/
Similarities and differences of the internal AMV at 2 resolutions of HadGEM3-GC3.1 Similarities and differences of the internal AMV at 2 resolutions of HadGEM3-GC3.1

Similarities and differences of the internal AMV at 2 resolutions of HadGEM3-GC3.1 - PowerPoint Presentation

Dragonfruit
Dragonfruit . @Dragonfruit
Follow
342 views
Uploaded On 2022-08-04

Similarities and differences of the internal AMV at 2 resolutions of HadGEM3-GC3.1 - PPT Presentation

Michael Lai Jon Robson Laura Wilcox Nick Dunstone Conclusions Models agree AMV of 5070 years with greatest variability in the subpolar Polar and subpolar upper OHC driven by ocean advection subtropical OHC driven by surface fluxes cloud changes ID: 935066

amv amoc density ocean amoc amv ocean density n216 n96 fluxes sea surface driven subsurface labrador nao atmosphere ssh

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "Similarities and differences of the inte..." is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

Similarities and differences of the internal AMV at 2 resolutions of HadGEM3-GC3.1

Michael Lai, Jon Robson, Laura Wilcox, Nick

Dunstone

Slide2

Conclusions

Models agree:

AMV of 50-70 years, with greatest variability in the subpolar.

Polar and subpolar upper OHC driven by ocean advection, subtropical OHC driven by surface fluxes (cloud changes)

Arctic-Atlantic exchanges of S-controlled density anomalies drive subsurface density.

Models disagree:

Ocean circulation changes

N216

: Dominated by latitudinally coherent AMOC changes

N96

: Both AMOC and SPG changes are important

Appears to be explained by subsurface density propagation.

Role of the atmosphere:

N216

: NAO drives Labrador Sea subsurface density

N96

: NAO is not a significant driver of Labrador Sea subsurface density (ocean-only mode?)

Are the differences due to mean state biases or model resolution?

Slide3

Characteristics of the AMV

N96ORCA1:

~135km atmosphere, 1

°

ocean

N216ORCA025

:

~60km atmosphere, 0.25

°

ocean

Slide4

SST, SLP, AMOC evolution

‘NAO’ leads AMV by 10 years. AMOC leads AMV by 5 years.

AMOC anomalies do not move as far South in N96 compared to N216.

Slide5

AMOC highly correlated with AMV in both models.NAO index is significantly correlated with AMV in

N216

but not in

N96

.

SST, SLP, AMOC evolution

Slide6

OHT convergence vs Surface Fluxes

Polar and Subpolar T100: Driven by ocean heat transport convergence

Subtropical T100: Driven by surface fluxes

Slide7

Ocean circulation changes

N216

SSH: SPG spin-up in the Labrador Sea region. GS extension / NAC SSH consistent with AMOC strengthening.

N96

SSH: Decrease in SSH consistent with SPG strengthening.

Slide8

What’s driving the ocean circulation changes?

A source of S-controlled density anomalies moves from the Arctic into the N. At.

Slide9

Role of the atmosphere in driving subsurface density changes

Surface fluxes over the Labrador Sea leads surface fluxes over the

Irminger

Sea

N216

: Wind changes drive SHF

N96

: Wind changes unimportant, SHF driven by vertical mixing instead?

Slide10

Summary schematic

AMOC strengthens

Positive AMV

Arctic dense anomaly

Positive winter NAO

AMOC strengthens

Positive AMV

Arctic dense anomaly

SPG strengthens

N216

N96