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FA scientific documentation
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/**
\page HWRF_famp HWRF Ferrier-Aligo (FA) Microphysics Scheme
\section des_famp Description

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.

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.

\image html FA_MP_schematic.png "Figure 1: Local Land-atmosphere Interaction (courtesy of Michael Ek)" width=10cm

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).

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.

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




\section intra_famp Intraphysics Communication

+ 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)

\section gen_famp General Algorithm
+ \ref general_gscond
+ \ref general_precpd


*/

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