Lecture 7-8: Energy balance and temperature (Ch 3) - PowerPoint PPT Presentation

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Lecture 7-8: Energy balance and temperature (Ch 3)

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Title: Lecture 7-8: Energy balance and temperature (Ch 3)


1
Lecture 7-8 Energy balance and temperature (Ch
3)
  • the diurnal cycle in net radiation, temperature
    and stratification
  • the friction layer
  • local microclimates
  • influences on regional temperature patterns

2
The diurnal (daily) cycle in net radiation at the
base of the atmos.
Q K L K? - K? L? - L?
L is typically negative unless there is low
cloud cover
3
Q QH QE QG
Surface energy budget
an arbitrary example of a duirnal cycle
4
Understanding the diurnal (daily) cycle in
temperature (similar principles apply to
understanding the seasonal cycle)
Fig. 3-22a
5
Diurnal cycle in near-ground stratification
Night-time near-ground temperature profile
stable stratification
Daytime near-ground temperature
profile unstable stratification
Inversion downward heat flow, mixing damped
Upward heat flow, vertical mixing enhanced (p65)
z
z
TT(z)
TT(z)
6
The atmospheric boundary layer and the depth (?)
of mixing
  • free atmosphere
  • no friction
  • vertical velocities steady and of order cm s-1
    except
  • in clouds/over mountains

?
  • friction layer or boundary layer
  • friction reduces windspeed
  • variation of wind with height, instability (warm
    air underneath cold), and flow around obstacles
  • produce turbulence
  • vertical velocities fluctuate and are of order m
    s-1

z
7
Depth (?) of mixing varies in time/space
  • Depth of the ABL (i.e. magnitude of ?) depends on
    the turbulence, and increases with
  • stronger surface heating QH
  • stronger wind
  • rougher surface

summer
Order 1 km
?
winter
Order 100 m
dawn
dusk
8
Nocturnal Radiation Inversion
  • ground cooling Q lt 0, ie. outgoing longwave
    radiation exceeds incoming longwave
  • then air above cools by convection (stirring),
    QH lt 0

Cause
Conditions for severest inversion
  • clear sky, dry air
  • long night with light wind

Result radiation frost?
Photo Keith Cooley
9
Figs. 3-21
Complexity of local (site-specific) effects on
local radiation and energy balance producing
micro-climates that can be manipulated (eg.
windbreaks)
10
Latitudinal variation in net allwave radiation
a S0L?
Averaged over a long period, latitudinal heat
advection by ocean (25) and atmosphere (75)
rectifies the imbalance
Fig. 3-15
( 1-a ) S0 , a the albedo
11
Why do we consider earths global climatological
temperature Teq to be at equilibrium (Sec. 3-2)?
Because there is a stabilizing feedback...
Let DTeq be the change in Teq over time interval
Dt. Then
area of earths surface
area of earths shadow
Rate of change ? gains
- losses
Where R is earths radius, S0 is the solar
constant, a (0.3) is the planetary albeto, ?
(?1) is the planetary emissivity and ? is the
Stefan-Boltzmann constant. The proportionality
constant involves the heat capacity of the
earth-atmosphere system. (In reality a,? may
depend on Teq ).
12
At earths equilibrium temperature, there is
balance...
Common factor cancels
Set a 0.3 and ? 1 to obtain earths
(radiative) equilibrium temperature (Sec. 3-2).
13
Factors controlling temperature on regional
global time space scales
  • Latitude
  • solar radiation
  • distribution of land water
  • surface thermal inertia, surface energy balance
  • topographic steering/blockage of winds
  • Ocean Currents
  • advective domination (horizontal heat transport)
  • Elevation

14
  • latitudinal temperature gradient is greatest in
    the winter hemisphere
  • in summer (winter) temperature over land warmer
    (cooler) than over ocean

Fig. 3-18a
15
Why are water bodies more conservative in their
temperature?
  • solar radiation penetrates to some depth so
    warms a volume
  • much of the available radiant energy used to
    evaporate water
  • mixing of the water in the ocean/lake mixed
    layer ensures heat deposited/drawn from a deep
    layer
  • water has a much higher specific heat (4128 J
    kg-1 K-1) than land
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