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Cold Fronts and their relationship to density currents: A case study and idealised modelling experiments Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI, University of Manchester, UK

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Cold Fronts and their relationship to density currents: A case study and idealised modelling experiments. Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI, University of Manchester, UK. Overview. - PowerPoint PPT Presentation

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Page 1: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Cold Fronts and their relationship to density currents: A case study and idealised modelling experiments

Victoria SinclairUniversity of HelsinkI

David SchultzUniversity of Helsinki, FMI,

University of Manchester, UK

Page 2: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Overview• Previous work and some theory concerning cold

fronts and density currents

• A Case Study– Observations– AROME simulation

• Idealised Modeling Experiments– 2D density current and 3D cold front– Quantify governing dynamics

Page 3: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Can cold fronts be considered density currents?

Plenty of papers state that a cold front resembles a density current in appearance

Visual similarity does not equal dynamical similarity

Tower observations of a cold front, Colorado

Shapiro et al. 1985

Page 4: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Density Current theory

0.5ghc k

• Coriolis force can be neglected

• Equations exists which predict the speed of movement as a function of density difference and the depth

• Density currents have a low-level feeder flow behind the leading edge: the wind speeds behind the front (u) are greater than the speed that the gravity current moves at (c)

1

1

Du pfvDt xDv pfuDt y

XX

0u c

Page 5: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Fronts Theory

• Fronts are often assumed to be balanced, at least in the cross front direction

• Acceleration term is assumed to be small.

1

1

Du pfvDt xDv pfuDt y

XX

• No formula to predict the speed that fronts move at

• Uncertainty remains as to what factors control the speed that cold fronts move at

Page 6: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Questions• What controls the speed that cold fronts move

at?– Why do some cold fronts propagate – i.e. move faster

than the normal component of the wind?– Why do some cold fronts move slower than the

normal wind, and hence share a feature with gravity currents?

• When do cold fronts collapse to resemble density currents?

• Are collapsed cold fronts dynamically similar to density currents?

Page 7: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Motivation

• Cold fronts that evolve into gravity current type features can produce hazardous weather

• The scale of a collapsed front means that even high resolution NWP models will not capture the structure and evolution well

Page 8: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Case Study: synoptic evolution

• Developed as a frontal wave on pre-existing front• Mature front and is far from the parent low• Simulated event with AROME 33h1, 2.5km

12 UTC 29 Oct 00 UTC 30 Oct 00 UTC 31 Oct

Page 9: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Shallow frontal zone 00:11 UTC

• Radial wind speeds from Kumpula Radar

• Cold air is confined to a shallow layer

• Resembles a density current

6 m/s

7 m/s

Image provided by Matti Leskinen

Page 10: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Temperature at Kivenlahti

Observations AROME

black: 5 m red: 26 mblue: 48 mmagenta: 93 m

grey: 141 mgreen: 218 mbrown: 266 m orange: 296 m

black: 2 m blue: 38 mmagenta: 112 m

green: 200 m orange: 300 m

Page 11: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Temperature at Kuopio

Observations AROME

black: 5 m red: 26 mblue: 48 mmagenta: 93 m

grey: 141 mgreen: 218 mbrown: 266 m orange: 296 m

black: 2 m blue: 38 mmagenta: 112 m

green: 200 m orange: 300 m

Page 12: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Heat Fluxes

SMEAR III SMEAR II

BLACK: observed. GREY: AROME

Data provided by Annika Nordbo and Ivan Mammarella

Page 13: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

AROME Potential Temperature 900hPa

Page 14: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Location of Cold Front from AROME

Averaged speed of front between 22:00 UTC and 02:00 UTC

Section B = 5.03 ms-1

Section C = 5.47 ms-1

Section A = 6.92 ms-1

Front is located objectively

Hewson (1998)

Jenker et al (2010)

Black: 18:00 UTC

Red: 20:00 UTC

Green: 22:00 UTC

Blue: 00:00 UTC

Purple: 02:00 UTC

Cyan: 04:00 UTC

BB

A

C

Page 15: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Wind Speeds from AROME

• Wind speeds decrease behind the front• Unconvincing evidence of a “feeder flow”

920 hPa 990 hPa

u – c > 0 especially in south u – c ≈ 0

Page 16: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Ascent, potential temperature Simulated Radar reflectivity

22 UTC, B 00 UTC, B

22 UTC, A 00 UTC, A

Page 17: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Case Study Conclusions• Shallow and narrow front

– stable mid-troposphere– Stable BL may have prevented frontolysis by turbulent

mixing

• Dynamics differ to density current dynamics– No clear feeder flow

• Prefrontal boundary layer appears to affect structure

Page 18: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Idealised Modelling with WRF

Page 19: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Idealized Experiment

• WRF-ARW– Weather Research and Forecasting –

Advance Research WRF. V3.1– Non-Hydrostatic, range of physics options– Supported by NCAR

• First simulated a 2D density current at high resolution (100m grid spacing)

• Calculate force balance.

Page 20: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Density Current

5 – 10 minutes : 20.5 ms-1

10 – 15 minutes: 15.3 ms-1

Page 21: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Force Balancelowest model level (995 hPa)

Blue: Potential temperature

Red: Pressure Gradient Force

Purple: Coriolis

Black: Acceleration

Page 22: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Simulate a Cold Front

• Model a full 3D baroclinic life cycle• Include two nested domains over the cold

front– horizontal grid spacing is 100km : 20km : 4km– All nests have 64 levels, model top at 100hPa

• Initial experiment has no moisture and no physical parameterizations

Page 23: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Potential temperature and surface pressure. Day 4.5. Parent domain

Page 24: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Potential Temperature and wind vectors. 20 km domain

Page 25: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Potential temperature and vertical motion

Page 26: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Force balance

Purple: Coriolis

Black: Acceleration

Blue: Potential temperature

Red: Pressure Gradient Force

LEVEL 1 ~ 975 h Pa LEVEL 7 ~ 805 h Pa

Page 27: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Force Balance 5 hrs later

Blue: Potential temperature

Red: Pressure Gradient Force

LEVEL 1 ~ 975 h Pa LEVEL 7 ~ 805 h Pa

Purple: Coriolis

Black: Acceleration

Blue: Potential temperature

Red: Pressure Gradient Force

Page 28: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Conclusions• Idealised cold front does not visually resemble a

density current, but does have many interesting features

• The force balance shows a three way balance near the cold front

• HYPOTHESIS– friction and turbulence will change force balance– Trailing part of cold front will be visually more similar

to density currents

Page 29: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Future work

• Higher resolution (1km) simulation of cold front, include boundary layer scheme

• Different baroclinic life cycles

• Simulate 3D density current at comparable resolution to cold front case

Page 30: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Thank you

You can look at more animations on my webpages

www.atm.helsinki.fi/~vsinclai

Page 31: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Force Balance: 5 hrs later

Page 32: Victoria Sinclair University of HelsinkI David Schultz University of Helsinki, FMI,

Force Balance across cold front