1 Clear-Sky irradiance observations and models to analyze aerosol characteristic over Semi-arid Reno, NV. By: Addison Liming Jayne Boehmler Marcela Loria-Salazar.

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Presentation transcript:

1 Clear-Sky irradiance observations and models to analyze aerosol characteristic over Semi-arid Reno, NV. By: Addison Liming Jayne Boehmler Marcela Loria-Salazar (Jammin group) :-D Clear-Sky irradiance observations and models to analyze aerosol characteristic over Semi-arid Reno, NV. By: Addison Liming Jayne Boehmler Marcela Loria-Salazar (Jammin group) :-D

2 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

3 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

4 Use of the sun-photometer to analyze aerosol characteristic in Reno. Under clear-sky conditions on April 10 th 2014 at 16:30 (PST) Compare SMARTS model against the observations taken from the sun-photometer. Models used: Urban Desert Min Desert MaxPurpose

5 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

Aerosol It is a suspension of fine solid particles or liquid droplets in a gas. Anthropogenic: Causes by human activities Natural: Causes by the nature 6

7 Aerosol modal distribution

8 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

9 April 10 th 2014, 16:30 (PST)

Instruments 10 AOD(500 nm)=0.1 PW =5mm Ocean Optics: Red tide 350 nm nm

11 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

Model Parameter: Asymmetry parameter Asymmetry parameter ~ 1 Forward scattering ~ -1 Back scattering It is a measure of the preferred scattering direction 12

Ratio between of light scattering ( β sca ) and light extinction ( β sca + β abs ) Ratio between of light scattering ( β sca ) and light extinction ( β sca + β abs ) SSA>0.9 SSA~0.3 Model Parameter: Single Scattering Albedo (SSA) SSA1 Total scattering 0 Total absorption 13

14 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

SMARTS: Urban Model 15

SMARTS: Desert Max Model 16

SMARTS: Desert Min Model 17

Irradiance measurements from the spectrometer April 10 th

Ratio of diffuse and direct radiation On April 10 th

Ratio of diffuse and direct radiation On April 10 th

Irradiance measurements from the spectrometer April 10 th

Ratio of diffuse and direct radiation SMARTS and Spectrometer 22

Ratio of diffuse and direct radiation SMARTS and Spectrometer 23

Irradiance measurements from the spectrometer April 10 th

Ratio of diffuse and direct radiation SMARTS and Spectrometer 25

Ratio of diffuse and direct radiation SMARTS and Spectrometer 26

27 OutlineOutline PurposeAerosol propertiesMethodsModel parametersResultsSummary

28Summary Model fits with the reality of April 10 th 2014 at 16:30 (PST) under clear – sky conditions over semi-arid Reno NV. Model: The noisy ratio from the UV-IR spectrometer is due to the fact that the light is completely filtered at the visible range. The inverse is true for the visible filtered spectrometer. Observations :

29Summary The ratio of diffuse to direct radiation in Reno fits between the models for urban and desert minimum at longer wavelength. UV-IR channel responds at shorter wavelength and follows the Desert Max and Urban models. Coarse mode respond to short wavelength range. Having two spectrometers is necessary to fully understand the aerosol content in the atmosphere especially in desert conditions where the effect of natural desert aerosols is not fully understood. Model and Observations:

30Questions