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Ice-Phase Precipitation Remote Sensing Using Combined Passive and Active Microwave Observations

Ice-Phase Precipitation Remote Sensing Using Combined Passive and Active Microwave Observations. Benjamin T. Johnson UMBC/JCET & NASA/GSFC (Code 613.1) Benjamin.T.Johnson@nasa.gov. Gail Skofronick -Jackson NASA/GSFC (Code 613.1 ). IGARSS 2011 – Vancouver, Canada.

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Ice-Phase Precipitation Remote Sensing Using Combined Passive and Active Microwave Observations

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  1. Ice-Phase Precipitation Remote Sensing Using Combined Passive and Active Microwave Observations Benjamin T. Johnson UMBC/JCET & NASA/GSFC (Code 613.1) Benjamin.T.Johnson@nasa.gov Gail Skofronick-Jackson NASA/GSFC (Code 613.1) IGARSS 2011 – Vancouver, Canada

  2. Figure 1.: whiteout conditions during a snow storm. 2/22

  3. Introduction • Midlatitude/Winter precipitation is difficult to measure using radars or radiometers alone. • Precipitating clouds consist of a wide range of particles with variable shape, size, number density, and composition, and microwave radiation is sensitive to these properties • Furthermore, ice clouds, water clouds, and gases and attenuate/emit microwave radiation B. Johnson IGARSS 2011 3/22

  4. Physically-based microwave precipitation remote sensing methods require (at least): • A physical description of the atmosphere and surface properties • Physical descriptions of hydrometeors (PSD, shape(s), composition) • Appropriate relationships between physical and scattering/extinction/backscattering properties • An inversion method for retrieving the desired physical properties given observations B. Johnson IGARSS 2011 4/22

  5. Relevant Key Problems • Uncertainties the physical description of the atmosphere: distribution of CLW, WV; particle composition, size distribution, and shape. • No current method for validating MW scattering properties of ice-phase hydrometeors. • Present Retrieval Approach • Physical method using “consistency matching” -- adjust simulations until consistent with PMW and radar observations across multiple wavelengths (e.g., Meneghini, 1997). • Pros: Simple to implement, works equally over land and water • Cons: “matches” may not represent reality, geometric issues ignored (NUBF, beam matching) • Important note: the uncertainty due to unknown particle shape is orders of magnitude greater than other known sources of uncertainties. B. Johnson IGARSS 2011 5/22

  6. Retrieval Schematic (1) Radar-only Retrieval Large set of Radar-Retrieved Vertical Profiles of PSD/IWC Observed Reflectivities (Zku, Zka) Attenuation “Correction” Inversion Z-S, DWR, etc. (2) Forward Model Physical - Radiative Database Physical Model Precip. & Atmos. Hydrometeor Model Ext., Scat., p(Q), Z Radiative Transfer Model (3) Radar/Radiometer Retrieval Simulated Radiances (TBsim) TB Constrained PSD/IWC Profiles PMW Retrieval Algorithm Observed Radiances (TBobs) 6/22

  7. Observed Reflectivities and Passive Microwave TBs during the 2003 Wakasa Bay Experiment B. Johnson IGARSS 2011 7/22

  8. (Const. Density Spheres) Retrieval Inputs at each vertical level Environment: Pressure, Temperature, Humidity, Cloud Water Content Microphysics: Particle Density, Shape, PSD Type Observables: Zm,14, Zm,35, DWR Forward Dual Wavelength Ratio Retrieval Method Update PIA for air, clouds, and precip. (A14, A35) Starting at storm top (ztop) down to z=0 PIA-corrected Reflectivities Ze,14, Ze,35 B. Johnson IGARSS 2011 8/22 Match DWR with D0 (3.67/L) in Database; compute N0 Is DWR  1? no yes Ze,35-IWC retrieval, infer D0 / N0

  9. WBAY 03: Dual Wavelength Ratio, and retrieved N0, and D0 (assuming a single constant particle density) B. Johnson IGARSS 2011 9/22

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  13. Part 1 comments: • The basic retrieval works surprisingly well using only constant-density spheres • approx. 5 K RMS error in precipitating regions, simply by adjusting the CLW and particle density. • However, constant-density spheres likely are not representative of the true distribution of mass and sizes of particles within the observed volume of the atmosphere… • Improvements: • Inclusion of well-known size-density relationships for spheres (following Brown and Ruf, 2007), • Include sets of non-spherical “realistically shaped” hydrometeors B. Johnson IGARSS 2011 13/22

  14. (Fixed IWC = 1.0 g m-3) Constant Density Spheres Mass-Density Relationships Magono and Nakamura (1965) Mitchell et al. (1990) Locatelli and Hobbs (1974) Barthazy (1998) UW-NMS (Tripoli, 1992) 14/22

  15. Retrieved log10(IWC) [g m-3] using size-density relationships (Brown and Ruf, 2007) 15/22

  16. B. Johnson IGARSS 2011 16/22

  17. Retrieved IWC [g m-3] :: “Realistic” particle shapes, exponential PSD B. Johnson IGARSS 2011 17/22

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  20. Final comments: • The present method is designed for testing advances in the physical-radiative properties of a physically based retrieval algorithm • The choice of particle shape and size distribution appears to be the largest uncertainty in physically-based precipitation retrieval algorithms (most certainly renders them ill-posed) • So, prior knowledge of the particle shapes and sizes should significantly constrain physically based retrievals • However, this requires that one has already computed the necessary physical-radiative properties ahead of time! B. Johnson IGARSS 2011 20/22

  21. Next Steps for this work: • (un-break my radiative transfer model… ) • Create complete database of IWC as a function of reflectivity, dual-wavelength ratio, and particle shape. • Add other non-spherical shapes (in progress, e.g., Kuo, G. Liu, others) • Add melting particles (in progress) • Apply retrieval to GPM satellite simulator data (T. Matsui, WK Tao, et al.) as a alg. dev. testbed. • Incorporate database(s) into official GPM combined radar/radiometer algorithm • currently assumes constant-density spheres(?) B. Johnson IGARSS 2011 21/22

  22. B. Johnson IGARSS 2011 22/22

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