO and IO at the Dead Sea and at the Salar de Uyuni) Studies in the free troposphere (first direct determination of BrO in the free troposphere by ballon-based spectroscopy) Studies at volcanoes (first identification of BrO, ClO, and OClO in volcanic plumes) Studies in coastal regions (first identification of IO in a coastal region (Mace Head, Ireland)) Satellite Studies (first measurement of polar trop. BrO from satellite) Identification of the Bromine Explosion Mechanism in polar regions. University of Heidelberg Institute for Environmental Physics

Intensität Intensity ( ) [cm 2 ] Differential Optical Absorption Spectroscopy (DOAS) The Idea a b I 0 D' ' b [nm] I' 0 Use differences of intensities at different wavelengths Record the intensity in many (typ. several 100) wavelength channels (entire spectra) High pass-filtering of spectra remove continuum Fit reference spectra Make use of all spectral information Cross Sections [arb.units] BrO IO I 2 OIO Cabo Verde Spectrometer: BrO, IO, NO 2, CH 2 O 300 350 400 450 500 550 600 wavelength [nm]

ϑ = 80 Stratospheric Layer MAX-DOAS The Idea ϑ AMF= SCD VCD ϑ = 30 Stratosphere: Signal determined by Solar Zenith Angleϑ AMF strat = AMF(ϑ) Boundary Layer: Signal determined by Observation Elevation Angle α AMF BL = AMF (α ) Boundary Layer O Observer Mean free path (355nm)=8-10km α Total Slant Column: S = S Trop 1 + S sinα Strat 1 = V cosϑ a 1 sin + α 1 cosϑ ( 1 a) Hönninger, v. Friedeburg, and Platt, Atmos. Chem. Phys. 4, 231 254, 2004

The Mini MAX-DOAS Instrument Cabo Verde Spectrometer: BrO, IO, NO 2, CH 2 O Copper Block Thermal Insulation Peltier Element Cooling Fins Miniature Spectrometer (Ocean Optics USB 2000) Telescop e Optical Fiber (also scrambles polarisation) Lens PC-Board (Electronics)

MAX - DOAS on the Atlantic (Polarstern, 2000) Time of day, October 1 Englisch Channel Time of day, October 12 Mid Atlantic Leser et al., GRL 2003 doi:10.1029/2002gl015811

Radiation Transport Considerations for MAX-DOAS Measurements Zenith direct sunlight Radiation scattered into the spectrometer's field of view Weighting Function α Shallow trace gas layer: Strong increase of trace gas column density with decreasing observation elevation angle Deep trace gas layer: Little increase of trace gas column density with decreasing observation elevation angle Spectrometer Spectrometer Spectrometer

Vertical Resolution of MAX-DOAS --> Poor Man s LIDAR SCD s Measured on May 4, 2000 (15:15 UT 15:40 UT), Alert 2000 PSE α -1 [deg -1 ] 0.0 0.1 0.2 0.3 0.4 0.5 SCD BrO [10 14 cm -2 ] 2.5 2.0 1.5 1.0 0.5 measured modelled P1 (0-1km) P2 (0-2km) P3 (0-1km+1-2km) P4 (1-2km) P5 (O 4 ) P6 (strat.) 2.5 2.0 1.5 1.0 0.5 0.0 0.0 90 20 10 5 elevation angle α [ ] Hönninger and Platt, Atmos. Environ. 36, 2481, 2002 2

Also Measure Species with Known Abundance, e.g. O 4 Aerosol Optical Density and Layer Height from O 4 Sinreich et al., Faraday Discuss. 130, 153-164, DOI: 10.1039/B419274P, 2005 Intensity

dscd 1.50E+015 1.20E+015 9.00E+014 6.00E+014 3.00E+014 BrO at Cape Verde, Oct. 28-31, 2006-2 2 5 10 20 70 0 3.000 6.000 12.00 60.00 0.00E+000-3.00E+014 28/10/2006 29/10/2006 30/10/2006 31/10/2006 01/11/2006 1.20E+015 BrO 28.10.06 Date 1.00E+015 8.00E+014 Spectral Range: 330-450 nm NO 2, BrO, IO (CH 2 O) dscd 6.00E+014 4.00E+014 2.00E+014 0.00E+000-2.00E+014 00:00 04:48 09:36 14:24 19:12 24:00 Time

dscd 1.00E+017 8.00E+016 6.00E+016 4.00E+016 NO 2 at Cape Verde, Oct. 28-31, 2006 0-2 2 3.000 5 6.000 10 12.00 20 69.00 70 2.00E+016 0.00E+000 1.00E+017 28.10.06 28/10/2006 29/10/2006 30/10/2006 Date 31/10/2006 01/11/2006 8.00E+016 6.00E+016 dscd 4.00E+016 2.00E+016 0.00E+000 07:12 09:36 12:00 14:24 16:48 19:12 Time

Questions, Hopes, and Plans... Scientific Questions: What is the liberation mechanisms of reactive halogen species from aerosol (and sea water?)? What is the role of Biogenic Sources and the transformation of organo-halogen species? What is the role of dust on halogen cycling? What is the extend of particle formation from halogen (iodine) precursors? What are the possible consequences global change on halogen and other chemistry? What are the consequences of tropospheric halogen chemistry on the oxidation capacity of the atmosphere and its impact on climate? Observations, e.g. BrO, IO dust correlations BrO, IO correlations with organohalogen levels BrO, IO correlations with biological activity in the ocean Future Better spectrometer (include I 2, OIO) Dedicated aerosol spectrometer...