impact of new arpege physics on rico case

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Impact of new ARPEGE physics on RICO case (19-sept- 2006) GCSS-GPCI / BLCL-RICO 18-21 sept 2006 P. Marquet, CNRM. Toulouse. Météo- France. + ARPEGE CLIMATE & N.W.P. team + Meso-Scale CNRM team + ENM (School of Met.) + CERFACS + IPSL- LMD …

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GCSS-GPCI / BLCL-RICO 18-21 sept 2006. Impact of new ARPEGE physics on RICO case. P. Marquet, CNRM . Toulouse . Météo-France. (19-sept-2006). + ARPEGE CLIMATE & N.W.P. team + Meso-Scale CNRM team + ENM (School of Met.) + CERFACS + IPSL-LMD …. Introduction. - PowerPoint PPT Presentation

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Page 1: Impact of new ARPEGE physics on RICO case

Impact of new ARPEGE physics on RICO case Impact of new ARPEGE physics on RICO case

(19-sept-2006)

GCSS-GPCI / BLCL-RICO 18-21 sept 2006

P. Marquet, CNRM. Toulouse. Météo-France.

+ ARPEGE CLIMATE & N.W.P. team + Meso-Scale CNRM team

+ ENM (School of Met.) + CERFACS + IPSL-LMD …

Page 2: Impact of new ARPEGE physics on RICO case

IntroductionIntroduction First aim of the study :

Run the French Météo-France (CNRM) ARPEGE-CLIMAT SCM for the new RICO_composite (L80 and L31) …

Send the results for the inter-comparison : done / Pier …

+ 4 Impact studies : Test STANDARD versus NEW physics (Turb, Conv, -Phys) ?

Test of ( L80 / t = 5 mn ) versus ( L31 / t = 15 mn ) ?

Impact of the explicit Top PBL entrainment ?

Impact of the (Dry)-thermals ?

Page 3: Impact of new ARPEGE physics on RICO case

The Climate ARPEGE physics : STANDARD / NEW1 / NEW2The Climate ARPEGE physics : STANDARD / NEW1 / NEW2

STANDARD / V3-V4 NEW1 / Mixed NEW2 / IPCC / full-Diagnostic Diag+Prog full-Prognostic

TURB DIAG. Mellor-Yamada DIAG. M&Y PROGN. / C.B.R. e / t = 0 e / t = 0 e / t = P + Dif – Dis

moist PDF / Bougeault moist PDF / moist PDF / Bougeault Bougeault / Bechtold

Micro-Phys DIAG. PROGN. PROGN.Smith/Kessler Smith/Kessler Bulk - Lopezq_liq / q_ice q_liq / q_ice q_cloud / q_rain

Shallow part in TURB , but why ? Mass-Flux Mass-FluxConvection + Mass-Flux Bougeault ? CAPE / Gueremy CAPE / Gueremy

Deep Mass-Flux / Bougeault Mass-Flux Mass-FluxConvection Convergence of HU CAPE / Gueremy CAPE / Gueremy

Top-PBL NO YES YESEntrainment Grenier & Breth. Grenier & Breth.

Page 4: Impact of new ARPEGE physics on RICO case

Validation of N_low : GCM (T63-L31)Validation of N_low : GCM (T63-L31)

Strato Cu<- STD

(DJF+JJA)N_low - ISCCP

Strato Cu<- NEW

Lopez + CV_GY

+ TKE-CBR

+ Ent_PBL

Page 5: Impact of new ARPEGE physics on RICO case

The NEW2 turbulent scheme : TKE-CBRThe NEW2 turbulent scheme : TKE-CBR

TKE-C.B.R. (2000) + B.L. (1989) for Mixing Length + F2 & 3 / Bougeault (1982) & Bechtold (1995) ; EUROCS : GCM <-> EPCI+GPCI+ACI <-> SCM

Page 6: Impact of new ARPEGE physics on RICO case

Micro-physics : pdf

TKE-C.B.R. (2000) + B.L. (1989) + F2 & 3 / Bougeault (1982) & Bechtold (1995)

Variance of q_cloud : PDF Variance of q_cloud : PDF

Sc

Cu

Page 7: Impact of new ARPEGE physics on RICO case

An Explicit Top-PBL EntrainmentAn Explicit Top-PBL Entrainment

Grenier (ARPEGE)

Vertical Diffusion of theBetts variables : _l and q_t

( A1 = 0.16 )( A2 = 0.0 )

Page 8: Impact of new ARPEGE physics on RICO case

SCM / EUROCS_ARM_Cu (Lenderink)SCM / EUROCS_ARM_Cu (Lenderink) q_cloud

ARP-NEW2 / L19

+ Top PBL ent.

LES-KNMI

ARP-NEW2 / L19

ARP-STD / L19

Page 9: Impact of new ARPEGE physics on RICO case

SCM / EUROCS_ARM_Cu (Lenderink)SCM / EUROCS_ARM_Cu (Lenderink) THETA (L19)

ARP-NEW2 +Top PBL ent.

LES-KNMI

ARP-NEW2

ARP-STD

Page 10: Impact of new ARPEGE physics on RICO case

Ayotte 24SC / L96Ayotte 24SC / L96

Hourdin, Couvreux,

Menut, J.A.S., 2002.

Page 11: Impact of new ARPEGE physics on RICO case

And for RICO ?And for RICO ?

Impact studies :

Test STANDARD versus NEW physics : STD versus NEW2

L80 / t = 5 mn ; L31 / t = 15 mn

Impact of the explicit Top PBL entrainment : NEW2_noent

Impact of the (Dry)-thermals : NEW2_noDTh

Page 12: Impact of new ARPEGE physics on RICO case

RICO L80 / THETA_l

NEW2_noent

NEW2_noDTh

STD NEW2

STD instable ; NEW2 better, But with a drift z>2km ?a –0.5 K bias in the PBL ?a very small impact of « entr. »a large impact of Dry Thermals

Page 13: Impact of new ARPEGE physics on RICO case

RICO L31 / THETA_l

NEW2_noent

NEW2_noDTh

STD NEW2

STD noisy ; NEW2 better, with a smaller drift z>2km ! ?a –0.5 K bias in the PBL ?a greater impact of « entr. »and larger impact of Dry Thermals

Page 14: Impact of new ARPEGE physics on RICO case

RICO L80 / Zonal Wind

STD NEW2 NEW2_noent

NEW2_noDTh

STD noisy ; NEW2 better, But why these oscillations ?A small impact of « ent »A greater impact of Dry Thermals

Page 15: Impact of new ARPEGE physics on RICO case

RICO L80 / Cloud Cover

NEW2_noent

NEW2_noDTh

STD NEW2

STD very noisy !! NEW2 better, Cloud Base and Maxi OK, Drift of Cloud top <-> theta ?A small impact of « ent »A large impact of Dry ThermalsWhat about the values of C.C. ??

Page 16: Impact of new ARPEGE physics on RICO case

L80

L31

LES KNMI

RICO / Cloud Cover Average 24h - 30h

STD very noisy up to 3.5 km !! NEW2 better L80 : from 0.5 to 2.5 km : OK ; the good shapeL31 : too deep cloud 0.2 to 4 km !!L31 : Large impact of Top PBL entr. !What about the values of C.C. ??

Page 17: Impact of new ARPEGE physics on RICO case

RICO / Cloud Content Average 24h - 30h

L80

L31

LES KNMI

SAME as for CLOUD-COVER… Except that values compare to LES…STD very noisy up to 3.5 km !! NEW2 better L80 : from 0.5 to 2.5 km : OK ; the good shapeL31 : too deep cloud 0.2 to 4 km !!L31 : Large impact of Top PBL entr. !

Page 18: Impact of new ARPEGE physics on RICO case

L80

LES KNMI

RICO / <w’’l> Average 24h - 30h

W/m2

K*(m/s)

W/m2

L31

NEW2 L80 realistic… except close to the surface !!

Page 19: Impact of new ARPEGE physics on RICO case

NEW2

LH (W/m2)L80

NEW2 L80 Cloud Cover

NEW2

L80 Precip. mm/day

NEW2 L80 LWP

Page 20: Impact of new ARPEGE physics on RICO case

L80 LES BOMEX

RICO / TKEAverage 24h - 30h

W/m2 m2/s2

W/m2

L31

Page 21: Impact of new ARPEGE physics on RICO case

ConclusionsConclusions Mainly, questions !…

Apart from the (internal) validation of the ARPEGE physics… Why this drift above 2.5 km ? smaller with L31 /t =15 mn : w ?

Are the oscillations for (u,v) Wind observed by others ?

How to compare Precip & C.C. to LES or Obs. ? => Radiation !

A real interest for this RICO case ! “Composite” -> “Long_Run” ? RICO GPCI & AMMA-CI (next talk)… Continue EUROCS’ method…

A deep impact of top-PBL/TURB shallow convection

Small for EUROCS- Cu / large for RICO… Precip ?

Page 22: Impact of new ARPEGE physics on RICO case

RICO L31 / Cloud Cover

NEW2_noent

NEW2_noDTh

STD

NEW2

STD very noisy up to 4 km !! NEW2 better, But worse than L31 (clud base ?)A large impact of « ent »And larger impact of Dry Thermals

Page 23: Impact of new ARPEGE physics on RICO case

L80

L31

LES KNMI

RICO / <w’q’t> Average 24h - 30h

W/m2

W/m2

(g/kg)*(m/s)

Page 24: Impact of new ARPEGE physics on RICO case

L80 LES KNMI

RICO / <w’’vl> Average 24h - 30h

W/m2 K*(m/s)

W/m2

L31

Page 25: Impact of new ARPEGE physics on RICO case

RICO SH (W/m2)

STD NEW2

STD NEW2

L80

L31 L31

L80

Page 26: Impact of new ARPEGE physics on RICO case

STD NEW2

STD NEW2

RICO LH (W/m2)

L80

L31 L31

L80

Page 27: Impact of new ARPEGE physics on RICO case

RICO Cloud Cover

STD

NEW2 L31 L31

STD

NEW2

L80

L80

Page 28: Impact of new ARPEGE physics on RICO case

RICO Precip.

STD

NEW2

STD NEW2

L31

L80 L80

L31

Page 29: Impact of new ARPEGE physics on RICO case

RICO LWP

STD

NEW2 L31 L31

STD

NEW2 L80 L80