NASA NTRS · 20190030824
The WRF Lightning Forecasting Algorithm: Sensitivities to Microphysics and Boundary Layer Physics Schemes
Abstract
As with WRF model simulated convection in general, LFA output is sensitive to cloud and PBL physics. WRF convection is also sensitive to model initialization uncertainties and unresolved errors. Large sensitivity exists in HRRR-like Thompson microphysics and PBL, for which original LFA calibration constant needs to be multiplied by 1.13 to give proper FRD amplitudes. Thompson microphysics scheme also shows poorest correlations relative to reference data, suggesting low predictability of HRRR LFA output. Need to validate HRRR LFA against GLM observations.
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McCaul, Eugene W., Jr., Priftis, Georgios, Case, Jonathan L., Chronis, Themis, Gatlin, Patrick N., Goodman, Steven J., Kong, Fanyou. 2019-09-07. The WRF Lightning Forecasting Algorithm: Sensitivities to Microphysics and Boundary Layer Physics Schemes. https://ntrs.nasa.gov/citations/20190030824
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