Physically Based Thermal Infrared Snow/Ice Surface Emissivity for Fast Radiative Transfer Models

Author:

Nalli Nicholas R.12ORCID,Dang Cheng34,Jung James A.5,Knuteson Robert O.6ORCID,Borbas E. Eva6,Johnson Benjamin T.347,Pryor Ken8ORCID,Zhou Lihang9ORCID

Affiliation:

1. IMSG, Inc., NOAA/NESDIS Center for Satellite Applications and Research (STAR), College Park, MD 20740, USA

2. National Geospatial-Intelligence Agency (NGA), Springfield, VA 22150, USA

3. University Corporation for Atmospheric Research (UCAR), Boulder, CO 80301, USA

4. Joint Center for Satellite Data Assimilation (JCSDA), Boulder, CO 20740, USA

5. Cooperative Institute for Meteorological Satellite Studies (CIMSS), University of Wisconsin-Madison, Madison, WI 53706, USA

6. Space Science and Engineering Center, University of Wisconsin-Madison, Madison, WI 53706, USA

7. NOAA/NWS National Centers for Environmental Prediction (NCEP), College Park, MD 20740, USA

8. NOAA/NESDIS/STAR, College Park, MD 20740, USA

9. NOAA JPSS Program Office, Lanham, MD 20706, USA

Abstract

Accurate thermal infrared (TIR) fast-forward models are critical for weather forecasting via numerical weather prediction (NWP) satellite radiance assimilation and operational environmental data record (EDR) retrieval algorithms. The thermodynamic and compositional data about the surface and lower troposphere are derived from semi-transparent TIR window bands (i.e., surface-sensitive channels) that can span into the far-infrared (FIR) region under dry polar conditions. To model the satellite observed radiance within these bands, an accurate a priori emissivity is necessary for the surface in question, usually provided in the form of a physical or empirical model. To address the needs of hyperspectral TIR satellite radiance assimilation, this paper discusses the research, development, and preliminary validation of a physically based snow/ice emissivity model designed for practical implementation within operational fast-forward models such as the U.S. National Oceanic and Atmospheric Administration (NOAA) Community Radiative Transfer Model (CRTM). To accommodate the range of snow grain sizes, a hybrid modeling approach is adopted, combining a layer scattering model based on the Mie theory (viz., the Wiscombe–Warren 1980 snow albedo model, its complete derivation provided in the Appendices) with a specular facet model. The Mie-scattering model is valid for the smallest snow grain sizes typical of fresh snow and frost, whereas the specular facet model is better suited for the larger sizes and welded snow surfaces typical of aged snow. Comparisons of the model against the previously published spectral emissivity measurements show reasonable agreement across zenith observing angles and snow grain sizes, and preliminary observing system experiments (OSEs) have revealed notable improvements in snow/ice surface window channel calculations versus hyperspectral TIR satellite observations within the NOAA NWP radiance assimilation system.

Funder

NOAA Joint Polar Satellite System (JPSS-STAR) Product System’s Development and Implementation (PSDI), Proving Ground and Risk Reduction

Cal/Val Programs

NOAA/NESDIS/STAR Satellite Meteorology and Climatology Division

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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