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/** | ||
\page HWRF_famp HWRF Ferrier-Aligo (FA) Microphysics Scheme | ||
\section des_famp Description | ||
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The Ferrier-Aligo (FA) microphysics (Aligo et al. 2018 \cite aligo_et_al_2018) is a single | ||
moment scheme predicting mass mixing ratios of rain water (\f$q_r\f$), cloud water (\f$q_c\f$), | ||
cloud ice (\f$q_i\f$), and snow-graupel (\f$q_s\f$). The FA scheme is currently used operationally | ||
in the North American Mesoscale Forecast System (NAM; including the parent 12-km domain, the 3-km | ||
NAM nests, and the 1.5km fire weather nest), the Hurricane Weather Research and Forecasting Model (HWRF), | ||
the Hurricanes in a Multi-scale Ocean-coupled Non-hydrostatic Model (HMON), and the High-Resolution | ||
Window (HiResW) Non-dydrostatic Multiscale Model on the B grid (NMMB). The FA scheme advects each | ||
species separately in the NAM nests, and advects the total condensate in the 12-km parent NAM,HiResW NMMB, | ||
HWRF, and HMON. | ||
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Unique to the FA scheme is the calculation of a diagnostic array called the "rime factor" (RF), which | ||
represents the degree of riming onto snow-graupel, and takes into account the temperature of the ice particle, | ||
the impact velocity of the cloud droplet on the ice particle, and the size of the cloud droplet. For all | ||
practical purposes, one can categorize precipitation ice as snow, graupel, or hail, similar to the ice | ||
species predicted in other microphysical schemes based on the value of the RF. For example, an RF = 1 | ||
represents unrimed snow; lightly rimed snow occurs when 1 < RF < 2; heavily rimed snow when 2< RF \f$\leqslant\f$ 5; | ||
graupel when 5 < RF < 10; and frozen drops or hail when RF \f$geqslant\f$ 10. In reality, the RF knows | ||
no arbitrary cutoff between different ice categories, and the categorizations above are somewhat subjective. | ||
Figure 1 is a schematic illustration of the FA scheme processes and each process is described in Table 1. | ||
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\image html FA_MP_schematic.png "Figure 1: Local Land-atmosphere Interaction (courtesy of Michael Ek)" width=10cm | ||
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Owing to operational computation constraints, and unique to the FA scheme, the sedimentation process | ||
does not use finite differencing of precipitation fluxes in the vertical in order to circumvent the | ||
requirement that small time steps be used in order to maintain numerical stability, particularly since | ||
the vertical resolution often increases dramatically near the ground. The algorithm is instead based upon | ||
a partitioning of precipitation already present in the grid box at the beginning of the time step and the | ||
precipitation entering the grid box from above at the end of the time step. A more detailed description | ||
of the sedimentation algorithm can be found in Aligo et al. (2018, appendix D). | ||
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An algorithm was developed in FA to improve stratiform rainfall by allowing the rain intercept parameter, | ||
\f$N_{or}\f$, to vary with height and the mean drop diameter to be fixed below melting layers. This is | ||
different from other single-moment microphysics schemes (WSM6 and Lin) that assume a constant value for | ||
\f$N_{or}\f$. The algorithm in the FA scheme, simular to what is done in the Thompson scheme \cite thompson_et_al_2008, | ||
assumes that a snow-graupel particle about to enter the melting layer from above has the same mean mass | ||
as a drop formed from melting below the melting layer. The mean drop diameter calculated below the melting layer | ||
acts as the lower limit for the mean drop sizes as the rain descends to lower levels. This algorithm is only | ||
active if 1) the snow-graupel density above the melting level (i.e.\f$T_c<0^{o}C\f$) is \f$<225kg m^{-3}\f$ | ||
(which corresponds to an RF=10), 2) the rain content does not exceed \f$1gm^{-3}\f$, and 3) there is vertical | ||
continuity of the rain at lower levels with the rain that formed from melting ice. | ||
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The FA scheme also uses a drizzle parameterization in order to minimize the spatial extent of light (<20dBZ) | ||
reflectivity echoes that developed at the top of moist boundary layers, over the Southeastern U.S., within | ||
warm conveyor belts, and over ocean areas covered by stratocumulus in the NMMB. The drizzle parameterization | ||
uses a variable \f$N_{or}\f$ following Westbrook et al. (2010) \cite westbrook_et_al_2010, and approach | ||
conceptually similar to that described in Thompson et al.(2008) for drizzle. Figure 2a | ||
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\section intra_famp Intraphysics Communication | ||
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+ For grid-scale condensation and evaporation of cloud process (\ref arg_table_zhaocarr_gscond_run) | ||
+ For precipitation (snow or rain) production (\ref arg_table_zhaocarr_precpd_run) | ||
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\section gen_famp General Algorithm | ||
+ \ref general_gscond | ||
+ \ref general_precpd | ||
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*/ |