Representation of convection and clouds in the IFS ......20 years and - - PowerPoint PPT Presentation

representation of convection and clouds in the
SMART_READER_LITE
LIVE PREVIEW

Representation of convection and clouds in the IFS ......20 years and - - PowerPoint PPT Presentation

Representation of convection and clouds in the IFS ......20 years and still the same? Peter Bechtold with contributions from Richard Forbes and Maike Ahlgrimm IITM Introspect 2017 workshop: IFS clouds and convection Slide 1 Challenge 1:


slide-1
SLIDE 1

IITM Introspect 2017 workshop: IFS clouds and convection Slide 1

Representation of convection and clouds in the IFS......20 years and still the same?

Peter Bechtold with contributions from Richard Forbes and Maike Ahlgrimm

slide-2
SLIDE 2

IITM Introspect 2017 workshop: IFS clouds and convection Slide 2

October 29, 2014

Challenge 1: Convective vs stratiform (grid-scale) precipitation

2 EUROPEAN CENTRE FOR MEDIUM-RANGE WEATHER FORECASTS

TCo1279 26/4/2016

slide-3
SLIDE 3

IITM Introspect 2017 workshop: IFS clouds and convection Slide 3 Cloud (K/day) Conv (K/day) Dynamics (K/day) Radiation (K/day)

P ( h P a) P ( h P a)

Challenge 2: represent accurate heating profiles and cloud radiation interaction

P ( h P a) 50E 100 150 20W 50E 100 150 20W 50E 100 150 20W 50E 100 150 20W

Latitude averaged difference in T-tendency MJO in phase 6/7 – MJO in phase 2/3: Convection over West Pacific - convection over Indian Ocean

slide-4
SLIDE 4

IITM Introspect 2017 workshop: IFS clouds and convection Slide 4

T ask of convection parametrisation

total Q1 and Q2

p s e c L Q Q Q

R C

∂ ′ ′ ∂ − − ≡ − ≡ ω ) (

1 1

Caniaux, Redelsperger, Lafore, JAS 1994

Q1c is dominated by condensation term

1

10 5 z ( k m ) (K/h)

  • 1

2 c-e Q1-Qr trans c-e Q2

10 5 z ( k m ) (K/h)

trans

  • 1
  • 2

2 1 a b

but for Q2 the transport and condensation terms are equally important

parameterization needs to describe the collective effects of a cloud ensemble: Condensation/Evaporation and Transport

slide-5
SLIDE 5

IITM Introspect 2017 workshop: IFS clouds and convection Slide 5

The IFS bulk mass flux scheme

Entrainment/Detrainment Downdraughts Link to cloud parameterization Cloud base mass flux - Closure Type of convection shallow/deep/frontal Where does convection occur Generation and fallout of precipitation

slide-6
SLIDE 6

IITM Introspect 2017 workshop: IFS clouds and convection Slide 6

Large-scale budget equations: M=ρw; Mu>0; Md<0

[ ]

) ( ) ( ) ( F M L e e c L s M M s M s M p g t s

f subcld d u d u d d u u cu

− − − − + + − + ∂ ∂ =       ∂ ∂

Mass-flux transport in up- and downdraughts condensation in updraughts

Heat (dry static energy):

  • Prec. evaporation

in downdraughts

  • Prec. evaporation

below cloud base Melting of precipitation Freezing of condensate in updraughts

Humidity:

[ ] ( )

subcld d u d u d d u u cu

e e c q M M q M q M p g t q − − − + − + ∂ ∂ =       ∂ ∂ ) (

slide-7
SLIDE 7

IITM Introspect 2017 workshop: IFS clouds and convection Slide 7

Large-scale budget equations

Cloud condensate:

u u cu

l D l t ∂   =  ÷ ∂  

[ ]

u M M u M u M p g t u

d u d d u u cu

) ( + − + ∂ ∂ =       ∂ ∂

Momentum:

[ ]

v M M v M v M p g t v

d u d d u u cu

) ( + − + ∂ ∂ =       ∂ ∂

slide-8
SLIDE 8

IITM Introspect 2017 workshop: IFS clouds and convection Slide 8

Entrainment/Detrainment

LES (black) IFS IFS formula with LES data Entrainment formulation looks sooo simple: ε=1.75x10-3 (1.3-RH)f(p) RH=relative humidity, so how does it compare to LES ?

Schlemmer et al. 2017

slide-9
SLIDE 9

IITM Introspect 2017 workshop: IFS clouds and convection Slide 9

9

CAPE closure - the basic idea

large-scale processes generate CAPE Convection consumes CAPE

slide-10
SLIDE 10

IITM Introspect 2017 workshop: IFS clouds and convection Slide 10

Closure - Deep convection

, , v u v e u esat v esat cloud cloud

T T CAPE g dz g dz T θ θ θ − − = ≈

∫ ∫

Use instead density scaling, time derivative then relates to mass flux:

, ,

1 1

Ptop Ptop v u v u v v base v v v Pbase Pbase base LS Cu BL Cu LS BL Cu shal deep

T T T T p PCAPE dp dp t T t T t T t PCAPE PCAPE PCAPE t t t

+ + = +

∂ − ∂ ∂ ∂ ≈ − − + = ∂ ∂ ∂ ∂ ∂ ∂ ∂ = + + ∂ ∂ ∂

∫ ∫

1 442 4 4 3 1 4 4 4 4 442 4 4 4 4 4 4 3

, Ptop v u v v Pbase

T T PCAPE dp T − = − ∫

this is a prognostic CAPE closure: now try to determine the different terms and try to achieve balance

/ / , /

cu LS

PCAPE t PCAPE t PCAPE t ∂ ∂ ∂ ∂ ∂ ∂ =

slide-11
SLIDE 11

IITM Introspect 2017 workshop: IFS clouds and convection Slide 11

Closure - Deep convection

* * , u d u b bl

M M M M PCAPE = +

* , , , * *

1 ; 1

BL u b u b u b v v cloud pbase v BL BL psurf BL

PCAPE PCAPE M M M T g M dz T z T PCAPE dp T t τ τ − = ≥ ∂ ∂ ∂ = − ∂

∫ ∫

Solve now for the cloud base mass flux by equating 1 and 2 Mass flux from the updraught/downdraught computation initial updraught mass flux at base, set proportional to 0.1Δp contains the boundary-layer tendencies due to surface heat fluxes, radiation and advection see Bechtold et al. 2014 JAS and work bei Saolo Freitas

slide-12
SLIDE 12

IITM Introspect 2017 workshop: IFS clouds and convection Slide 12

Impact of closure on diurnal cycle

JJA 2011-2012 against Radar

Bechtold et al., 2014, J. Atmos. Sci. ECMWF Newsletter No 136 Summer 2013

Obs radar NEW=with PCAPEBbl term

slide-13
SLIDE 13

IITM Introspect 2017 workshop: IFS clouds and convection Slide 13

October 29, 2014

Resolution scaling +absolute mass flux limit

10 km 5 km

Developed in collaboration with Deutsche Wetterdienst and ICON model

( )(

)( )

e c e c

Φ − Φ − − = Φ − Φ = Φ′ ′ ω ω σ σ ω ω ω 1

f(Δx)

Kwon and Hong, 2016 MWR independently developed very similar relations

slide-14
SLIDE 14

IITM Introspect 2017 workshop: IFS clouds and convection Slide 14

October 29, 2014

Cy42r1 Tco1999 no deep Cy42r1 TCo1999 5 km scaled Mfl Obs 9 Aug 2015 Cy42r1 TCo1999 5 km

Convection parameterisation at 5km resolution

14

Resolution scaling and a bit of light in the grey zone

slide-15
SLIDE 15

IITM Introspect 2017 workshop: IFS clouds and convection Slide 15

October 29, 2014

Convection issue 1: inland penetration of (winter snow) showers

Obs 42r1 TCo1279 Oper advection

15 EUROPEAN CENTRE FOR MEDIUM-RANGE WEATHER FORECASTS

slide-16
SLIDE 16

IITM Introspect 2017 workshop: IFS clouds and convection Slide 16

Realism of heating profiles: DYNAMO MJO campaign

Importance of melting level and mixed-phase microphysics: : green shows smaller discontinuity at the melting level

with J-E Kim and C. Zhang

slide-17
SLIDE 17

IITM Introspect 2017 workshop: IFS clouds and convection Slide 17

October 29, 2014

Issue: Global models are not reflective enough over the Southern Ocean, but too reflective over tropical oceans

Li et al. 2013 (blue = not reflective enough) Annual mean 10-20 Wm-2 difference from CERES-EBAF

17 EUROPEAN CENTRE FOR MEDIUM-RANGE WEATHER FORECASTS

Also true for IFS even if total cloud cover against ISCCP and MODIS looks pretty good IFS MODIS

slide-18
SLIDE 18

IITM Introspect 2017 workshop: IFS clouds and convection Slide 18

Issue: not reflective enough storm tracks

Effect of detraining more liquid phase condensate to cloud scheme corrects SW radiation error in SH storm tracks (during cold air

  • utbreaks) by around 5

W/m2 or 20% future tests: producing only liquid for shallow, but requires more technical developments and might produce biases

slide-19
SLIDE 19

IITM Introspect 2017 workshop: IFS clouds and convection Slide 19

October 29, 2014

Issue too reflective subtropics: sensitivity to shallow detrainment

19 C42r1- MODIS low cloud cover: annual mean 43r1-42r1 change in low cloud cover

slide-20
SLIDE 20

IITM Introspect 2017 workshop: IFS clouds and convection Slide 20

Subgrid BL turbulent mixing

Moist process parametrizations:

The integrated view

Subgrid convection Subgrid cloud Microphysics Examples: Increased consistency between existing parametrizations Prognostic cloud PDF schemes (e.g. Tompkins et al 2002) Eddy-diffusivity + multiple mass flux plumes (e.g. EDMF Dual-M) Higher order closure (e.g. CLUBB)

Dynamics Radiation Surface interactions

How the different parametrizations interact can be as important as the parametrizations themselves

slide-21
SLIDE 21

IITM Introspect 2017 workshop: IFS clouds and convection Slide 21

Microphysics Parametrization: The “category” view

Single moment schemes

Cloud ice qi Snow qs Cloud water ql Rain qr Water vapour qv

Freezing - Melting Autoconversion Collection Autoconversion Collection Freezing – Melting - Bergeron Deposition Sublimation Condensation Evaporation Collection

Rutledge and Hobbs (1983)

Sedimentatio n

slide-22
SLIDE 22

IITM Introspect 2017 workshop: IFS clouds and convection Slide 22

Microphysics Parametrization: The “category” view

Double moment schemes

Cloud ice qi + Ni Snow qs + Ns Cloud water ql + Nl Rain qr + Nr Water vapour qv

Freezing - Melting Autoconversion Collection Autoconversion Collection Freezing – Melting - Bergeron Deposition Sublimation Condensation Evaporation Collection

e.g. Ferrier (1994) Seifert and Beheng (2001) Morrison et al. (2005)

Sedimentatio n

slide-23
SLIDE 23

IITM Introspect 2017 workshop: IFS clouds and convection Slide 23

Microphysics Parametrization: The “category” view

Double moment schemes – multiple ice categories

Snow qs + Ns

Cloud water ql + Nl Rain qr + Nr Water vapour qv

Freezing - Melting Autoconversion Collection Freezing – Melting - Bergeron Deposition Sublimation Condensation Evaporation Collection

Cloud ice qi + Ni

Sedimentatio n

Graupel qg + Ng Hail qh + Nh

e.g. Lin et al. (1983) Meyers et al. (1997) Milbrandt and Yau (2005)

slide-24
SLIDE 24

IITM Introspect 2017 workshop: IFS clouds and convection Slide 24

24

Microphysics Parametrization: The cloud fraction

qt

Uniform-delta:

Tiedtke (1993)

  • The ECMWF global NWP model has prognostic water

vapour, cloud water and cloud fraction. With a uniform function for heterogeneity in the clear air and a delta function (homogeneous) in-cloud.

  • The UK Met Office global NWP model (PC2 scheme)

also has prognostic water vapour, cloud water and cloud fraction.

  • Many other operational global NWP/climate models

have diagnostic sub-grid cloud schemes, e.g. NCEP GFS: Sundquist et al. (1989)

  • Research is ongoing for statistical schemes with

prognostic PDF moments (e.g. Tompkins scheme tested in ECHAM, CLUBB tested in CAM).

qt

Double-Gaussian

(CLUBB)

qt

slide-25
SLIDE 25

IITM Introspect 2017 workshop: IFS clouds and convection Slide 25

25

Mixed-phase clouds: Mixed-phase clouds:

Observed supercooled liquid water occurrence Observed supercooled liquid water occurrence

Observations:

  • Colder than -38oC, no supercooled liquid water.
  • Supercooled liquid water increasingly common as

approach 0oC.

  • Often in shallow layers at cloud top, or in strong

updraughts associated with convection

  • Often mixed-phase cloud – liquid and ice present
  • Convective clouds with tops warmer than -5oC

rarely have ice. Lidar: high backscatter from liquid water layers

Lidar in space

Lidar: lower backscatter from ice cloud

slide-26
SLIDE 26

IITM Introspect 2017 workshop: IFS clouds and convection Slide 26

Parametrizing cloud phase

Diagnostic vs prognostic

  • Many (global) models with a single condensate prognostic parametrize ice/liquid

phase as a diagnostic function of temperature (see dashed line for ECMWF model pre-2010 below).

  • Models with separate prognostic variables for liquid water and ice, parametrize

deposition allowing a wide range of supercooled liquid water/ice fraction for a given temperature (see shading in example below). PDF of liquid water fraction of cloud for a diagnostic mixed phase scheme (dashed line) and prognostic ice/liquid scheme (shading)

∂m ∂t = 4πsCF Ls RT −1      ÷ Ls k

aT + RT

χe

si

slide-27
SLIDE 27

IITM Introspect 2017 workshop: IFS clouds and convection Slide 27

Why represent heterogeneity?

Important scales of cloud cover & reflectance

Contribution to global cloud cover (solid), number (dotted) and SW reflectance (dashed) from clouds with chord lengths greater than L (based on MODIS, aircraft and NWP data).

(from Wood and Field 2011, JClim)

Map of the cloud size for which 50% of cloud cover comes from larger clouds (from 2 years of MODIS data)

50% of cloud cover is from clouds with scale > 200 km 85% of cloud cover is from clouds with scale > 10 km 15% of cloud cover is from clouds with scale < 10 km Larger scales dominate mid-latitude storm tracks Small scales dominate over subtropical ocean

slide-28
SLIDE 28

IITM Introspect 2017 workshop: IFS clouds and convection Slide 28

Cloud heterogeneity in radiation and microphysics (autoconversion): using fractional standard deviation FSD

E.g.:

  • Enhanced heterogeneity in winter storm

tracks, summertime NH continent

  • detrainment ratio highlights areas with

enhanced variability

  • apparent height dependence in zonal mean

CALIPSO observed FSD Parameterized

3.0

current assumption in radiation: FSD=1