Lecture 3

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Experimental determination of the PBL depth, Thermally driven winds, Slope winds, Valley winds, Cold air pools, Low level jets

Last updated 8:10 AM on 6/20/26
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51 Terms

1
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What is the parcel method used for?

determination of PBL depth from measurements

2
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Which two applications of the parcel method exist in general?

simple and advanced parcel method

3
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Describe the simple parcel method.

seek height where potential temperature profile equals the surface temperature

assumes a CBL-like vertical structure

in SBL no PBL-depth which is a problem

does not account for mixing due to windshear

<p>seek height where potential temperature profile equals the surface temperature</p><p>assumes a CBL-like vertical structure</p><p>in SBL no PBL-depth which is a problem</p><p>does not account for mixing due to windshear</p>
4
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Describe the advanced parcel method.

does account for a surface temperature excess delta theta which represents effects of entrainment in the unstable case and of shear-driven mixing in the stable case

works well for CBL and SBL

delta theta is scaled on the strength of shear

<p>does account for a surface temperature excess delta theta which represents effects of entrainment in the unstable case and of shear-driven mixing in the stable case</p><p>works well for CBL and SBL</p><p>delta theta is scaled on the strength of shear</p>
5
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What is the gradient method used for?

determine PBL depth from measurements

6
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Describe the gradient method.

seek height of strongest potential temperature gradient (or other quantities RH, q)

alternatively height where potential temperature gradient exceeds a predetermined value

7
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What is a known issue when using parcel or gradient method to determine PBL depth?

often PBL-depths don’t agree between methods

<p>often PBL-depths don’t agree between methods</p>
8
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Describe how wavelet algorithms work with LIDAR backscatter measurements to determine the PBL-depth.

uniform strong backscatter in lower well mixed BL

weak backscatter in free atmosphere above

transition trough entrainment zone in the shape of a haar wavelet

wavelet slides up the profile, at transition zone suddenly strong negative contribution → PBL depth

<p>uniform strong backscatter in lower well mixed BL</p><p>weak backscatter in free atmosphere above</p><p>transition trough entrainment zone in the shape of a haar wavelet</p><p></p><p>wavelet slides up the profile, at transition zone suddenly strong negative contribution → PBL depth</p>
9
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How can one determine the PBL depth from SODAR backscatter?

CBL: sharp vertical changes in turbulence and temperature stratification at BL top cause elevated max. in reture signal → look for secondary maximum in the SODAR-backscatter

SBL: less useful, if necessary look for hight of strongest curvature of SODAR-backscatter

10
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What are the key steps to get to the linearized version of the ideal gas law?

assume mean + pertubation and pert. « mean

insert in ideal gas law, products of pertubations are small → neglect

use ideal gas law with only mean quantities, insert and bring equation to form: pertubations / means

<p>assume mean + pertubation and pert. « mean</p><p>insert in ideal gas law, products of pertubations are small → neglect</p><p>use ideal gas law with only mean quantities, insert and bring equation to form: pertubations / means</p>
11
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How does the linearized version of the ideal gas law look?

knowt flashcard image
12
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From which equation can the diurnal cycle of the mean circulation in the PBL be understood?

Vorticity eqation, especially the baroclinic production term

<p>Vorticity eqation, especially the baroclinic production term</p>
13
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What would be a typical example for a diurnal variable mean circulation in the PBL

Sea breezes

<p>Sea breezes</p>
14
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How does the baroclinic production term can be written in terms of buoyancy?

knowt flashcard image
15
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What is a key property of all thermally driven winds?

have a distinct diurnal variability

16
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What are favourable conditions for pronounced thermally-driven winds?

days with clear skies, strong incoming solar radiation, weak synoptic scale pressure gradients

17
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What are typical velocity scales of thermally-driven winds?

a few m/s, rarely above 10-15m/s

18
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What is the main reason for the variety of thermally driven circulation systems over mountains?

differential heating at various spatial scales

19
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What are the three thermally-driven winds over mountains?

slope winds

valey winds

plane-to-mountain winds

<p>slope winds</p><p>valey winds</p><p>plane-to-mountain winds</p>
20
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For differential heating, which are the warm/cold sectors for daytime slope winds?

atmosphere near slope (warm) and atmosphere in the valley and the adjacent plain (cold)

21
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For differential heating, which are the warm/cold sectors for daytime valley winds?

atmosphere in the valley (warm) and atmosphere in the adjacent plain (cold)

22
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How do slope winds behave at night?

surface cools at slope and leads to local stable stratification, from the baroclinic production term resulting cross-wise vorticity is postive → into the picture

so we get flow down the slope

<p>surface cools at slope and leads to local stable stratification, from the baroclinic production term resulting cross-wise vorticity is postive → into the picture</p><p>so we get flow down the slope</p>
23
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How do slope winds behave during daytime?

local heating of slope leads to local unstable stratification, from baroclinic production term resulting cross-wise vorticity is negative → out of the picture

so we get flow up the slope

24
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What is an alternative view to understand slope winds apart from local stratification?

Looking at pressure pertubations,

heating hydrostatically induces a pressure pertubation near the slope

the vector sum of the buoyancy force due to heating and the pressure gradient result in upslope acceleration

(local differences in heating → isobars not parallel)

friction counteracts acceleration → steady state

<p>Looking at pressure pertubations, </p><p>heating hydrostatically induces a pressure pertubation near the slope</p><p>the vector sum of the buoyancy force due to heating and the pressure gradient result in upslope acceleration</p><p>(local differences in heating → isobars not parallel)</p><p>friction counteracts acceleration → steady state</p>
25
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What does the Prandlt model describe?

describes steady state of slope wind system

model cast in rotated coordinates parallel/normal to the slope (s,n)

provides a profile along n of wind speed and temperature pertubation caused by surface heating/cooling

model is 1D → does not account for any variability along s

provides similar to Ekman spiral analytic solution to Navier-Stokes equations and features an exponential decay of disturbances

<p>describes steady state of slope wind system</p><p>model cast in rotated coordinates parallel/normal to the slope (s,n)</p><p>provides a profile along n of wind speed and temperature pertubation caused by surface heating/cooling</p><p>model is 1D → does not account for any variability along s</p><p>provides similar to Ekman spiral analytic solution to Navier-Stokes equations and features an exponential decay of disturbances</p>
26
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What are the governing equations for the Prandl model for flow over a slope?

alpha … slope angle

us … along slope wind component

K … eddy transfer coefficients

gamma … potential temperature gradient in the environment

<p>alpha … slope angle</p><p>us … along slope wind component</p><p>K … eddy transfer coefficients</p><p>gamma … potential temperature gradient in the environment</p>
27
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What are eddy transfer coefficients?

for momentum and heat they account for mixing effect of atmospheric turbulence,

for the laminar version of the Prandtl model they become the molecular transfer coefficients (nu, Kappa)

for atmospheric processes they are essentially tuning parameters (1-10 m²s^-1)

<p>for momentum and heat they account for mixing effect of atmospheric turbulence,</p><p>for the laminar version of the Prandtl model they become the molecular transfer coefficients (nu, Kappa)</p><p>for atmospheric processes they are essentially tuning parameters (1-10 m²s^-1)</p>
28
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What are the solutions to the Prandtl model assuming steady state?

knowt flashcard image
29
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What are important properties of the solution to the Prandtl model?

  • amplitude of pertubation not dependant on slope angle → upslope speed same for same pertubation

  • steeper slopes → pertubations with shorter wavelenght and faster decay with n,
    shallow slopes → deep upslope circulation systems

  • no solution for alpha = 0 (flat terrain) and N = 0 → only exist in stably stratified atmosphere

  • in a well mixed valley there are no slope winds possible → they happen mostly in the morning

30
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What can be a reason for slope winds to detach from the slope?

encountering of an inversion layer, resulting cross -valley circulation sometimes visible as clouds if LCL at right place

<p>encountering of an inversion layer, resulting cross -valley circulation sometimes visible as clouds if LCL at right place</p>
31
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What are reasons for Valley winds?

  • pressure gradients along the valley axis

  • compared to an adjacent plain, the atmosphere of the valley is warmer/cooler during day/night

  • the valley atmosphere has a larger amplitude of diurnal temperature cycle

<ul><li><p>pressure gradients along the valley axis</p></li><li><p>compared to an adjacent plain, the atmosphere of the valley is warmer/cooler during day/night</p></li><li><p>the valley atmosphere has a larger amplitude of diurnal temperature cycle</p></li></ul><p></p><p></p>
32
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How do Valley winds in behave in winter?

they do not exist as the temperature in the valley is cooler day and night than in the plain leading to no positive pressure difference

33
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How do geometric effects impact valley winds?

larger temperature oscillations in the valley due to part of atmospheric volume is taken by orography

stonger heating/cooling because of less volume and more surface area

34
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How does the vertical extent of thermals influence valley winds?

capping inversions below or at mountain top lead to stronger heating in the valley than in the plain → Valley winds

mixing above the mountain top reduces differntial heating

for very strong thermal convection there is basically no differential heating anymore so no valley winds

<p>capping inversions below or at mountain top lead to stronger heating in the valley than in the plain → Valley winds</p><p>mixing above the mountain top reduces differntial heating</p><p>for very strong thermal convection there is basically no differential heating anymore so no valley winds</p>
35
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What is the reason for nocturnal cooling over a flat terrain?

near surface air is cooled by net longwave radiation loss of the uppermost soil layer

baiscally surface cools → atmosphere above cools

36
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How do radiation fluxes behave during nighttime cooling?

downward sensible heat flux

upward ground heat flux

decrease in net outgoing longwave radiation

these 3 processes combined lead to a negative feedback: the more the surface cools, the slower the cooling rate becomes

<p>downward sensible heat flux</p><p>upward ground heat flux</p><p>decrease in net outgoing longwave radiation</p><p>these 3 processes combined lead to a negative feedback: the more the surface cools, the slower the cooling rate becomes</p>
37
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What are factors favouring strong nocturnal cooling and very low temperatures?

cold dry airmass

weak winds (less mixing due to turbulence)

for very stable conditions turbulent heat flux is smaller than the net radiation loss leading to an imbalance which leads to rapid cooling and further surpression of turbulence heat transport → runaway cooling as negative buoyancy wins over shear

<p>cold dry airmass</p><p>weak winds (less mixing due to turbulence)</p><p>for very stable conditions turbulent heat flux is smaller than the net radiation loss leading to an imbalance which leads to rapid cooling and further surpression of turbulence heat transport → runaway cooling as negative buoyancy wins over shear</p>
38
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What are the two major differences for nocturnal cooling in a basin compared to the flat case?

  • concave orography keeps air at basin floor from being mixed with the ambient flow once stable stratifcation has developed, also windless conditions at basin floor established earlier in the night and maintained more easily, by cooling down fastest air at basin floor isolates itself from air higher above

  • sky-view factor reduced → part of downward LW-radiation at basin floor does not originate from the atmosphere, but the surrounding terrain. this effectively enhances net radiation available at night.

<ul><li><p>concave orography keeps air at basin floor from being mixed with the ambient flow once stable stratifcation has developed, also windless conditions at basin floor established earlier in the night and maintained more easily, by cooling down fastest air at basin floor isolates itself from air higher above</p></li><li><p>sky-view factor reduced → part of downward LW-radiation at basin floor does not originate from the atmosphere, but the surrounding terrain. this effectively enhances net radiation available at night.</p></li></ul><p></p>
39
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<p>Example GrĂĽnloch: What is happening in this case?</p>

Example GrĂĽnloch: What is happening in this case?

Clouds first part of the night

<p>Clouds first part of the night</p>
40
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<p>Example GrĂĽnloch: What is happening in this case?</p>

Example GrĂĽnloch: What is happening in this case?

Cooling, then stopped by clouds

<p>Cooling, then stopped by clouds</p>
41
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<p>Example GrĂĽnloch: What is happening in this case?</p>

Example GrĂĽnloch: What is happening in this case?

wind influence leading to mixing

<p>wind influence leading to mixing</p>
42
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Undisturbed evolution

<p>Undisturbed evolution</p>
43
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Late buildup: dissipation of clouds or suddenly weakend winds at some point during the night

<p>Late buildup: dissipation of clouds or suddenly weakend winds at some point during the night</p>
44
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Early breakup: Frontal passages, Föhn onsets

<p>Early breakup: Frontal passages, Föhn onsets</p>
45
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Mixing event: Strong and gusty windsat the top of the cold air pool

<p>Mixing event: Strong and gusty windsat the top of the cold air pool</p>
46
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Upper disturbance: Similar to mixing but cold air pools remains stably stratified

<p>Upper disturbance: Similar to mixing but cold air pools remains stably stratified</p>
47
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Lower disturbance: Possibly intrusions of relatively warm air into part of the basin (horizontal, not vertical heterogeneity)

<p>Lower disturbance: Possibly intrusions of relatively warm air into part of the basin (horizontal, not vertical heterogeneity)</p>
48
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Layered erosion: Increasing winds with shift in direction (turbulent erosion on top, lateral advection below)

<p>Layered erosion: Increasing winds with shift in direction (turbulent erosion on top, lateral advection below)</p>
49
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<p>What is happening here to the cold air pool?</p>

What is happening here to the cold air pool?

Cold air pool window: Cloud gap or short wind calm, similar to late buildup case, but favourable conditions do not persist

<p>Cold air pool window: Cloud gap or short wind calm, similar to late buildup case, but favourable conditions do not persist</p>
50
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What are some favourable conditions for persistant cold air pools?

clear sky, weak wind, etc…

synoptic scale subsidence

persistent low level cloudiness

51
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What is the main cause for nocturnal low level jets?

caused by decoupling of the geostrophic wind from surface friction which is a consequence of formation of a stable BL at night, which implies the cessation of deep vertical mixing

decoupling breaks original balance between pressure gradient force, Coriolis force and friction → leading to inertial oscillations

Their maximum is seen as nocturnal LLJ just above the SBL