G REGORY T HOMPSON, R OY M . R ASMUSSEN, AND K EVIN M ANNING
description
Transcript of G REGORY T HOMPSON, R OY M . R ASMUSSEN, AND K EVIN M ANNING
Explicit Forecasts of Winter Precipitation Using an Improved Bulk Microphysics
Scheme.Part : Description and Sensitivity AnalysisⅠ
GREGORY THOMPSON, ROY M. RASMUSSEN,
AND KEVIN MANNING
February 2004 Monthly Weather Review 519~542
1.Introduction
• Explicit bin-resolving cloud models(Rasmussen et al 2002, hereafter RG)
• Bulk microphysics parameterization• 利用 Reisner et al.(hereafter RRB) 作為修正基準• 目的:改善顯示 (explicit) 的即時過冷水滴預報,藉以防止飛機積冰 (aircraft icing) 的現象發生
Note : 利用 bulk model 來替代 explicit model ,節省計算時間
2.Description of the bulk microphysics
parameterization
• Initiation of cloud ice• Autoconversion • Treatment of graupel• Intercept parameter of the snow size distribution • Intercept parameter of the rain size distribution
Initiation of cloud ice
Fletcher 1962
Meyers 1992
Cooper 1986
Note : 在最近的研究指出 ice 的形成 Si >5% , T<-5℃
Autoconversion
Kessler 1969
Berry 1968
(Berry and Reinhardt 1974)
υ is a gamma distribution parameter
Qr is rain content,Db=0.3, Nb is cloud droplet concentration, Qc is the cloud water content
Treatment of graupel
改進冰雹形成中兩個最大量:
Rutledge and Hobbs 1983
1983 Hobbsand Rutledge
)/(101.0
)/(105.0
,1/
3
3
kgkgq
kgkgq
PSACWPSDEP
s
c
Intercept parameter of snow size
• 因為固定的截斷參數 (N0,S) 使得過多的雲水被消耗• 發展一個跟混和比和 single moment 相關的關係式 (Sw
ann 1998)• 平均粒子直徑跟溫度一起增加,且 N0,S和 λ 減小時,溫度也會增加 (Houze et al. 1979)
Houze et al 1979
灰粗線 /虛線是利用 Houze et al.1979
細實線 /虛線是 Reisner et al.1998
Intercept parameter of rain size distribution
• Droplet size drizzle drops rain ( 雨滴的形成過程 )
• 在大部分的 single moment scheme 中,都是假設雨水突然由雲水形成而且呈現 Marshall-Pamler size distibution and intercept parameter(8106(m-4))
• 考慮 drizzle to rain
小雨滴
大雨滴
粗實線是利用上頁公式畫出來的終端速度和雨混和比圖,虛線是利用 N0,r= 8106(m- 4) 做出來的圖
3.Approach • Mesoscale model (MM5) • 2-D idealized configuration• 120points, spacing 10km
• 39σp level, flow is 15ms-1
• Bell-shaped mountain 1km high with 100km half-width
敏感度實驗的設定
4.Sensitivity tests
CONTROL experiment
b.Bin model
Initial cloud ice 是利用 Cooper(1986)
c.Ice initial:Meyers and Fletcher experiment
• Fletcher experiment 減少了 cloud ice 在鋒值的數量
• Meyers experiment 增加了 cloud ice 的數量
d.Autoconversion:Kessler1, Kessler5, B
erry, and BandR
Kessler1(qco=0.110-3)
Kessler5(qco=0.5 10-3)
Berry(1986)
BandR(Berry and Reinhardt
autoconversion 1974)
e.CCN spectra:Maritime, Continent1, and Continent2
experiment
Maritime(Nc=50cm-3)
Continent1(Nc=200cm-3)
Continent2(Nc=500cm-3)
f.Treatment of graupel: Graupel1
and Graupel2 experiment
Graupel1:original exponential distribution, No,g=4 106m-4, and Reisner rimed snow-to-graupel conversion
Graupel2:Riming growth of snow must be 3 times larger then depositional growth before creating graupel
g.Version2
• 把 Fletcher, Kessler5, Graupel1 一起使用
• 可以得到一個非常接近 Graupel1 的結果,所以在這三組實驗中以 Graupel1 比較敏感
h.Snow intercept parameter:SON and SONV experiment
SON(No,s=2 107m-4)
SONV(No,s=f(T))
i.Rain intercept parameter:RON
and RONV
RON(No,r=11010m-4)
RONV(No,r=f(qr))
Note : combine SNOV
j.Final experiment
BandR, Graupel2, SONV, RONV 一起使用
k.Deeper/colder cloud system
• CCT=-25℃• CCT=-60℃• Seeder and feeder system
CCT=-25℃
CCT=-60℃
Seeder and feeder system
上層都是由冰晶跟雪組成的溫度較低的雲
下層是混和雲
在經過兩小時之後上層的雲開始影響下層
在下層會有一些過冷毛雨被冰覆蓋落在地面
Conclusion • Primary ice nucleation using Copper(1986), replaces the
Fletcher(1962) curve• Autoconversion using Walko et al.(1995), replaces the
Kessler scheme• A generalized gamma distribution for graupel (eq. 8)
replaces the exponential distribution; the intercept parameter depends on mixing ratio (eq. 10) instead of constant; and riming growth of snow must exceed depositional growth of snow by a factor 3 before rimed snow transfers graupel
• The intercept parameter of snow size distribution depends on temperature replacing the mixing ratio dependency
• The intercept parameter for rain size distribution depend on mixing ratio, thereby simulating the fall velocity of drizzle drops as well as raindrops