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Long open path Fourier Transform Spectroscopy measurements of atmospheric greenhouse gases David Griffith University of Wollongong, Australia & Sam Hammer, Sanam Vardag, Ingeborg Levin Denis Pöhler, Stefan Schmitt, Ulrich Platt, University of Heidelberg, Germany 2 nd ICOS Science Conference Helsinki, Sept 2016

Long open path Fourier Transform Spectroscopy measurements … · 2019. 8. 19. · Spectroscopy measurements of atmospheric greenhouse gases David Griffith University of Wollongong,

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  • Long open path Fourier Transform Spectroscopy measurements of atmospheric greenhouse gases

    David Griffith University of Wollongong, Australia

    & Sam Hammer, Sanam Vardag, Ingeborg Levin

    Denis Pöhler, Stefan Schmitt, Ulrich Platt, University of Heidelberg, Germany

    2nd ICOS Science Conference Helsinki, Sept 2016

  • History 1: open path FTIR in the mid IR Measuring greenhouse gases from agriculture

    Tracer release (N2O) FTIR beam

    wind

    FTIR

    Retroreflector

    FTIR & telescope

  • OP-FTIR-tracer: results

    Tracer

    CHTracerCH C

    CFF 4

    4=

  • History 2: TCCON, GOSAT and OCO-2: Near IR remote sensing of CO2, CH4, N2O, CO, H2O

    Long path absorption spectroscopy in the near IR Sun as source, ~8-40 km absorption path TCCON precision/accuracy for CO2 0.1 – 0.2% (0.4 – 0.8 ppm)

    TCCON FTIR

    Satellite SCIA, GOSAT, OCO-2

  • Open path FTIR meets DOAS in the NIR

    The most accurate greenhouse gas measurements are point-based Open path spectroscopy has some advantages

    Spatial averaging Better match to regional-scale model resolution How spatially representative are point measurements? How accurate are open path measurements?

    TCCON provides precise measurements of GHGs Solar NIR absorption spectroscopy, 8-20 km-atm atmospheric path,

    high spectral resolution Precision/accuracy 0.1 – 0.2% (0.4 – 0.8 ppm for CO2)

    How well can we measure GHGs at the ground in an open path? Low resolution portable FTS Weaker source than the sun (50W quartz lamp) 2-6 km path

  • Long path FTS setup

    FT detector

    interferogram source spectrum

    FT Interferometer 0.5 cm-1 resoln Bruker IRcube

    1.5 km

    Illuminating bundle Receiving fibre

    φ 30 cm

    FL 150 cm

    17 x 70mm retroreflectors

  • IUP

    Retrorefl.

    Heidelberg Commercial centre

  • FTIR-DOAS setup

  • NIR long path spectrum 3.1 km return path IUP - Philosophen Weg

    Weak CO2 Strong CO2

    2 1.6 Microns 1.25 2.5

    CH4

    O2

    1.4

    H2O H2O

  • “Strong” CO2 band 4900-5000 cm-1

    CO2

    H2O

    CO2

  • CH4 is weaker…

    CH4

  • O2

    O2

  • Quantitative spectrum analysis Least squares calculated fit: example CO2

  • Temperatures point vs path averaged

  • O2 – reality check

    Stray sunlight

    0.21

  • Water vapour and δD

    2.0

    1.5

    1.0H2O

    / %

    21-Jul-14 10-Aug-14 30-Aug-14 19-Sep-14 09-Oct-14 29-Oct-14

    -200

    -100

    0 δD / ‰

    30

    20

    10

    0

    Air t

    emp

    / °C

    H2O - open path H2O - met station delD Temperature

  • CO2 July-October 2014

  • CO2 – 3 days in July

    Germany wins World Cup!

  • CO2 open path – point in situ differences

    “1σ” = 7ppm (n=21,800) Slight skew from SE (city)

    in situ > open path

    -40

    -20

    0

    20

    40

    CO

    2 di

    ffere

    nce

    / ppm

    108642

    Wind Speed / m s-1

    -50

    -25

    0

    +25

    +50

    -25 0 +25 +50

    0

    45

    90

    135

    180

    225

    270

    315

  • CH4 July-October 2014

  • CH4 open path – point in situ differences

    “1σ” = 93 ppb (n=21,800)

    -300

    -200

    -100

    0

    +100

    +200

    +300

    -200 -100 0 +100+200+300

    0

    45

    90

    135

    180

    225

    270

    315

    -400

    -200

    0

    200

    400

    CH

    4 diff

    eren

    ce /

    ppm

    86420

    Wind speed / m s-1

  • Precision and accuracy - summary

    Repeatability limited by signal noise optical throughput

    Accuracy/bias limited by HITRAN/MALT ~ 2-4% Temperature ~ 3°C (1%) Pressure

  • An interesting artefact …

    18:15 every sunny day!

  • Solar beam travels through ~17 km path - Apparent increase in CO2, CH4, O2

  • Potential improvements & future work

    More light! Precision is detector noise limited

    Brighter source larger telescope/retro reflector area

    Pre-modulate IR source before transmission Removes stray (sun)light artefacts

    Remove or co-fit fibre spectral structures Higher resolution?

    Better discrimination against interferences, but… Lower SNR => lower precision Less portable

  • Thank you !

    Long open path Fourier Transform Spectroscopy measurements of atmospheric greenhouse gases�History 1: open path FTIR in the mid IR�Measuring greenhouse gases from agricultureOP-FTIR-tracer: resultsHistory 2: TCCON, GOSAT and OCO-2: �Near IR remote sensing of CO2, CH4, N2O, CO, H2OOpen path FTIR meets DOAS in the NIRLong path FTS setupSlide Number 7Slide Number 8FTIR-DOAS setupNIR long path spectrum�3.1 km return path IUP - Philosophen Weg“Strong” CO2 band 4900-5000 cm-1CH4 is weaker…O2Quantitative spectrum analysis�Least squares calculated fit: example CO2Temperatures�point vs path averagedO2 – reality checkWater vapour and dDCO2 July-October 2014CO2 – 3 days in July�CO2�open path – point in situ differencesCH4 �July-October 2014CH4�open path – point in situ differencesPrecision and accuracy - summaryAn interesting artefact …Slide Number 25Potential improvements & future workSlide Number 27Slide Number 28