windprofiler radars and detection of ste events w.k. hocking university of western ontario

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Windprofiler Radars and detection of STE eve W.K. Hocking University of Western Ontario

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Page 1: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Windprofiler Radars and detection of STE events

W.K. HockingUniversity of Western Ontario

Page 2: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Radar.

Small airport radars to giant dishes…

Page 3: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Purpose – to create a narrow beam of radiation, of VERY high intensity.

Page 4: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Japan MU radar

Looks like a dish…

Page 5: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Zoom in…

> $10M for 1 radar in 1985!!

Page 6: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

With a dish, we can move itaround …

But even if we cannot do that with our radar, we CAN steer the beam by feeding different signals to different antennas – the whole beam can be steered in a fraction of a second!

Page 7: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

The Canadian approach…

Effective, and much cheaper…

Page 8: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Require:

High Power – 40 kW in short bursts

c.f. Japan and Germany – 1 MW.

But our system is still effective, and by spreading multipleradars across the province, we gain great meteorologicaladvantage.

Page 9: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 10: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Receivingand DigitizationSystem

Page 11: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

BeamSteeringUnit

Page 12: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Highly sensitive receivers are needed – transmitted signal is kilovolts, but received signal is microvolts!

Special signal processing is required – coded pulses, coherent integration, spectral fitting…

Page 13: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 14: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Measure winds, turbulence, backscattered power.

Page 15: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Armin Dehghan, poster

Page 16: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 17: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 18: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Relation to Ozone?

Page 19: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 20: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Radar/Ozone

Page 21: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 22: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 23: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 24: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 25: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 26: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 27: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Why is there enhanced scatter at the tropopause?

1.Specular Reflectors

Page 28: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Sheets….

Common in regions of HIGH STATIC STABILITYe.g. tropopause.

Page 29: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 30: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Turbulence

Page 31: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

When people talk about turbulence,they often talk about “eddies”.

We often envisage turbulent particletrajectories to be elliptical in shape...

Page 32: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

“Eddies”(Laboratory photographs of tracers)

Page 33: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Due to the velocity shears (differential velocities)in the fluid, even initially isotropic objectsare stretched and torn apart ...

Page 34: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Computer simulations showing vorticitystrings in a patch of turbulence (Werne, Fritts et al.)

Page 35: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

There are also various stages of turbulence - developing,steady-state, and decaying.

Page 36: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Enhanced VHF signal due to

EITHER specular reflections or turbulence

Page 37: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Yamadaet al., GRL, 2001.

Time

sequence.

It may appear in patches of limited extent...

Cause of upper level turbulence – Gravity Waves.

Page 38: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 39: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Gravity waves propagating upward increase In amplitude as they encounter regions of high static stability.

Can result in turbulent layers just above the tropopause.

Page 40: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

t=0 t=t1

z z

xx

--------- Layering

Page 41: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 42: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Energy deposition - at the smallest scales, large wind-shears produce fluid frictional heating (depositionof kinetic energy).

We talk about the “energy dissipation rate”

Energy may also be dissipated by deposition of potential energy.

Turbulence may in fact also function as a storage mechanism of energy.

Page 43: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

C. Diffusion...

Diffusion is often represented by an “eddy diffusion coefficient”,using an analogy with molecular diffusion.

But this grossly over-simplifies the process of turbulent diffusion in the atmosphere.

Different diffusion mechanisms apply at different scales.

Page 44: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

4. What are the unique aspects of turbulence pertaining to the atmosphere?

In the atmosphere, turbulence is:

Spatially and temporally variable and intermittent

Frequently anisotropic

Driven by multiple phenomena, some of which themselves are scale dependent.

Subject to unique measures of stability (Richardson number compared to Reynolds number, Froude number etc.)

Species-dependent (ions compared to electrons compared to neutrals)

Page 45: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Layered structures higher up ...

Page 46: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Fully developed turbulence (FM-CW radar,Eaton et al.)

LAYERING in Turbulence

Page 47: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 48: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Czechowsky et al.

Page 49: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario
Page 50: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Relevance here?

Homogeneous Turbulence:

cmolecular diametermean free path

K = Lv, L = “eddy size”, v = associated velocity.

K = L2/T, L = dimension, T = time scale.

L = (KT)1/2

Page 51: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

K = 1-10 m2s-1, T = 4 days,

D ~ 2 km.

????

Page 52: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

But does this apply in the case of layered turbulence?

Page 53: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

K = K(Layer depth, Klayer, Freq. of Occ., Spatial variability)

K = c1./N2, K=Lv etc no longer apply!

Current models grossly oversimplify K.

Page 54: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Relevance to STE.

How does ozone cross the stable tropopause layer?

Need for turbulent transport?Turbulent layers at the tropopause?

Is FlexPart always valid? Do we need to “open the tap” first?

Page 55: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Mohammed Osman

Page 56: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

Jet Stream can generate gravity waves.Production of small scale turbulence?

Page 57: Windprofiler Radars and detection of STE events W.K. Hocking University of Western Ontario

The End

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