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2/ 47
Introduction Winds Air mass Fronts
ENV 111: Introduction to Meteorology
Lecture 4
Winds, air masses and fronts
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2/ 47
Introduction Winds Air mass Fronts
Presentation outline
1 Introduction
2 Winds in the atmosphere
How does air move?
Large scale winds
Local wind systems
3 Air masses
4 Frontal systems
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Introduction Winds Air mass Fronts
Introduction
Figure 2 : Winds and its effects
We all experience winds blowing
Sometimes, like a pool of cool air,
making us shiver
In other circumstances, air with
different properties meet and cause
certain weather conditions
Is this usual for the atmosphere?
Wind is an exhibition that air
moves, and cause other weather
phenomena
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4/ 47
Introduction Winds Air mass Fronts
Winds in the atmosphere
Figure 3 : Sea breeze
Wind is simply air in motion. The
atmosphere creates kinetic energy
(wind) from heat energy
Energy source is the temperature
differences between:
⇒ the poles and the equator
⇒ the upper and the lower atmosphere
Air is set into motion by pressure
imbalance due to temperature
difference
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5/ 47
Introduction Winds Air mass Fronts
Winds
Figure 4 : Daily variation of pressure
Pressure exhibits daily
fluctuations;
The largest difference
occurs near equator
Mainly due to the
absorption of solar
energy by:
⇒ ozone in the upper
atmosphere
⇒ water vapour in the
lower atmosphere
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6/ 47
Introduction Winds Air mass Fronts
Forces that influence winds
Figure 5 : A balance
between pressure force
and gravity
The motion created is modified by friction, the
Earth’s rotation, and gravity (in the vertical
direction)
So, pressure distribution (see illustration) is the
primary factor for wind formation
Since P1 < P2, pressure (gradient) force is
directed upward and balances with the gravity
force, g which is directed downward
The air is then in hydrostatic equilibrium
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7/ 47
Introduction Winds Air mass Fronts
Forces . . .
With no balance, vertical accelerations occur and convective currents
are created
However, mean vertical velocity over large areas are negligibly small
Since pressure varies also in horizontal, the difference in pressure will
tend to drive the cube horizontally in the direction from high to low
pressure
As no component of gravity in horizontal, the created horizontal
pressure force maintains the motion
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8/ 47
Introduction Winds Air mass Fronts
Forces . . .
So the large wind systems are mainly horizontal currents
Mathematically, pressure gradient force (PGF) is given as:
PGF = ∆ p/(ρ∆z)
Winds blow due to pressure gradient force, but modified by the effects
of the Earth’s rotation and friction
The Earth’s rotation causes a deflecting force (Coriolis force), acts
everywhere at right angles to the path and to the right of the
direction of the motion.
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9/ 47
Introduction Winds Air mass Fronts
Forces . . .
Figure 6 : A balance
between pressure and
Coriolis forces
This force varies with wind speed, latitude
(φ) and equals to:
FCo = 2V ωsinφ
The force is maximum at the pole and
decreases to zero at the equator
If a unit of air moves under the influence of
the pressure force and the deflecting force;
its motion eventually becomes parallel to
the isobars
Such motion is steady; not accelerating,
called geostrophic wind
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10/ 47
Introduction Winds Air mass Fronts
Forces . . .
Figure 7 : Geostrophic wind flow
The geostrophic wind blows along the
isobars with high pressure to the right and
low pressure to the left of the direction of
the motion
The wind has neither divergence nor
convergence
It blows between the isobars in the same
manner as the water streams in a river i.e.
the narrower the cross section of the river,
the faster is the flow
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Introduction Winds Air mass Fronts
Forces . . .
Figure 8 : Actual wind
drifts across isobars due
to frictional force, F
However, in practice, a slight drift across
the isobars that is actually observed in
nature, occurs. It means another force
(friction) affects wind
Under the influence of friction (see
illustration), pressure force (G) balances the
resultant force (R) of the deflecting force
(D) and friction force (F)
Since the pressure force is perpendicular to
the isobars, the wind (V) must blow to the
left of the isobars
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12/ 47
Introduction Winds Air mass Fronts
Forces . . .
The angle between the isobar and the wind direction increases with
increasing friction; it is greater over land than at sea. Its range is
25 − 35◦
under normal conditions
Actual wind near the Earth’s surface deviates to the left of the
direction of the geostrophic wind
Wind velocity increases with height as the frictional force decreases.
So the wind direction also change to be more parallel to the isobars
The influence of friction is palpable up to a height of 1 km; the layer is
called the friction layer (planetary boundary layer)
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13/ 47
Introduction Winds Air mass Fronts
Global wind systems
Figure 9 : Atmospheric general circulation
depicting the global wind systems
The wind velocity continues to
increase in the free atmosphere since
pressure force varies with elevation
The maximum value is at the
tropopause and then the velocity
decreases
The atmospheric general circulation
is thus an idealized diagram of
pressure distribution and prevailing
global winds
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14/ 47
Introduction Winds Air mass Fronts
Global winds . . .
Around the equator, the winds are light and variable; the belt is
called the doldrums
The belts of high pressure (subtropical anticyclones) separates the
easterly winds (trade winds) on their equatorial sides and westerly
winds on their poleward sides
The trade winds converge at the doldrums bringing there frequent
showers, thunderstorms, and heavy rainfall
The anticyclones are characterized by divergence and subsiding air
currents, low relative humidity, almost clear sky, and less rainfall
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15/ 47
Introduction Winds Air mass Fronts
Global winds . . .
They move slightly poleward in summer and toward the equator in
winter
The belts of high pressure are referred to as horse latitudes by sailors
The westerlies increase in strength as the latitude increases and are
bounded on their poleward sides by a subpolar low
The energy imbalance that exists between high and low latitudes
cause air to move fast in a narrow channel, called a Jet stream
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16/ 47
Introduction Winds Air mass Fronts
Global wind systems: Jet streams
Figure 10 : Main jetstreams
They occur due to horizontal
variations in temperature and
pressure
The main jet streams at a global
scale are:
⇒ Polar Front Jet
⇒ Subtropical Jet
⇒ Tropical easterly jet
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17/ 47
Introduction Winds Air mass Fronts
Upper winds: Classification
Figure 11 : Upper wind flows
Upper winds exhibit various flows:
⇒ Geostrophic, where it blows in a
straight path parallel to evenly
spaced lines
⇒ Gradient, where it blows parallel to
curved contour lines
⇒ Meridional, where it flows in large,
looping meanders in a north-south
trajectory
⇒ Zonal, where it blows in a
west-to-east direction
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18/ 47
Introduction Winds Air mass Fronts
Local wind systems
Figure 12 : Scales of motion
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19/ 47
Introduction Winds Air mass Fronts
Local wind systems
Figure 13 : Clouds developing at Lukobe hill in Morogoro
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20/ 47
Introduction Winds Air mass Fronts
Sea and land breezes
Local wind systems form due to thermal circulation caused by heating
and cooling of the atmosphere near the ground
Such thermal pressure systems are:
⇒ shallow,
⇒ weakens with height,
⇒ but are mainly maintained by local surface heating and cooling
Examples:
⇒ sea and land breezes
⇒ mountain and valley breezes
⇒ katabatic wind
⇒ chinook (Foen) wind
⇒ dust devils or whirlwinds
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21/ 47
Introduction Winds Air mass Fronts
Sea and land breezes
Figure 14 : Sea and land breezes
The sea and land breezes are
mesoscale coastal winds system
It is caused by uneven heating rates
of land and water
During the day, intensive heating of
the air above land produces a
shallow thermal low
Whereas a shallow thermal high
exists above the water
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22/ 47
Introduction Winds Air mass Fronts
Sea and land breezes
Thus sea breeze blows at the surface from the sea toward the land
The strongest winds typically occur right near the beach and diminish
inland
Sea breezes are strongest in the afternoon due greatest contrast in
temperature between land and water
At night the system reverses by surface breeze blowing from the land
toward the water hence a land breeze
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23/ 47
Introduction Winds Air mass Fronts
Mountain and valley breezes
Figure 15 : Mountain and valley
breezes
During the day, air in upslope is warmer
than the air of the same altitude above the
valley. It rises as a gentle upslope wind
known as a valley breeze
The flow reverses at night since the
mountain slopes cool quickly, chilling the
air in contact with them.
The cooler, more-dense air glides downslope
into the valley, providing a mountain breeze
(also known as gravity, or nocturnal
drainage winds)
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24/ 47
Introduction Winds Air mass Fronts
Mountain and valley breezes
The upslope winds begin early in the morning, reach a peak speed by
midday, and reverse direction by late evening
While the downslope mountain breeze reaches its peak in the early
morning hours usually before sunrise
A well developed upslope wind with sufficient moisture, reveals itself
by cumulus clouds at summits
Hence cloudiness, showers, and even thunderstorms are common over
mountains during the warmest part of the day
Very strong downslope winds usually on the order of 10 knots or
less.are referred to as katabatic winds
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25/ 47
Introduction Winds Air mass Fronts
Mountain and valley breezes
The ideal setting for a katabatic wind is an elevated plateau
surrounded by mountains, with an opening that slopes rapidly
downhill
Such winds in excess of 100 knots occur:
⇒ Northern Adriatic coast, bora - a cold, gusty;
⇒ Mistral winds into the Rhone Valley of France
⇒ Downslope winds off the ice sheets in Greenland and Antarctica
⇒ Columbia Plateau of Idaho, Oregon, and Washington
Whereas, a warm, dry, downslope wind that descends the eastern
slope of the Rocky Mountains is specifically termed as chinook
(Foehn) winds
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26/ 47
Introduction Winds Air mass Fronts
Mountain and valley breezes
Foehn winds are characterized by sharp temperature rise, sometimes
20◦
C per hour, and a corresponding sharp drop in the relative
humidity
Chinook winds are warm due to compressional heating as the air
descends is compressed and warms at the dry adiabatic rate (10 ◦
/km)
Clouds and precipitation on the mountain’s windward side enhance
the chinook
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27/ 47
Introduction Winds Air mass Fronts
Mountain and valley breezes
Figure 16 : Chinook winds
St. Ana wind is a warm, dry
wind blowing downhill from the
east or northeast into southern
California
In desert areas, huge dust
storms (textitdesrt winds) form,
where strong winds are able to
lift and fill the air with particles
of fine dust
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28/ 47
Introduction Winds Air mass Fronts
Mountain and valley breezes
Figure 17 : Dust devils or whirlwinds
Whereas, dust devils or whirlwinds
are rotating vortices on a small scale
area that form on clear, hot days
over a dry surface
The spin of a dust devil around its
central core is either cyclonic or
anticyclonic, depending on the
nature of the topographic feature
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29/ 47
Introduction Winds Air mass Fronts
Monsoon winds
Figure 18 : Monsoon winds
Monsoon winds are examples of thermal
circulations that are much larger than those
of the more local sea and land breezes.
Monsoon is a seasonally changing wind
system
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30/ 47
Introduction Winds Air mass Fronts
Wind measurements
Figure 19 : A sonic anemometer
Wind is measured in terms of
direction and speed. Wind direction
is measured by using a wind vane
Anemometer is used to measure
wind speed. The oldest type of
anemometer is the pressure plate
anemometer developed by Robert
Hooke in 1667
Sonic anemometer is the modern
and most accurate instrument to
determine wind speed and direction
ndettoel@2016 ENV 111: Introduction to Meteorology

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Winds, air masses and fronts

  • 1. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2/ 47 Introduction Winds Air mass Fronts ENV 111: Introduction to Meteorology Lecture 4 Winds, air masses and fronts ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 2/ 47 Introduction Winds Air mass Fronts Presentation outline 1 Introduction 2 Winds in the atmosphere How does air move? Large scale winds Local wind systems 3 Air masses 4 Frontal systems ndettoel@2016 ENV 111: Introduction to Meteorology
  • 2. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 3/ 47 Introduction Winds Air mass Fronts Introduction Figure 2 : Winds and its effects We all experience winds blowing Sometimes, like a pool of cool air, making us shiver In other circumstances, air with different properties meet and cause certain weather conditions Is this usual for the atmosphere? Wind is an exhibition that air moves, and cause other weather phenomena ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 4/ 47 Introduction Winds Air mass Fronts Winds in the atmosphere Figure 3 : Sea breeze Wind is simply air in motion. The atmosphere creates kinetic energy (wind) from heat energy Energy source is the temperature differences between: ⇒ the poles and the equator ⇒ the upper and the lower atmosphere Air is set into motion by pressure imbalance due to temperature difference ndettoel@2016 ENV 111: Introduction to Meteorology
  • 3. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5/ 47 Introduction Winds Air mass Fronts Winds Figure 4 : Daily variation of pressure Pressure exhibits daily fluctuations; The largest difference occurs near equator Mainly due to the absorption of solar energy by: ⇒ ozone in the upper atmosphere ⇒ water vapour in the lower atmosphere ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 6/ 47 Introduction Winds Air mass Fronts Forces that influence winds Figure 5 : A balance between pressure force and gravity The motion created is modified by friction, the Earth’s rotation, and gravity (in the vertical direction) So, pressure distribution (see illustration) is the primary factor for wind formation Since P1 < P2, pressure (gradient) force is directed upward and balances with the gravity force, g which is directed downward The air is then in hydrostatic equilibrium ndettoel@2016 ENV 111: Introduction to Meteorology
  • 4. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7/ 47 Introduction Winds Air mass Fronts Forces . . . With no balance, vertical accelerations occur and convective currents are created However, mean vertical velocity over large areas are negligibly small Since pressure varies also in horizontal, the difference in pressure will tend to drive the cube horizontally in the direction from high to low pressure As no component of gravity in horizontal, the created horizontal pressure force maintains the motion ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8/ 47 Introduction Winds Air mass Fronts Forces . . . So the large wind systems are mainly horizontal currents Mathematically, pressure gradient force (PGF) is given as: PGF = ∆ p/(ρ∆z) Winds blow due to pressure gradient force, but modified by the effects of the Earth’s rotation and friction The Earth’s rotation causes a deflecting force (Coriolis force), acts everywhere at right angles to the path and to the right of the direction of the motion. ndettoel@2016 ENV 111: Introduction to Meteorology
  • 5. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9/ 47 Introduction Winds Air mass Fronts Forces . . . Figure 6 : A balance between pressure and Coriolis forces This force varies with wind speed, latitude (φ) and equals to: FCo = 2V ωsinφ The force is maximum at the pole and decreases to zero at the equator If a unit of air moves under the influence of the pressure force and the deflecting force; its motion eventually becomes parallel to the isobars Such motion is steady; not accelerating, called geostrophic wind ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10/ 47 Introduction Winds Air mass Fronts Forces . . . Figure 7 : Geostrophic wind flow The geostrophic wind blows along the isobars with high pressure to the right and low pressure to the left of the direction of the motion The wind has neither divergence nor convergence It blows between the isobars in the same manner as the water streams in a river i.e. the narrower the cross section of the river, the faster is the flow ndettoel@2016 ENV 111: Introduction to Meteorology
  • 6. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11/ 47 Introduction Winds Air mass Fronts Forces . . . Figure 8 : Actual wind drifts across isobars due to frictional force, F However, in practice, a slight drift across the isobars that is actually observed in nature, occurs. It means another force (friction) affects wind Under the influence of friction (see illustration), pressure force (G) balances the resultant force (R) of the deflecting force (D) and friction force (F) Since the pressure force is perpendicular to the isobars, the wind (V) must blow to the left of the isobars ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12/ 47 Introduction Winds Air mass Fronts Forces . . . The angle between the isobar and the wind direction increases with increasing friction; it is greater over land than at sea. Its range is 25 − 35◦ under normal conditions Actual wind near the Earth’s surface deviates to the left of the direction of the geostrophic wind Wind velocity increases with height as the frictional force decreases. So the wind direction also change to be more parallel to the isobars The influence of friction is palpable up to a height of 1 km; the layer is called the friction layer (planetary boundary layer) ndettoel@2016 ENV 111: Introduction to Meteorology
  • 7. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13/ 47 Introduction Winds Air mass Fronts Global wind systems Figure 9 : Atmospheric general circulation depicting the global wind systems The wind velocity continues to increase in the free atmosphere since pressure force varies with elevation The maximum value is at the tropopause and then the velocity decreases The atmospheric general circulation is thus an idealized diagram of pressure distribution and prevailing global winds ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 14/ 47 Introduction Winds Air mass Fronts Global winds . . . Around the equator, the winds are light and variable; the belt is called the doldrums The belts of high pressure (subtropical anticyclones) separates the easterly winds (trade winds) on their equatorial sides and westerly winds on their poleward sides The trade winds converge at the doldrums bringing there frequent showers, thunderstorms, and heavy rainfall The anticyclones are characterized by divergence and subsiding air currents, low relative humidity, almost clear sky, and less rainfall ndettoel@2016 ENV 111: Introduction to Meteorology
  • 8. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15/ 47 Introduction Winds Air mass Fronts Global winds . . . They move slightly poleward in summer and toward the equator in winter The belts of high pressure are referred to as horse latitudes by sailors The westerlies increase in strength as the latitude increases and are bounded on their poleward sides by a subpolar low The energy imbalance that exists between high and low latitudes cause air to move fast in a narrow channel, called a Jet stream ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 16/ 47 Introduction Winds Air mass Fronts Global wind systems: Jet streams Figure 10 : Main jetstreams They occur due to horizontal variations in temperature and pressure The main jet streams at a global scale are: ⇒ Polar Front Jet ⇒ Subtropical Jet ⇒ Tropical easterly jet ndettoel@2016 ENV 111: Introduction to Meteorology
  • 9. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17/ 47 Introduction Winds Air mass Fronts Upper winds: Classification Figure 11 : Upper wind flows Upper winds exhibit various flows: ⇒ Geostrophic, where it blows in a straight path parallel to evenly spaced lines ⇒ Gradient, where it blows parallel to curved contour lines ⇒ Meridional, where it flows in large, looping meanders in a north-south trajectory ⇒ Zonal, where it blows in a west-to-east direction ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18/ 47 Introduction Winds Air mass Fronts Local wind systems Figure 12 : Scales of motion ndettoel@2016 ENV 111: Introduction to Meteorology
  • 10. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19/ 47 Introduction Winds Air mass Fronts Local wind systems Figure 13 : Clouds developing at Lukobe hill in Morogoro ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 20/ 47 Introduction Winds Air mass Fronts Sea and land breezes Local wind systems form due to thermal circulation caused by heating and cooling of the atmosphere near the ground Such thermal pressure systems are: ⇒ shallow, ⇒ weakens with height, ⇒ but are mainly maintained by local surface heating and cooling Examples: ⇒ sea and land breezes ⇒ mountain and valley breezes ⇒ katabatic wind ⇒ chinook (Foen) wind ⇒ dust devils or whirlwinds ndettoel@2016 ENV 111: Introduction to Meteorology
  • 11. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21/ 47 Introduction Winds Air mass Fronts Sea and land breezes Figure 14 : Sea and land breezes The sea and land breezes are mesoscale coastal winds system It is caused by uneven heating rates of land and water During the day, intensive heating of the air above land produces a shallow thermal low Whereas a shallow thermal high exists above the water ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 22/ 47 Introduction Winds Air mass Fronts Sea and land breezes Thus sea breeze blows at the surface from the sea toward the land The strongest winds typically occur right near the beach and diminish inland Sea breezes are strongest in the afternoon due greatest contrast in temperature between land and water At night the system reverses by surface breeze blowing from the land toward the water hence a land breeze ndettoel@2016 ENV 111: Introduction to Meteorology
  • 12. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 23/ 47 Introduction Winds Air mass Fronts Mountain and valley breezes Figure 15 : Mountain and valley breezes During the day, air in upslope is warmer than the air of the same altitude above the valley. It rises as a gentle upslope wind known as a valley breeze The flow reverses at night since the mountain slopes cool quickly, chilling the air in contact with them. The cooler, more-dense air glides downslope into the valley, providing a mountain breeze (also known as gravity, or nocturnal drainage winds) ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 24/ 47 Introduction Winds Air mass Fronts Mountain and valley breezes The upslope winds begin early in the morning, reach a peak speed by midday, and reverse direction by late evening While the downslope mountain breeze reaches its peak in the early morning hours usually before sunrise A well developed upslope wind with sufficient moisture, reveals itself by cumulus clouds at summits Hence cloudiness, showers, and even thunderstorms are common over mountains during the warmest part of the day Very strong downslope winds usually on the order of 10 knots or less.are referred to as katabatic winds ndettoel@2016 ENV 111: Introduction to Meteorology
  • 13. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25/ 47 Introduction Winds Air mass Fronts Mountain and valley breezes The ideal setting for a katabatic wind is an elevated plateau surrounded by mountains, with an opening that slopes rapidly downhill Such winds in excess of 100 knots occur: ⇒ Northern Adriatic coast, bora - a cold, gusty; ⇒ Mistral winds into the Rhone Valley of France ⇒ Downslope winds off the ice sheets in Greenland and Antarctica ⇒ Columbia Plateau of Idaho, Oregon, and Washington Whereas, a warm, dry, downslope wind that descends the eastern slope of the Rocky Mountains is specifically termed as chinook (Foehn) winds ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26/ 47 Introduction Winds Air mass Fronts Mountain and valley breezes Foehn winds are characterized by sharp temperature rise, sometimes 20◦ C per hour, and a corresponding sharp drop in the relative humidity Chinook winds are warm due to compressional heating as the air descends is compressed and warms at the dry adiabatic rate (10 ◦ /km) Clouds and precipitation on the mountain’s windward side enhance the chinook ndettoel@2016 ENV 111: Introduction to Meteorology
  • 14. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27/ 47 Introduction Winds Air mass Fronts Mountain and valley breezes Figure 16 : Chinook winds St. Ana wind is a warm, dry wind blowing downhill from the east or northeast into southern California In desert areas, huge dust storms (textitdesrt winds) form, where strong winds are able to lift and fill the air with particles of fine dust ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28/ 47 Introduction Winds Air mass Fronts Mountain and valley breezes Figure 17 : Dust devils or whirlwinds Whereas, dust devils or whirlwinds are rotating vortices on a small scale area that form on clear, hot days over a dry surface The spin of a dust devil around its central core is either cyclonic or anticyclonic, depending on the nature of the topographic feature ndettoel@2016 ENV 111: Introduction to Meteorology
  • 15. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29/ 47 Introduction Winds Air mass Fronts Monsoon winds Figure 18 : Monsoon winds Monsoon winds are examples of thermal circulations that are much larger than those of the more local sea and land breezes. Monsoon is a seasonally changing wind system ndettoel@2016 ENV 111: Introduction to Meteorology . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30/ 47 Introduction Winds Air mass Fronts Wind measurements Figure 19 : A sonic anemometer Wind is measured in terms of direction and speed. Wind direction is measured by using a wind vane Anemometer is used to measure wind speed. The oldest type of anemometer is the pressure plate anemometer developed by Robert Hooke in 1667 Sonic anemometer is the modern and most accurate instrument to determine wind speed and direction ndettoel@2016 ENV 111: Introduction to Meteorology