Interannual Variability of Solar Reflectance From Data and Model

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Interannual Variability of Solar Reflectance From Data and Model Z. Jin, C. Lukachin, B. Wielicki, and D. Young SSAI, Inc. / NASA Langley research Center April 10-13, 2012

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Interannual Variability of Solar Reflectance From Data and Model. Z. Jin, C. Lukachin , B. Wielicki , and D. Young SSAI, Inc. / NASA Langley research Center April 10-13, 2012. Objectives: Understand the interannual variability expected in the CLARREO solar benchmark spectra. - PowerPoint PPT Presentation

Transcript of Interannual Variability of Solar Reflectance From Data and Model

Page 1: Interannual  Variability of Solar Reflectance From Data and Model

Interannual Variability of Solar Reflectance From Data and Model

Z. Jin, C. Lukachin, B. Wielicki, and D. Young

SSAI, Inc. / NASA Langley research CenterApril 10-13, 2012

Page 2: Interannual  Variability of Solar Reflectance From Data and Model

Objectives:1) Understand the interannual variability expected in the CLARREO solar

benchmark spectra.2) Evaluate the modeling ability to simulate the spectral solar reflectance

and its variability.

Data: SCIAMACHY radiance and solar irradiance (2003-2010).Spectral range: 300-1750 nm; resolution: 1 nm.

Model: MODTRAN with input parameters from CERES SSF, MODIS and SMOBA.

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NP (60N-90N)

NML (30N-60N)

TRO (30S-30N)

SML (30S-60S)

SP (60S-90S)

Five latitude regions

Data are first averaged to 10 deg latitude zones in each month. Reflectance is averaged over 5 large latitude regions and globe.

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A sample of SCIAM measured solar irradiance over 7 years (2004-2010).(Each colored line is for a different year)

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An example of SCIAM measured solar

reflectance averaged to the 5 latitude

regions and globe.

(Each panel is for a different region,

each color is for a different year.)

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An example to show the interannual and seasonal variability of the monthly mean solar reflectance from SCIAM data.

Line thickness =

2σ of reflectance

across all years

LandOcean

Averaged reflectance over 2004-2010 from SCIAM.

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An example of model-observation comparison of reflectance over the

SML ocean.(Each panel is for a different

month)

SCIAM measuredModeled with mean cloud τ

Reflectance diff.

Mean SZA (deg)

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The probability distribution function (PDF) of cloud τ from CERES MODIS in three 10 degree zones (20N-10S) in April months spanning 2000-2005, separated by cloud phase and by ocean and land.

The cloud τ PDF is used in the RT modeling to account the large cloud variation from footprint to footprint.

Example of cloud PDF

τ

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A model-observation comparison over global ocean.

SCIAM measuredModeled with mean cloud τModeled with τ PDF

Use mean tauUse tau PDF

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The largest improvement is in the tropic.

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SCIAM measuredModeled with mean cloud τModeled with τ PDF

Use mean tauUse tau PDF

The least improvement is in the polar regions.

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An example of monthly mean reflectance anomaly from SCIAM and model. (Anomaly is defined as the reflectance difference from the average of the same months across all years).

Dotted: SCIAMSolid: Model

One panel for one region, one color for one year.

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Comparison of the global monthly mean reflectance anomalies between SCIAM measurements and model.

Dotted: SCIAMSolid: Model

One panel for one month, one color for one year.

Spectral ranges with large measurement uncertainty.

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Comparison of the model-observation reflectance anomalies over the tropic region.

Dotted: SCIAMSolid: Model

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Ocean Land

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1σ of the monthly mean global reflectance across all years from SCIAM and model.

One panel for one month.

Spectral ranges with large measurement uncertainty.

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The monthly mean reflectance σ from SCIAM and model.

Each panel shows a different region.

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The annual mean reflectance σ from SCIAM and model.

Each panel shows a different region.

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Summary1) Measurement data have shown large seasonal and regional variations in

the solar benchmark spectra, but their interannual variability is much smaller (within ±0.005 for monthly global mean).

2) When simple mean cloud τ is used, the modeled monthly mean solar reflectance over large climate regions could be biased from observation by 5-20% in magnitude, depending on season and region. When the cloud τ PDF is adopted, the bias can be reduced significantly.

3) Modeled solar reflectance spectrum and its variability are consistent with observations, for example, both show an interannual variability (1σ) of 1-2% for monthly global mean reflectance and <1% for global annual mean.

4) IF the PCRTM (X Liu) is fast enough, it will be used for footprint by footprint computation with CERES SSF for further comparison with SCIAM.

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Acknowledgement:

We thank the CERES team and DAAC at NASA Langley for the CERES SSF data, Sciamachy science team for the spectral solar radiance/irradiance data, and Dr. Sky Yang and Dr. Shuntai Zhou for the SMOBA data.