SlideShare uma empresa Scribd logo
1 de 90
6-1-S290-EPUnit 6 Atmospheric Stability
Unit 6
Atmospheric Stability
6-2-S290-EPUnit 6 Atmospheric Stability
Unit 6 Objectives
2. Describe temperature lapse rate and stability, and
the different temperature lapse rates used to
determine the stability of the atmosphere.
4. Name four types of temperature inversions and
describe their influence on wildland fire behavior,
including the thermal belt.
3. Describe the effects of atmospheric stability on
wildland fire behavior.
1. Describe the relationship among atmospheric
pressure, temperature, density and volume.
6-3-S290-EPUnit 6 Atmospheric Stability
5. Name and describe the four lifting processes that
can produce thunderstorms.
6. Describe the elements of a thunderstorm and its
three stages of development.
7. Use visual indicators to describe the stability
of the atmosphere.
8. Describe the four principle cloud groups, and
identify the six clouds most often associated with
critical wildland fire behavior.
Unit 6 Objectives
6-4-S290-EPUnit 6 Atmospheric Stability
Up to now, our attention has been on
temperature and the factors that influence its
change on and near the earth’s surface.
In this unit we will focus on air temperature in
the third dimension, atmospheric stability, and
how stability affects wildland fire behavior.
We will also discuss several visual indicators
commonly used to identify critical changes in
atmospheric stability.
6-5-S290-EPUnit 6 Atmospheric Stability
Our atmosphere is composed of
numerous gases.
This gaseous mixture includes
permanent dry air gases
such as nitrogen, oxygen, argon,
helium, hydrogen, and xenon.
Nitrogen and oxygen account for 99%
of all permanent dry air gases
in the troposphere.
6-6-S290-EPUnit 6 Atmospheric Stability
The remaining gases, called
variable gases;
include water vapor, carbon dioxide,
methane, nitrous oxide and ozone.
Of these gases,
water vapor is the most abundant,
varying from a trace to 4 percent by volume.
6-7-S290-EPUnit 6 Atmospheric Stability
Nearly all gases in the atmosphere
respond uniformly to changes in
temperature and pressure.
Behavior of Gases
For that reason, we can use the
Ideal Gas Law (Equation of State)
which is based on a set of gas behavior laws,
to describe their behavior.
6-8-S290-EPUnit 6 Atmospheric Stability
The relationship among pressure,
temperature and density (mass per volume)
can be expressed by the gas law equation
where: P is pressure, ρ is density, m is the
mass of the gas, V is volume, R is a gas
constant, and T is temperature.
P = (ρ)RT or P = (m/V)RT
6-9-S290-EPUnit 6 Atmospheric Stability
R is the gas constant, and can be ignored.
~ is the symbol meaning “is proportional to.”
Again: The term (m/V) represents the
density (ρ) of the gas.
P ~ (ρ)T or P ~ (m/V)T
6-10-S290-EPUnit 6 Atmospheric Stability
Often when
referring to air in
motion, we
represent it in
small units or
volumes called
air parcels.
6-11-S290-EPUnit 6 Atmospheric Stability
An air parcel is a volume
of air, large enough to
contain a great number of
molecules, but small
enough so that its energy
(heat) and mass (air
molecules) are nearly
uniform within is
boundaries.
Air Parcel
6-12-S290-EPUnit 6 Atmospheric Stability
Air parcels
expand and contract freely,
but neither heat nor outside air
is able to mix with air inside;
making an air parcel
a sealed container.
Air parcels are commonly
portrayed as 3-dimensional
cubes or spheres.
Air Parcel
6-13-S290-EPUnit 6 Atmospheric Stability
Rising
Air Parcel
As atmospheric pressure decreases
with increasing altitude:
 volume increases
 density decreases
Rising air parcels
always expand and cool
Cooler &
Less dense
 temperature decreases
Applying this Relationship
To a Rising Air Parcel
6-14-S290-EPUnit 6 Atmospheric Stability
Sinking
Air Parcel
As atmospheric pressure increases
with decreasing altitude:
 volume decreases
 temperature increases
Sinking air parcels
always compress and warm
Warmer &
more dense
 density increases
Applying this Relationship
To a Sinking Air Parcel
6-15-S290-EPUnit 6 Atmospheric Stability
When an air parcel
rises or sinks
without any loss of energy or mass
to the surrounding atmosphere
ADIABATIC PROCESS
6-16-S290-EPUnit 6 Atmospheric Stability
EXERCISE 1
6-17-S290-EPUnit 6 Atmospheric Stability
Air in Motion
The rotation of the earth on its axis,
together with large and small scale variations
in pressure and temperature
are what produce the
horizontal and vertical
movement of air in the atmosphere.
6-18-S290-EPUnit 6 Atmospheric Stability 06-18-S290-EP
Wind and Stability
6-18-S290-EP
6-19-S290-EPUnit 6 Atmospheric Stability
The magnitude or strength of wind is
far greater than the vertical movement of air
associated with atmospheric stability.
However, their influence on the behavior of
wildland fires is equally important.
In this unit, our attention will be on
vertically moving air associated with
atmospheric stability.
6-20-S290-EPUnit 6 Atmospheric Stability
What is Stability?
It is the resistance of the atmosphere
to vertical motion.
More precisely, it is the degree to
which vertical motion in the atmosphere is
enhanced or suppressed.
Depending on the vertical temperature profile
of the atmosphere, air will either rise,
sink or remain at rest.
6-21-S290-EPUnit 6 Atmospheric Stability
Stable Atmosphere
Suppresses or resists vertical movement of air
Unstable Atmosphere
Enhances or encourages vertical movement of air
Three Types of Stability
Neutral Atmosphere
Neither suppresses nor enhances vertical
movement of air. This condition seldom exists for
long periods of time.
6-22-S290-EPUnit 6 Atmospheric Stability
Unstable Atmosphere
Air parcels
will continue
to rise
Level of
Origin
6-23-S290-EPUnit 6 Atmospheric Stability
Rising
Air
Unstable Atmosphere
Promotes the formation
and growth of
vertically developed
clouds, thunderstorms
and tall smoke columns
6-24-S290-EPUnit 6 Atmospheric Stability
Stable Atmosphere
Air parcels displaced upward (downward) will
eventually return to their level of origin.
Level of
Origin
6-25-S290-EPUnit 6 Atmospheric Stability
Stable Atmosphere
Light winds and poor
smoke dispersal from
poor vertical mixing
trapped smoke
and haze
6-26-S290-EPUnit 6 Atmospheric Stability
In mountainous
terrain, however,
stable conditions
can produce gusty
ridgetop winds, and
warm, dry and gusty
downslope winds
called foehn winds.
mountain wave
clouds
windward
slope
leeward
slope foehn
wind
6-27-S290-EPUnit 6 Atmospheric Stability
Neutral Stability
• Usually exists for only short periods of
time during the transition between a
stable and an unstable atmosphere.
• Little vertical air motion occurs.
• If this condition should exist through a
deep layer of atmosphere, an air
parcel’s vertical motion will cease.
6-28-S290-EPUnit 6 Atmospheric Stability
An unstable
atmosphere
is most often
associated with
critical or extreme
wildland fire
behavior.
6-29-S290-EPUnit 6 Atmospheric Stability
A stable
atmosphere
will tend to
suppress or
reduce
wildland fire
behavior.
6-30-S290-EPUnit 6 Atmospheric Stability
Neutral atmospheric conditions
have little if any effect on
wildland fire behavior.
6-31-S290-EPUnit 6 Atmospheric Stability
Four Ways
To Change
Atmospheric
Stability
Heating from
below
Warming aloft
Cooling from
below
Cooling aloft
6-32-S290-EPUnit 6 Atmospheric Stability
Temperature Lapse Rate
The change in temperature with
a change in altitude.
Change in Temperature
Change in Altitude
6-33-S290-EPUnit 6 Atmospheric Stability
Temperature Lapse Rates
differ throughout the troposphere,
particularly in the lowest 3000 feet
above the ground
where air temperature is
strongly influenced by:
• daytime solar heating
• nighttime radiational cooling
6-34-S290-EPUnit 6 Atmospheric Stability
This lowest layer of
the troposphere is
called the
boundary layer.Boundary
Layer
We will often refer to
the boundary layer
near the ground.
6-35-S290-EPUnit 6 Atmospheric Stability
+15ºF per 1000 feet,
within a 24 hour period
Lapse Rates within the
Boundary Layer
6-36-S290-EPUnit 6 Atmospheric Stability
Recall
from Unit 4
that temperature
normally decreases
with increasing
altitude in the
troposphere.
cooling
6-37-S290-EPUnit 6 Atmospheric Stability
Air temperature can also increase
with increasing altitude in the troposphere.
This reversal in the normal trend in
temperature reduction with
altitude is what we refer to as an
inversion.
(More on inversions later)
6-38-S290-EPUnit 6 Atmospheric Stability
Positive
Lapse Rate
Warming with
Increasing
Altitude
Negative
Lapse Rate
Cooling with
Increasing
Altitude
6-39-S290-EPUnit 6 Atmospheric Stability
Weather observing
balloons called
radiosondes, and
other observing systems,
including weather satellites
and aircraft, are routinely
used to record changes in
air temperature aloft.
Determining the
Lapse Rate
6-40-S290-EPUnit 6 Atmospheric Stability
Three Lapse Rates You Need to Know
• Dry Adiabatic Lapse Rate
• Moist Adiabatic Lapse Rate
• Average Lapse Rate
6-41-S290-EPUnit 6 Atmospheric Stability
Represents the rate of
change in temperature of
rising and sinking
unsaturated air.
Dry Adiabatic Lapse Rate
Rising “dry” air will
always cool at a rate of
-5.5º F per 1000 feet.
Sinking “dry” air will
always warm at a rate of
+5.5º F per 1000 feet.
6-42-S290-EPUnit 6 Atmospheric Stability
Moist Adiabatic Lapse Rate
Rising saturated air
cools at a rate of
approximately
-3.0ºF per 1000 feet.
Represents the rate of
change in temperature
of rising and sinking
saturated air.
6-43-S290-EPUnit 6 Atmospheric Stability
Heat released during
condensation offsets the cooling
that occurs due to expansion.
Heat released during
condensation offsets the cooling
that occurs due to expansion.
Rising saturated air parcels also
lose mass, in the form of cloud
droplets and precipitation.
Rising saturated air parcels also
lose mass, in the form of cloud
droplets and precipitation.
During the
Moist Adiabatic Process
During the
Moist Adiabatic Process
saturated
parcel
Not a true adiabatic processNot a true adiabatic process
6-43-S290-EP
6-44-S290-EPUnit 6 Atmospheric Stability
Sinking air parcels rarely warm at the moist lapse rate.
Once saturated air begins to sink, for
example down the lee slope of a mountain
range, compression causes it to warm.
Once this air becomes
unsaturated, or its relative
humidity lowers below 100
percent, this sinking air will
warm at the faster dry
adiabatic lapse rate of
+5.5ºF per 1000 feet.
6-44-S290-EP
6-45-S290-EPUnit 6 Atmospheric Stability
The skew-T diagram is used to represent the pressure,
temperature, density, moisture, wind and atmospheric
stability within a column of atmosphere above a point on
the earth’s surface. 6-45-S290-EP
6-46-S290-EPUnit 6 Atmospheric Stability
Average Lapse Rate: +/- 3.5ºF per 1000 feet
Represents
average vertical
temperature change
for the entire
troposphere.
Can NOT be used
to determine the
stability of the
atmosphere.
6-47-S290-EPUnit 6 Atmospheric Stability
Because of variations in
topography, vegetation, wind, cloud cover, etc.
avoid using a lapse rate to
project temperatures more than 2000 feet above or
below your location.
Average lapse rate is useful
for estimating temperature and RH
for a shallow layer in the atmosphere
or for a point on a mountain side.
6-48-S290-EPUnit 6 Atmospheric Stability
Example Using the Average Lapse Rate
4500 ft.
94ºF
6500 ft.
87ºF
-3.5ºF/1000 ft
Knowing your temperature at
an elevation 4500 feet, project
the temperature on a fireline at
6500 feet using the average
lapse rate.
Elevation Change: 2000 feet
Lapse rate: -3.5ºF/1000 feet
Temp. at 6500 feet: 87ºF
Temp. Change: (2 x -3.5ºF)
Average Lapse Rate
6-49-S290-EPUnit 6 Atmospheric Stability
0 ft AGL0 ft AGL
5,000 ft AGL5,000 ft AGL
13,000 ft AGL13,000 ft AGL
80.080.0ºº FF
52.552.5ºº FF
8.58.5ºº FF
A Day in the Life of aA Day in the Life of a
Rising Air ParcelRising Air Parcel
If the parcel becomes saturated during
its ascent, at 5,000 feet for instance, a
cloud forms; assuming the parcel
remains saturated as it continues to
rise.
74.074.0ºº FF
49.049.0ºº FF
8.08.0ºº FF
bare field Fields covered with vegetation 6-49-S290-EP
6-50-S290-EPUnit 6 Atmospheric Stability 06-50-S290-EP
90ºF90ºF 82ºF82ºF80ºF80ºF
The greater the
temperature difference
between
an air parcel and the
surrounding air, the
faster the parcel will rise
or sink. This difference in
temperature is an
indicator of how unstable
or stable a layer of
atmosphere is.
The greater the
temperature difference
between
an air parcel and the
surrounding air, the
faster the parcel will rise
or sink. This difference in
temperature is an
indicator of how unstable
or stable a layer of
atmosphere is.
Fast
Slow
air temp.
How Fast Will Air Rise?How Fast Will Air Rise?
6-50-S290-EP
6-51-S290-EPUnit 6 Atmospheric Stability
Large wildfires can
produce strong
convective
updrafts capable
of lifting debris as
large as small trees
hundreds of feet
into the air.
Strong
Updraft
6-52-S290-EPUnit 6 Atmospheric Stability
Influence of Moisture on Atmospheric Stability
Dry air is generally more STABLE than UNSTABLE
because it is “heavier.”
6-53-S290-EPUnit 6 Atmospheric Stability 06-53-S290-EP
Use the appropriate lapse rates to calculate the temperatureUse the appropriate lapse rates to calculate the temperature
of this moving air parcel at the designated altitudes.of this moving air parcel at the designated altitudes.
80F80F
??
??
??
??
63.5F
48.5F
76.0F
92.5F
Exercise 2
UNSTABLE STABLE
6-53-S290-EP
6-54-S290-EPUnit 6 Atmospheric Stability
EXERCISE 3
Lapse Rates and
Atmospheric Stability
6-55-S290-EPUnit 6 Atmospheric Stability
The Mixing Layer
Top of the
Mixing
Layer
Earth’s Surface
The lowest layer of the
troposphere where surface
heating mixes and
vertically transports air
molecules, water vapor
and pollutants, such as
smoke,
potentially to thousands
of feet above the ground.
Over United States varies
from about
1/2 to 3 1/2 miles thick
6-55-S290-EP
6-56-S290-EPUnit 6 Atmospheric Stability 06-56-S290-EP
Deepest over
the Interior of
Continents
Shallowest over
Oceans and
Coastal Regions
Shallowest over
Oceans and
Coastal Regions
Generally deepest or highest over the interior regions ofover the interior regions of
continents and tropical regions, and is shallowest orcontinents and tropical regions, and is shallowest or
lowest over the oceans, coasts and polar regionslowest over the oceans, coasts and polar regions
Generally deepest or highest over the interior regions ofover the interior regions of
continents and tropical regions, and is shallowest orcontinents and tropical regions, and is shallowest or
lowest over the oceans, coasts and polar regionslowest over the oceans, coasts and polar regions
The Mixing Layer or Convective Mixing Layer
6-56-S290-EP
6-57-S290-EPUnit 6 Atmospheric Stability
Top of the Mixing Layer
Top of the Mixing Layer
The convective mixing layer is normally “capped” by a layer of
very stable air, which limits the rise of vertically developed
clouds and smoke columns. The tops of tall smoke columns
and cumulonimbus clouds are often seen spreading out at the
top of the mixing layer.
6-57-S290-EP
6-58-S290-EPUnit 6 Atmospheric Stability
Evolution of the
Daytime
Mixing Layer
55ºF
58F
63ºF 75ºF 80ºF 88ºF
8 AM
10 AM
Noon
2 PM
8 AM
1500 Ft AGL10 AM
2800 FT AGL
Noon
7400 Ft AGL
2 PM
12,000 Ft AGL
Maximum Mixing Height
G r o u n d
6-58-S290-EP
6-59-S290-EPUnit 6 Atmospheric Stability
Seasonal Variation in the Height of the Mixing Layer
The depth of the mixing layer varies considerably
during the year.
Average depth of the Mixing Layer
The wildfire is at 2,500 feet ASL.
6-60-S290-EPUnit 6 Atmospheric Stability
Effects of Unstable Atmospheric Conditions
on Wildland Fire Behavior
• Increased likelihood of fire whirls and dust devils
• Increased likelihood for gusty and erratic surface
winds
• The height and strength of convection and smoke
columns often increase significantly
• Increased likelihood of fire brands being lifted to
great heights
6-61-S290-EPUnit 6 Atmospheric Stability
Effects of Stable Atmospheric Conditions
on Wildland Fire Behavior
• Limited rise of smoke columns, resulting in
poor smoke dispersion and visibility.
• Reduced inflow of fresh air, thereby limiting
wildland fire growth and intensity.
• Lowers surface wind speeds and fire spread
rates except in mountainous or hilly terrain.
6-62-S290-EPUnit 6 Atmospheric Stability
A combination of:
stability and dryness
Indicates potential for large
plume-dominated fire growth.
Haines Index
6-63-S290-EPUnit 6 Atmospheric Stability
Due to large elevation differences, three atmospheric
layers are used to determine the Haines Index.
Haines Index
Low: 2,000-5,000 ft
Mid: 5,000-10,000 ft
High: 10,000-18,000 ft
6-64-S290-EPUnit 6 Atmospheric Stability
Haines Index Numbers
The Potential for Large Plume
Dominated Fire Growth
2 or 3 … Very low potential
4 … Low potential
5 … Moderate potential
6 … High potential
6-65-S290-EPUnit 6 Atmospheric Stability
Haines Index
The drier and more unstable the lower
atmosphere, the HIGHER the Haines Index.
Bottom Line…
The more humid and stable the lower
atmosphere, the LOWER the Haines Index.
6-66-S290-EPUnit 6 Atmospheric Stability
6-67-S290-EPUnit 6 Atmospheric Stability
An inversion is a layer
of very stable air
where temperature
increases with an
increase in altitude.
An inversion acts like
a cap or lid to severely
limit the upward
movement of air.
Inversions often exist
at many levels of the
troposphere.
What is a Temperatures Inversion?
Warmer
6-67-S290-EP
6-68-S290-EPUnit 6 Atmospheric Stability
Four Types of Inversions
6-68-S290-EP
6-69-S290-EPUnit 6 Atmospheric Stability
Nighttime or Radiation Inversion
Sunset Midnight Sunrise
During the evening hours, this surface based inversion is weak and
shallow, usually no more than a few hundred feet deep. As cold air
drainage and radiational cooling continues overnight, this inversion
strengthens and eventually reaches its maximum depth around sunrise
when surface temperatures are at their lowest.
Strong cold
air drainage
Weak cold
air drainage
Little or no
drainage flow
Weak
inversion Moderate
Inversion
Strong
Inversion
6-69-S290-EP
6-70-S290-EPUnit 6 Atmospheric Stability
The depth or strength of the nighttime or
radiation inversion can range from several
hundred feet to several thousand feet
depending on:
cloud cover, wind, precipitation, snow
cover, valley or canyon width and
depth, and time of year
6-71-S290-EPUnit 6 Atmospheric Stability
Weak, Shallow
Nighttime Inversion
Strong, Deep
Nighttime
Inversion
Effects of Cloud Cover and Wind
Surface-based nighttime or radiation inversions
are deepest or strongest on clear nights with
light or no winds; and shallowest or weakest on
cloudy, breezy nights.
Top of the Inversion
Top of the Inversion
6-72-S290-EPUnit 6 Atmospheric Stability
Dissipation of the Nighttime Inversion
Early Morning
Top of Surface Based Inversion
Transport Wind
20-ft wind
Mid-Morning
Transport
Wind
Top of the Inversion Rises as it Weakens
20-ft wind
Late Morning
Transport Wind
Surface Inversion
Has Dissipated
20-foot Wind
When the surface inversion breaks, fire intensity may
suddenly increase with a rush of fresh oxygen.
6-72-S290-EP
6-73-S290-EPUnit 6 Atmospheric Stability
What to Expect When
Nighttime Inversions Break
• Winds often increase suddenly and
possibly become gusty and erratic
• Air temperature increases suddenly
• Relative humidity decreases
suddenly
6-74-S290-EPUnit 6 Atmospheric Stability
There are several aspects of
stable air that should be understood
by the firefighter:
One is the relationship of the
nighttime or radiation inversion
to thermal belts.
6-75-S290-EPUnit 6 Atmospheric Stability
The Thermal Belt
Thermal belts form
where the top of the
nighttime inversion
makes frequent
contact with valley
wall or mountain slope.
Highest temperature
and lowest average
relative humidity
at night.
Nighttime
6-75-S290-EP
6-76-S290-EPUnit 6 Atmospheric Stability
Hazards of the Thermal Belt
Dries out fuels and
can create
severe burning
conditions.
Most importantly:
active burning at night,
while areas above and
below relatively quiet.
Nighttime
6-76-S290-EP
6-77-S290-EPUnit 6 Atmospheric Stability
Elevation and location of the
thermal belt varies by:
• Locality
• Time of year
• Length of nighttime darkness
• Size and steepness of the valley or
canyon
6-78-S290-EPUnit 6 Atmospheric Stability
Summer Nights
Winter Nights
Shallow
Inversions
Deep
Inversions
Higher on winter nights
with stronger radiational
cooling and cold air
drainage. May be
thousands of feet above
the valley floor.
Lower on valley walls
and mountain slopes
during the summer with
shorter nights and less
radiational cooling and
cold air drainage.
6-78-S290-EP
6-79-S290-EPUnit 6 Atmospheric Stability
Thermal belts tend to
form higher on the walls
of broad valleys and
gently slopes canyons.
Lower on mountain
slopes and steep
canyons with strong
drainage.
Broad Valleys
6-79-S290-EP
6-80-S290-EPUnit 6 Atmospheric Stability
Nighttime cloud cover
will limit the depth of
the nighttime or
radiation inversion.
Shallow
Inversion
Deep
Inversion
Clear Nights
Cloudy Nights
Thermal
Belt
Thermal
Belt
Thermal
Belt
Thermal
Belt
6-80-S290-EP
6-81-S290-EPUnit 6 Atmospheric Stability
Frontal Inversion
The frontal inversion is strongest behind the
advancing frontal boundary, as much as a hundred
miles or more.
warmer, lighter air
cooler, heavier air
6-81-S290-EP
6-82-S290-EPUnit 6 Atmospheric Stability 06-82-S290-EP
Marine Inversion
• Commonly found along the shorelines of large lakes
and the West coast of the United States.
• Varies in depth from a few hundred feet to several
thousand, and may extend hundreds of miles inland.
Ocean
Stratus clouds
Similar to frontal inversions,
but often with more moisture
Ocean
6-82-S290-EP
6-83-S290-EPUnit 6 Atmospheric Stability
Warm, drier
air aloft
Inland Extent of Marine Inversions
Cool, moist and stable marine air beneath a layer of
warm, dry and unstable air will frequently move over
the lowlands along the west coast with the diurnal
cycle of winds and temperature.
6-84-S290-EPUnit 6 Atmospheric Stability
Subsidence Inversion
Form when an extensive layer of atmosphere slowly sinks
beneath a large ridge of high pressure.
6-85-S290-EPUnit 6 Atmospheric Stability
Lowering Subsidence
Inversion
Subsidence is a slow process that can
occur over several days.
6-86-S290-EPUnit 6 Atmospheric Stability
The top of mountain
ranges will
experience
the warm, very dry
conditions of the
subsidence
inversion first.
Poor smoke dispersal
conditions may also
develop below a
lowering subsidence
inversion.
Temperature
Sounding
6-87-S290-EPUnit 6 Atmospheric Stability
Subsidence
Inversions
Subsidence
Inversions
Subsidence
Inversions
Strongest in late
summer and
autumn, on the
North and East
sides of strong
high pressure
ridges.
Sometimes
remains over a
region for weeks
at a time.
Aloft
Aloft
6-88-S290-EPUnit 6 Atmospheric Stability
Winds on flat terrain are normally light in speed underneath
large high pressure ridges and subsidence inversions.
In mountain regions, these same atmospheric conditions can
produce warm and dry downslope winds called foehn winds.
light winds light winds
Light winds
HH
gusty
winds
gusty
winds
Foehn Winds
Subsidence and Foehn Winds
6-88-S290-EP
6-89-S290-EPUnit 6 Atmospheric Stability
EXERCISE 4
Stability and Its Effects On
Wildland Fire Behavior
6-90-S290-EPUnit 6 Atmospheric Stability
End of Part I

Mais conteúdo relacionado

Mais procurados

STRUCTURE OF THE ATMOSPHERE
STRUCTURE OF THE ATMOSPHERESTRUCTURE OF THE ATMOSPHERE
STRUCTURE OF THE ATMOSPHERE
GeoCoops
 
Weather And Climate
Weather And ClimateWeather And Climate
Weather And Climate
jdmcd
 
Clouds and percipitation powerpoint
Clouds and percipitation powerpointClouds and percipitation powerpoint
Clouds and percipitation powerpoint
FC Meteorology
 
Ppp on clouds and their classification
Ppp on clouds and their classificationPpp on clouds and their classification
Ppp on clouds and their classification
Fasihud Din Nauman
 
Cloud Types Presentation
Cloud Types PresentationCloud Types Presentation
Cloud Types Presentation
Maribeth Yoder
 
Atmospheric humidity
Atmospheric humidityAtmospheric humidity
Atmospheric humidity
rb roonbat
 
Atmosphere, weather and climate
Atmosphere, weather and climateAtmosphere, weather and climate
Atmosphere, weather and climate
krferraro
 
Presentation El Nino
Presentation  El  NinoPresentation  El  Nino
Presentation El Nino
Matt Beat
 

Mais procurados (20)

Cyclones and western disturbances By Lohit Saini
Cyclones and western disturbances By Lohit SainiCyclones and western disturbances By Lohit Saini
Cyclones and western disturbances By Lohit Saini
 
Clouds
CloudsClouds
Clouds
 
STRUCTURE OF THE ATMOSPHERE
STRUCTURE OF THE ATMOSPHERESTRUCTURE OF THE ATMOSPHERE
STRUCTURE OF THE ATMOSPHERE
 
weather and climate ppt.pptx
weather and climate ppt.pptxweather and climate ppt.pptx
weather and climate ppt.pptx
 
Atmospheric stability and plume behaviour
Atmospheric stability and plume behaviourAtmospheric stability and plume behaviour
Atmospheric stability and plume behaviour
 
Weather And Climate
Weather And ClimateWeather And Climate
Weather And Climate
 
Clouds and precipitation
Clouds and precipitationClouds and precipitation
Clouds and precipitation
 
Clouds and percipitation powerpoint
Clouds and percipitation powerpointClouds and percipitation powerpoint
Clouds and percipitation powerpoint
 
Thunderstorms
ThunderstormsThunderstorms
Thunderstorms
 
Secondary Three Geography: Elements-relative humidity and rain
Secondary Three Geography: Elements-relative humidity and rainSecondary Three Geography: Elements-relative humidity and rain
Secondary Three Geography: Elements-relative humidity and rain
 
Ppp on clouds and their classification
Ppp on clouds and their classificationPpp on clouds and their classification
Ppp on clouds and their classification
 
Cloud Types Presentation
Cloud Types PresentationCloud Types Presentation
Cloud Types Presentation
 
Atmospheric humidity
Atmospheric humidityAtmospheric humidity
Atmospheric humidity
 
Winds and Wind System
Winds and Wind SystemWinds and Wind System
Winds and Wind System
 
Atmosphere, weather and climate
Atmosphere, weather and climateAtmosphere, weather and climate
Atmosphere, weather and climate
 
Chapter 11 Weather and Climate lesson slides published
Chapter 11  Weather and Climate lesson slides publishedChapter 11  Weather and Climate lesson slides published
Chapter 11 Weather and Climate lesson slides published
 
Synoptic Charts
Synoptic ChartsSynoptic Charts
Synoptic Charts
 
Presentation El Nino
Presentation  El  NinoPresentation  El  Nino
Presentation El Nino
 
Lesson 17: Weather and Climate
Lesson 17: Weather and ClimateLesson 17: Weather and Climate
Lesson 17: Weather and Climate
 
AS GEOGRAPHY - ATMOSPHERE AND WEATHER - CLOUD FORMATION
AS GEOGRAPHY - ATMOSPHERE AND WEATHER - CLOUD FORMATIONAS GEOGRAPHY - ATMOSPHERE AND WEATHER - CLOUD FORMATION
AS GEOGRAPHY - ATMOSPHERE AND WEATHER - CLOUD FORMATION
 

Destaque

GEOG100--Lecture 05--Atmos energy, temp, weather
GEOG100--Lecture 05--Atmos energy, temp, weatherGEOG100--Lecture 05--Atmos energy, temp, weather
GEOG100--Lecture 05--Atmos energy, temp, weather
angelaorr
 

Destaque (20)

S290 Unit 5
S290 Unit 5S290 Unit 5
S290 Unit 5
 
S290 Unit 2
S290 Unit 2S290 Unit 2
S290 Unit 2
 
S290 Unit 10
S290 Unit 10S290 Unit 10
S290 Unit 10
 
S290 Unit 12 part 1
S290 Unit 12 part 1S290 Unit 12 part 1
S290 Unit 12 part 1
 
S290 Unit 1
S290 Unit 1S290 Unit 1
S290 Unit 1
 
Air Pollution
Air PollutionAir Pollution
Air Pollution
 
S290 Unit 9
S290 Unit 9S290 Unit 9
S290 Unit 9
 
S290 Unit 12 part 2
S290 Unit 12 part 2S290 Unit 12 part 2
S290 Unit 12 part 2
 
AIR POLLUTION CONTROL L 14
AIR POLLUTION CONTROL L 14AIR POLLUTION CONTROL L 14
AIR POLLUTION CONTROL L 14
 
GEOG100--Lecture 05--Atmos energy, temp, weather
GEOG100--Lecture 05--Atmos energy, temp, weatherGEOG100--Lecture 05--Atmos energy, temp, weather
GEOG100--Lecture 05--Atmos energy, temp, weather
 
AIR POLLUTION CONTROL L 15
AIR POLLUTION CONTROL L 15AIR POLLUTION CONTROL L 15
AIR POLLUTION CONTROL L 15
 
AIR POLLUTION CONTROL L 12 and 13
AIR POLLUTION CONTROL L  12 and 13AIR POLLUTION CONTROL L  12 and 13
AIR POLLUTION CONTROL L 12 and 13
 
Environmental Lapse Rate vs Adibatic Lapse Rate
Environmental Lapse Rate vs Adibatic Lapse RateEnvironmental Lapse Rate vs Adibatic Lapse Rate
Environmental Lapse Rate vs Adibatic Lapse Rate
 
Atmospheric transport
Atmospheric transportAtmospheric transport
Atmospheric transport
 
Upper atmosphere air movements
Upper atmosphere air movementsUpper atmosphere air movements
Upper atmosphere air movements
 
Air pollution and meteorology
Air pollution and meteorologyAir pollution and meteorology
Air pollution and meteorology
 
2jottey
2jottey2jottey
2jottey
 
S290 Unit 0
S290 Unit 0S290 Unit 0
S290 Unit 0
 
Trouble in the air
Trouble in the airTrouble in the air
Trouble in the air
 
2 W&C OVERVIEW PPT
2 W&C OVERVIEW PPT 2 W&C OVERVIEW PPT
2 W&C OVERVIEW PPT
 

Semelhante a S290 Unit 6 part 1

HeatEnginesVol 1 Chapter 1 RS.pdf
HeatEnginesVol 1 Chapter 1 RS.pdfHeatEnginesVol 1 Chapter 1 RS.pdf
HeatEnginesVol 1 Chapter 1 RS.pdf
DagmawiGenanaw
 
The State of Atmosphere Stability and Instability Effects on Air Quality
The State of Atmosphere Stability and Instability Effects on Air QualityThe State of Atmosphere Stability and Instability Effects on Air Quality
The State of Atmosphere Stability and Instability Effects on Air Quality
theijes
 
Atmospheric Dispersion in Nuclear Power Plant Siting
Atmospheric Dispersion in Nuclear Power Plant SitingAtmospheric Dispersion in Nuclear Power Plant Siting
Atmospheric Dispersion in Nuclear Power Plant Siting
Hussain Majid
 
Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...
Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...
Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...
ujiburrahman2
 
Thermodynamics Lecture 1
Thermodynamics Lecture 1Thermodynamics Lecture 1
Thermodynamics Lecture 1
VJTI Production
 
Sheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docx
Sheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docxSheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docx
Sheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docx
lesleyryder69361
 

Semelhante a S290 Unit 6 part 1 (20)

HeatEnginesVol 1 Chapter 1 RS.pdf
HeatEnginesVol 1 Chapter 1 RS.pdfHeatEnginesVol 1 Chapter 1 RS.pdf
HeatEnginesVol 1 Chapter 1 RS.pdf
 
Bradley witham lesson 4
Bradley witham lesson 4Bradley witham lesson 4
Bradley witham lesson 4
 
The State of Atmosphere Stability and Instability Effects on Air Quality
The State of Atmosphere Stability and Instability Effects on Air QualityThe State of Atmosphere Stability and Instability Effects on Air Quality
The State of Atmosphere Stability and Instability Effects on Air Quality
 
Industrial Air Controls
Industrial Air ControlsIndustrial Air Controls
Industrial Air Controls
 
08-Tephigrams.ppt
08-Tephigrams.ppt08-Tephigrams.ppt
08-Tephigrams.ppt
 
Atmospheric Dispersion in Nuclear Power Plant Siting
Atmospheric Dispersion in Nuclear Power Plant SitingAtmospheric Dispersion in Nuclear Power Plant Siting
Atmospheric Dispersion in Nuclear Power Plant Siting
 
Basic meteorological processes
Basic meteorological processesBasic meteorological processes
Basic meteorological processes
 
Chapter03.pure substance
Chapter03.pure substanceChapter03.pure substance
Chapter03.pure substance
 
Physics and its laws in anaesthesia
Physics and its laws in anaesthesiaPhysics and its laws in anaesthesia
Physics and its laws in anaesthesia
 
Physics and its laws in anesthesia
Physics and its laws in anesthesiaPhysics and its laws in anesthesia
Physics and its laws in anesthesia
 
IRJET- Study on Effect of Moisture Contain on Temperature
IRJET-  	  Study on Effect of Moisture Contain on TemperatureIRJET-  	  Study on Effect of Moisture Contain on Temperature
IRJET- Study on Effect of Moisture Contain on Temperature
 
Properties of pure substances
Properties of pure substancesProperties of pure substances
Properties of pure substances
 
ATMOSPHERIC THERMODYNAMICS BASIC CONCEPTS.pptx
ATMOSPHERIC THERMODYNAMICS BASIC CONCEPTS.pptxATMOSPHERIC THERMODYNAMICS BASIC CONCEPTS.pptx
ATMOSPHERIC THERMODYNAMICS BASIC CONCEPTS.pptx
 
Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...
Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...
Mekanika Fluida 1 P2. Oke.pdf, Presentasi kuliah pertemuan 2 untuk mata kulia...
 
Air + Plane
Air + PlaneAir + Plane
Air + Plane
 
Psychrometry and air conditioning
Psychrometry and air conditioningPsychrometry and air conditioning
Psychrometry and air conditioning
 
Thermodynamics Lecture 1
Thermodynamics Lecture 1Thermodynamics Lecture 1
Thermodynamics Lecture 1
 
am3.pptx
am3.pptxam3.pptx
am3.pptx
 
Sheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docx
Sheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docxSheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docx
Sheet1Initial Popluation0Rate 10Rate 20Rate 30Time (years)Future P.docx
 
HYDRAULICS AND PNEUMATICS (UNIT 4)
HYDRAULICS AND PNEUMATICS   (UNIT 4)HYDRAULICS AND PNEUMATICS   (UNIT 4)
HYDRAULICS AND PNEUMATICS (UNIT 4)
 

Mais de University of Alaska, Fairbanks

Mais de University of Alaska, Fairbanks (16)

Cabin Point Protection in Alaska
Cabin Point Protection in AlaskaCabin Point Protection in Alaska
Cabin Point Protection in Alaska
 
AK Orientation part 2
AK Orientation part 2AK Orientation part 2
AK Orientation part 2
 
AK Orientation part 1
AK Orientation part 1AK Orientation part 1
AK Orientation part 1
 
S215 unit 10
S215 unit 10S215 unit 10
S215 unit 10
 
S215 unit 9
S215 unit 9S215 unit 9
S215 unit 9
 
S215 unit 8
S215 unit 8S215 unit 8
S215 unit 8
 
S215 unit 7
S215 unit 7S215 unit 7
S215 unit 7
 
S215 unit 6
S215 unit 6S215 unit 6
S215 unit 6
 
S215 unit 5
S215 unit 5S215 unit 5
S215 unit 5
 
S215 unit 4
S215 unit 4S215 unit 4
S215 unit 4
 
S215 unit 3
S215 unit 3S215 unit 3
S215 unit 3
 
S215 unit 2
S215 unit 2S215 unit 2
S215 unit 2
 
S215 unit 1
S215 unit 1S215 unit 1
S215 unit 1
 
S215 unit 0
S215 unit 0S215 unit 0
S215 unit 0
 
P 101 ep 3-g
P 101 ep 3-gP 101 ep 3-g
P 101 ep 3-g
 
P 101 ep 3-f
P 101 ep 3-fP 101 ep 3-f
P 101 ep 3-f
 

Último

Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
ZurliaSoop
 

Último (20)

Unit 3 Emotional Intelligence and Spiritual Intelligence.pdf
Unit 3 Emotional Intelligence and Spiritual Intelligence.pdfUnit 3 Emotional Intelligence and Spiritual Intelligence.pdf
Unit 3 Emotional Intelligence and Spiritual Intelligence.pdf
 
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptxSKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
SKILL OF INTRODUCING THE LESSON MICRO SKILLS.pptx
 
2024-NATIONAL-LEARNING-CAMP-AND-OTHER.pptx
2024-NATIONAL-LEARNING-CAMP-AND-OTHER.pptx2024-NATIONAL-LEARNING-CAMP-AND-OTHER.pptx
2024-NATIONAL-LEARNING-CAMP-AND-OTHER.pptx
 
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
Jual Obat Aborsi Hongkong ( Asli No.1 ) 085657271886 Obat Penggugur Kandungan...
 
Mehran University Newsletter Vol-X, Issue-I, 2024
Mehran University Newsletter Vol-X, Issue-I, 2024Mehran University Newsletter Vol-X, Issue-I, 2024
Mehran University Newsletter Vol-X, Issue-I, 2024
 
Graduate Outcomes Presentation Slides - English
Graduate Outcomes Presentation Slides - EnglishGraduate Outcomes Presentation Slides - English
Graduate Outcomes Presentation Slides - English
 
Holdier Curriculum Vitae (April 2024).pdf
Holdier Curriculum Vitae (April 2024).pdfHoldier Curriculum Vitae (April 2024).pdf
Holdier Curriculum Vitae (April 2024).pdf
 
Kodo Millet PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
Kodo Millet  PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...Kodo Millet  PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
Kodo Millet PPT made by Ghanshyam bairwa college of Agriculture kumher bhara...
 
SOC 101 Demonstration of Learning Presentation
SOC 101 Demonstration of Learning PresentationSOC 101 Demonstration of Learning Presentation
SOC 101 Demonstration of Learning Presentation
 
Accessible Digital Futures project (20/03/2024)
Accessible Digital Futures project (20/03/2024)Accessible Digital Futures project (20/03/2024)
Accessible Digital Futures project (20/03/2024)
 
Jamworks pilot and AI at Jisc (20/03/2024)
Jamworks pilot and AI at Jisc (20/03/2024)Jamworks pilot and AI at Jisc (20/03/2024)
Jamworks pilot and AI at Jisc (20/03/2024)
 
Sensory_Experience_and_Emotional_Resonance_in_Gabriel_Okaras_The_Piano_and_Th...
Sensory_Experience_and_Emotional_Resonance_in_Gabriel_Okaras_The_Piano_and_Th...Sensory_Experience_and_Emotional_Resonance_in_Gabriel_Okaras_The_Piano_and_Th...
Sensory_Experience_and_Emotional_Resonance_in_Gabriel_Okaras_The_Piano_and_Th...
 
Food safety_Challenges food safety laboratories_.pdf
Food safety_Challenges food safety laboratories_.pdfFood safety_Challenges food safety laboratories_.pdf
Food safety_Challenges food safety laboratories_.pdf
 
HMCS Max Bernays Pre-Deployment Brief (May 2024).pptx
HMCS Max Bernays Pre-Deployment Brief (May 2024).pptxHMCS Max Bernays Pre-Deployment Brief (May 2024).pptx
HMCS Max Bernays Pre-Deployment Brief (May 2024).pptx
 
Fostering Friendships - Enhancing Social Bonds in the Classroom
Fostering Friendships - Enhancing Social Bonds  in the ClassroomFostering Friendships - Enhancing Social Bonds  in the Classroom
Fostering Friendships - Enhancing Social Bonds in the Classroom
 
How to Manage Global Discount in Odoo 17 POS
How to Manage Global Discount in Odoo 17 POSHow to Manage Global Discount in Odoo 17 POS
How to Manage Global Discount in Odoo 17 POS
 
Python Notes for mca i year students osmania university.docx
Python Notes for mca i year students osmania university.docxPython Notes for mca i year students osmania university.docx
Python Notes for mca i year students osmania university.docx
 
On National Teacher Day, meet the 2024-25 Kenan Fellows
On National Teacher Day, meet the 2024-25 Kenan FellowsOn National Teacher Day, meet the 2024-25 Kenan Fellows
On National Teacher Day, meet the 2024-25 Kenan Fellows
 
Introduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The BasicsIntroduction to Nonprofit Accounting: The Basics
Introduction to Nonprofit Accounting: The Basics
 
How to Create and Manage Wizard in Odoo 17
How to Create and Manage Wizard in Odoo 17How to Create and Manage Wizard in Odoo 17
How to Create and Manage Wizard in Odoo 17
 

S290 Unit 6 part 1

  • 1. 6-1-S290-EPUnit 6 Atmospheric Stability Unit 6 Atmospheric Stability
  • 2. 6-2-S290-EPUnit 6 Atmospheric Stability Unit 6 Objectives 2. Describe temperature lapse rate and stability, and the different temperature lapse rates used to determine the stability of the atmosphere. 4. Name four types of temperature inversions and describe their influence on wildland fire behavior, including the thermal belt. 3. Describe the effects of atmospheric stability on wildland fire behavior. 1. Describe the relationship among atmospheric pressure, temperature, density and volume.
  • 3. 6-3-S290-EPUnit 6 Atmospheric Stability 5. Name and describe the four lifting processes that can produce thunderstorms. 6. Describe the elements of a thunderstorm and its three stages of development. 7. Use visual indicators to describe the stability of the atmosphere. 8. Describe the four principle cloud groups, and identify the six clouds most often associated with critical wildland fire behavior. Unit 6 Objectives
  • 4. 6-4-S290-EPUnit 6 Atmospheric Stability Up to now, our attention has been on temperature and the factors that influence its change on and near the earth’s surface. In this unit we will focus on air temperature in the third dimension, atmospheric stability, and how stability affects wildland fire behavior. We will also discuss several visual indicators commonly used to identify critical changes in atmospheric stability.
  • 5. 6-5-S290-EPUnit 6 Atmospheric Stability Our atmosphere is composed of numerous gases. This gaseous mixture includes permanent dry air gases such as nitrogen, oxygen, argon, helium, hydrogen, and xenon. Nitrogen and oxygen account for 99% of all permanent dry air gases in the troposphere.
  • 6. 6-6-S290-EPUnit 6 Atmospheric Stability The remaining gases, called variable gases; include water vapor, carbon dioxide, methane, nitrous oxide and ozone. Of these gases, water vapor is the most abundant, varying from a trace to 4 percent by volume.
  • 7. 6-7-S290-EPUnit 6 Atmospheric Stability Nearly all gases in the atmosphere respond uniformly to changes in temperature and pressure. Behavior of Gases For that reason, we can use the Ideal Gas Law (Equation of State) which is based on a set of gas behavior laws, to describe their behavior.
  • 8. 6-8-S290-EPUnit 6 Atmospheric Stability The relationship among pressure, temperature and density (mass per volume) can be expressed by the gas law equation where: P is pressure, ρ is density, m is the mass of the gas, V is volume, R is a gas constant, and T is temperature. P = (ρ)RT or P = (m/V)RT
  • 9. 6-9-S290-EPUnit 6 Atmospheric Stability R is the gas constant, and can be ignored. ~ is the symbol meaning “is proportional to.” Again: The term (m/V) represents the density (ρ) of the gas. P ~ (ρ)T or P ~ (m/V)T
  • 10. 6-10-S290-EPUnit 6 Atmospheric Stability Often when referring to air in motion, we represent it in small units or volumes called air parcels.
  • 11. 6-11-S290-EPUnit 6 Atmospheric Stability An air parcel is a volume of air, large enough to contain a great number of molecules, but small enough so that its energy (heat) and mass (air molecules) are nearly uniform within is boundaries. Air Parcel
  • 12. 6-12-S290-EPUnit 6 Atmospheric Stability Air parcels expand and contract freely, but neither heat nor outside air is able to mix with air inside; making an air parcel a sealed container. Air parcels are commonly portrayed as 3-dimensional cubes or spheres. Air Parcel
  • 13. 6-13-S290-EPUnit 6 Atmospheric Stability Rising Air Parcel As atmospheric pressure decreases with increasing altitude:  volume increases  density decreases Rising air parcels always expand and cool Cooler & Less dense  temperature decreases Applying this Relationship To a Rising Air Parcel
  • 14. 6-14-S290-EPUnit 6 Atmospheric Stability Sinking Air Parcel As atmospheric pressure increases with decreasing altitude:  volume decreases  temperature increases Sinking air parcels always compress and warm Warmer & more dense  density increases Applying this Relationship To a Sinking Air Parcel
  • 15. 6-15-S290-EPUnit 6 Atmospheric Stability When an air parcel rises or sinks without any loss of energy or mass to the surrounding atmosphere ADIABATIC PROCESS
  • 16. 6-16-S290-EPUnit 6 Atmospheric Stability EXERCISE 1
  • 17. 6-17-S290-EPUnit 6 Atmospheric Stability Air in Motion The rotation of the earth on its axis, together with large and small scale variations in pressure and temperature are what produce the horizontal and vertical movement of air in the atmosphere.
  • 18. 6-18-S290-EPUnit 6 Atmospheric Stability 06-18-S290-EP Wind and Stability 6-18-S290-EP
  • 19. 6-19-S290-EPUnit 6 Atmospheric Stability The magnitude or strength of wind is far greater than the vertical movement of air associated with atmospheric stability. However, their influence on the behavior of wildland fires is equally important. In this unit, our attention will be on vertically moving air associated with atmospheric stability.
  • 20. 6-20-S290-EPUnit 6 Atmospheric Stability What is Stability? It is the resistance of the atmosphere to vertical motion. More precisely, it is the degree to which vertical motion in the atmosphere is enhanced or suppressed. Depending on the vertical temperature profile of the atmosphere, air will either rise, sink or remain at rest.
  • 21. 6-21-S290-EPUnit 6 Atmospheric Stability Stable Atmosphere Suppresses or resists vertical movement of air Unstable Atmosphere Enhances or encourages vertical movement of air Three Types of Stability Neutral Atmosphere Neither suppresses nor enhances vertical movement of air. This condition seldom exists for long periods of time.
  • 22. 6-22-S290-EPUnit 6 Atmospheric Stability Unstable Atmosphere Air parcels will continue to rise Level of Origin
  • 23. 6-23-S290-EPUnit 6 Atmospheric Stability Rising Air Unstable Atmosphere Promotes the formation and growth of vertically developed clouds, thunderstorms and tall smoke columns
  • 24. 6-24-S290-EPUnit 6 Atmospheric Stability Stable Atmosphere Air parcels displaced upward (downward) will eventually return to their level of origin. Level of Origin
  • 25. 6-25-S290-EPUnit 6 Atmospheric Stability Stable Atmosphere Light winds and poor smoke dispersal from poor vertical mixing trapped smoke and haze
  • 26. 6-26-S290-EPUnit 6 Atmospheric Stability In mountainous terrain, however, stable conditions can produce gusty ridgetop winds, and warm, dry and gusty downslope winds called foehn winds. mountain wave clouds windward slope leeward slope foehn wind
  • 27. 6-27-S290-EPUnit 6 Atmospheric Stability Neutral Stability • Usually exists for only short periods of time during the transition between a stable and an unstable atmosphere. • Little vertical air motion occurs. • If this condition should exist through a deep layer of atmosphere, an air parcel’s vertical motion will cease.
  • 28. 6-28-S290-EPUnit 6 Atmospheric Stability An unstable atmosphere is most often associated with critical or extreme wildland fire behavior.
  • 29. 6-29-S290-EPUnit 6 Atmospheric Stability A stable atmosphere will tend to suppress or reduce wildland fire behavior.
  • 30. 6-30-S290-EPUnit 6 Atmospheric Stability Neutral atmospheric conditions have little if any effect on wildland fire behavior.
  • 31. 6-31-S290-EPUnit 6 Atmospheric Stability Four Ways To Change Atmospheric Stability Heating from below Warming aloft Cooling from below Cooling aloft
  • 32. 6-32-S290-EPUnit 6 Atmospheric Stability Temperature Lapse Rate The change in temperature with a change in altitude. Change in Temperature Change in Altitude
  • 33. 6-33-S290-EPUnit 6 Atmospheric Stability Temperature Lapse Rates differ throughout the troposphere, particularly in the lowest 3000 feet above the ground where air temperature is strongly influenced by: • daytime solar heating • nighttime radiational cooling
  • 34. 6-34-S290-EPUnit 6 Atmospheric Stability This lowest layer of the troposphere is called the boundary layer.Boundary Layer We will often refer to the boundary layer near the ground.
  • 35. 6-35-S290-EPUnit 6 Atmospheric Stability +15ºF per 1000 feet, within a 24 hour period Lapse Rates within the Boundary Layer
  • 36. 6-36-S290-EPUnit 6 Atmospheric Stability Recall from Unit 4 that temperature normally decreases with increasing altitude in the troposphere. cooling
  • 37. 6-37-S290-EPUnit 6 Atmospheric Stability Air temperature can also increase with increasing altitude in the troposphere. This reversal in the normal trend in temperature reduction with altitude is what we refer to as an inversion. (More on inversions later)
  • 38. 6-38-S290-EPUnit 6 Atmospheric Stability Positive Lapse Rate Warming with Increasing Altitude Negative Lapse Rate Cooling with Increasing Altitude
  • 39. 6-39-S290-EPUnit 6 Atmospheric Stability Weather observing balloons called radiosondes, and other observing systems, including weather satellites and aircraft, are routinely used to record changes in air temperature aloft. Determining the Lapse Rate
  • 40. 6-40-S290-EPUnit 6 Atmospheric Stability Three Lapse Rates You Need to Know • Dry Adiabatic Lapse Rate • Moist Adiabatic Lapse Rate • Average Lapse Rate
  • 41. 6-41-S290-EPUnit 6 Atmospheric Stability Represents the rate of change in temperature of rising and sinking unsaturated air. Dry Adiabatic Lapse Rate Rising “dry” air will always cool at a rate of -5.5º F per 1000 feet. Sinking “dry” air will always warm at a rate of +5.5º F per 1000 feet.
  • 42. 6-42-S290-EPUnit 6 Atmospheric Stability Moist Adiabatic Lapse Rate Rising saturated air cools at a rate of approximately -3.0ºF per 1000 feet. Represents the rate of change in temperature of rising and sinking saturated air.
  • 43. 6-43-S290-EPUnit 6 Atmospheric Stability Heat released during condensation offsets the cooling that occurs due to expansion. Heat released during condensation offsets the cooling that occurs due to expansion. Rising saturated air parcels also lose mass, in the form of cloud droplets and precipitation. Rising saturated air parcels also lose mass, in the form of cloud droplets and precipitation. During the Moist Adiabatic Process During the Moist Adiabatic Process saturated parcel Not a true adiabatic processNot a true adiabatic process 6-43-S290-EP
  • 44. 6-44-S290-EPUnit 6 Atmospheric Stability Sinking air parcels rarely warm at the moist lapse rate. Once saturated air begins to sink, for example down the lee slope of a mountain range, compression causes it to warm. Once this air becomes unsaturated, or its relative humidity lowers below 100 percent, this sinking air will warm at the faster dry adiabatic lapse rate of +5.5ºF per 1000 feet. 6-44-S290-EP
  • 45. 6-45-S290-EPUnit 6 Atmospheric Stability The skew-T diagram is used to represent the pressure, temperature, density, moisture, wind and atmospheric stability within a column of atmosphere above a point on the earth’s surface. 6-45-S290-EP
  • 46. 6-46-S290-EPUnit 6 Atmospheric Stability Average Lapse Rate: +/- 3.5ºF per 1000 feet Represents average vertical temperature change for the entire troposphere. Can NOT be used to determine the stability of the atmosphere.
  • 47. 6-47-S290-EPUnit 6 Atmospheric Stability Because of variations in topography, vegetation, wind, cloud cover, etc. avoid using a lapse rate to project temperatures more than 2000 feet above or below your location. Average lapse rate is useful for estimating temperature and RH for a shallow layer in the atmosphere or for a point on a mountain side.
  • 48. 6-48-S290-EPUnit 6 Atmospheric Stability Example Using the Average Lapse Rate 4500 ft. 94ºF 6500 ft. 87ºF -3.5ºF/1000 ft Knowing your temperature at an elevation 4500 feet, project the temperature on a fireline at 6500 feet using the average lapse rate. Elevation Change: 2000 feet Lapse rate: -3.5ºF/1000 feet Temp. at 6500 feet: 87ºF Temp. Change: (2 x -3.5ºF) Average Lapse Rate
  • 49. 6-49-S290-EPUnit 6 Atmospheric Stability 0 ft AGL0 ft AGL 5,000 ft AGL5,000 ft AGL 13,000 ft AGL13,000 ft AGL 80.080.0ºº FF 52.552.5ºº FF 8.58.5ºº FF A Day in the Life of aA Day in the Life of a Rising Air ParcelRising Air Parcel If the parcel becomes saturated during its ascent, at 5,000 feet for instance, a cloud forms; assuming the parcel remains saturated as it continues to rise. 74.074.0ºº FF 49.049.0ºº FF 8.08.0ºº FF bare field Fields covered with vegetation 6-49-S290-EP
  • 50. 6-50-S290-EPUnit 6 Atmospheric Stability 06-50-S290-EP 90ºF90ºF 82ºF82ºF80ºF80ºF The greater the temperature difference between an air parcel and the surrounding air, the faster the parcel will rise or sink. This difference in temperature is an indicator of how unstable or stable a layer of atmosphere is. The greater the temperature difference between an air parcel and the surrounding air, the faster the parcel will rise or sink. This difference in temperature is an indicator of how unstable or stable a layer of atmosphere is. Fast Slow air temp. How Fast Will Air Rise?How Fast Will Air Rise? 6-50-S290-EP
  • 51. 6-51-S290-EPUnit 6 Atmospheric Stability Large wildfires can produce strong convective updrafts capable of lifting debris as large as small trees hundreds of feet into the air. Strong Updraft
  • 52. 6-52-S290-EPUnit 6 Atmospheric Stability Influence of Moisture on Atmospheric Stability Dry air is generally more STABLE than UNSTABLE because it is “heavier.”
  • 53. 6-53-S290-EPUnit 6 Atmospheric Stability 06-53-S290-EP Use the appropriate lapse rates to calculate the temperatureUse the appropriate lapse rates to calculate the temperature of this moving air parcel at the designated altitudes.of this moving air parcel at the designated altitudes. 80F80F ?? ?? ?? ?? 63.5F 48.5F 76.0F 92.5F Exercise 2 UNSTABLE STABLE 6-53-S290-EP
  • 54. 6-54-S290-EPUnit 6 Atmospheric Stability EXERCISE 3 Lapse Rates and Atmospheric Stability
  • 55. 6-55-S290-EPUnit 6 Atmospheric Stability The Mixing Layer Top of the Mixing Layer Earth’s Surface The lowest layer of the troposphere where surface heating mixes and vertically transports air molecules, water vapor and pollutants, such as smoke, potentially to thousands of feet above the ground. Over United States varies from about 1/2 to 3 1/2 miles thick 6-55-S290-EP
  • 56. 6-56-S290-EPUnit 6 Atmospheric Stability 06-56-S290-EP Deepest over the Interior of Continents Shallowest over Oceans and Coastal Regions Shallowest over Oceans and Coastal Regions Generally deepest or highest over the interior regions ofover the interior regions of continents and tropical regions, and is shallowest orcontinents and tropical regions, and is shallowest or lowest over the oceans, coasts and polar regionslowest over the oceans, coasts and polar regions Generally deepest or highest over the interior regions ofover the interior regions of continents and tropical regions, and is shallowest orcontinents and tropical regions, and is shallowest or lowest over the oceans, coasts and polar regionslowest over the oceans, coasts and polar regions The Mixing Layer or Convective Mixing Layer 6-56-S290-EP
  • 57. 6-57-S290-EPUnit 6 Atmospheric Stability Top of the Mixing Layer Top of the Mixing Layer The convective mixing layer is normally “capped” by a layer of very stable air, which limits the rise of vertically developed clouds and smoke columns. The tops of tall smoke columns and cumulonimbus clouds are often seen spreading out at the top of the mixing layer. 6-57-S290-EP
  • 58. 6-58-S290-EPUnit 6 Atmospheric Stability Evolution of the Daytime Mixing Layer 55ºF 58F 63ºF 75ºF 80ºF 88ºF 8 AM 10 AM Noon 2 PM 8 AM 1500 Ft AGL10 AM 2800 FT AGL Noon 7400 Ft AGL 2 PM 12,000 Ft AGL Maximum Mixing Height G r o u n d 6-58-S290-EP
  • 59. 6-59-S290-EPUnit 6 Atmospheric Stability Seasonal Variation in the Height of the Mixing Layer The depth of the mixing layer varies considerably during the year. Average depth of the Mixing Layer The wildfire is at 2,500 feet ASL.
  • 60. 6-60-S290-EPUnit 6 Atmospheric Stability Effects of Unstable Atmospheric Conditions on Wildland Fire Behavior • Increased likelihood of fire whirls and dust devils • Increased likelihood for gusty and erratic surface winds • The height and strength of convection and smoke columns often increase significantly • Increased likelihood of fire brands being lifted to great heights
  • 61. 6-61-S290-EPUnit 6 Atmospheric Stability Effects of Stable Atmospheric Conditions on Wildland Fire Behavior • Limited rise of smoke columns, resulting in poor smoke dispersion and visibility. • Reduced inflow of fresh air, thereby limiting wildland fire growth and intensity. • Lowers surface wind speeds and fire spread rates except in mountainous or hilly terrain.
  • 62. 6-62-S290-EPUnit 6 Atmospheric Stability A combination of: stability and dryness Indicates potential for large plume-dominated fire growth. Haines Index
  • 63. 6-63-S290-EPUnit 6 Atmospheric Stability Due to large elevation differences, three atmospheric layers are used to determine the Haines Index. Haines Index Low: 2,000-5,000 ft Mid: 5,000-10,000 ft High: 10,000-18,000 ft
  • 64. 6-64-S290-EPUnit 6 Atmospheric Stability Haines Index Numbers The Potential for Large Plume Dominated Fire Growth 2 or 3 … Very low potential 4 … Low potential 5 … Moderate potential 6 … High potential
  • 65. 6-65-S290-EPUnit 6 Atmospheric Stability Haines Index The drier and more unstable the lower atmosphere, the HIGHER the Haines Index. Bottom Line… The more humid and stable the lower atmosphere, the LOWER the Haines Index.
  • 67. 6-67-S290-EPUnit 6 Atmospheric Stability An inversion is a layer of very stable air where temperature increases with an increase in altitude. An inversion acts like a cap or lid to severely limit the upward movement of air. Inversions often exist at many levels of the troposphere. What is a Temperatures Inversion? Warmer 6-67-S290-EP
  • 68. 6-68-S290-EPUnit 6 Atmospheric Stability Four Types of Inversions 6-68-S290-EP
  • 69. 6-69-S290-EPUnit 6 Atmospheric Stability Nighttime or Radiation Inversion Sunset Midnight Sunrise During the evening hours, this surface based inversion is weak and shallow, usually no more than a few hundred feet deep. As cold air drainage and radiational cooling continues overnight, this inversion strengthens and eventually reaches its maximum depth around sunrise when surface temperatures are at their lowest. Strong cold air drainage Weak cold air drainage Little or no drainage flow Weak inversion Moderate Inversion Strong Inversion 6-69-S290-EP
  • 70. 6-70-S290-EPUnit 6 Atmospheric Stability The depth or strength of the nighttime or radiation inversion can range from several hundred feet to several thousand feet depending on: cloud cover, wind, precipitation, snow cover, valley or canyon width and depth, and time of year
  • 71. 6-71-S290-EPUnit 6 Atmospheric Stability Weak, Shallow Nighttime Inversion Strong, Deep Nighttime Inversion Effects of Cloud Cover and Wind Surface-based nighttime or radiation inversions are deepest or strongest on clear nights with light or no winds; and shallowest or weakest on cloudy, breezy nights. Top of the Inversion Top of the Inversion
  • 72. 6-72-S290-EPUnit 6 Atmospheric Stability Dissipation of the Nighttime Inversion Early Morning Top of Surface Based Inversion Transport Wind 20-ft wind Mid-Morning Transport Wind Top of the Inversion Rises as it Weakens 20-ft wind Late Morning Transport Wind Surface Inversion Has Dissipated 20-foot Wind When the surface inversion breaks, fire intensity may suddenly increase with a rush of fresh oxygen. 6-72-S290-EP
  • 73. 6-73-S290-EPUnit 6 Atmospheric Stability What to Expect When Nighttime Inversions Break • Winds often increase suddenly and possibly become gusty and erratic • Air temperature increases suddenly • Relative humidity decreases suddenly
  • 74. 6-74-S290-EPUnit 6 Atmospheric Stability There are several aspects of stable air that should be understood by the firefighter: One is the relationship of the nighttime or radiation inversion to thermal belts.
  • 75. 6-75-S290-EPUnit 6 Atmospheric Stability The Thermal Belt Thermal belts form where the top of the nighttime inversion makes frequent contact with valley wall or mountain slope. Highest temperature and lowest average relative humidity at night. Nighttime 6-75-S290-EP
  • 76. 6-76-S290-EPUnit 6 Atmospheric Stability Hazards of the Thermal Belt Dries out fuels and can create severe burning conditions. Most importantly: active burning at night, while areas above and below relatively quiet. Nighttime 6-76-S290-EP
  • 77. 6-77-S290-EPUnit 6 Atmospheric Stability Elevation and location of the thermal belt varies by: • Locality • Time of year • Length of nighttime darkness • Size and steepness of the valley or canyon
  • 78. 6-78-S290-EPUnit 6 Atmospheric Stability Summer Nights Winter Nights Shallow Inversions Deep Inversions Higher on winter nights with stronger radiational cooling and cold air drainage. May be thousands of feet above the valley floor. Lower on valley walls and mountain slopes during the summer with shorter nights and less radiational cooling and cold air drainage. 6-78-S290-EP
  • 79. 6-79-S290-EPUnit 6 Atmospheric Stability Thermal belts tend to form higher on the walls of broad valleys and gently slopes canyons. Lower on mountain slopes and steep canyons with strong drainage. Broad Valleys 6-79-S290-EP
  • 80. 6-80-S290-EPUnit 6 Atmospheric Stability Nighttime cloud cover will limit the depth of the nighttime or radiation inversion. Shallow Inversion Deep Inversion Clear Nights Cloudy Nights Thermal Belt Thermal Belt Thermal Belt Thermal Belt 6-80-S290-EP
  • 81. 6-81-S290-EPUnit 6 Atmospheric Stability Frontal Inversion The frontal inversion is strongest behind the advancing frontal boundary, as much as a hundred miles or more. warmer, lighter air cooler, heavier air 6-81-S290-EP
  • 82. 6-82-S290-EPUnit 6 Atmospheric Stability 06-82-S290-EP Marine Inversion • Commonly found along the shorelines of large lakes and the West coast of the United States. • Varies in depth from a few hundred feet to several thousand, and may extend hundreds of miles inland. Ocean Stratus clouds Similar to frontal inversions, but often with more moisture Ocean 6-82-S290-EP
  • 83. 6-83-S290-EPUnit 6 Atmospheric Stability Warm, drier air aloft Inland Extent of Marine Inversions Cool, moist and stable marine air beneath a layer of warm, dry and unstable air will frequently move over the lowlands along the west coast with the diurnal cycle of winds and temperature.
  • 84. 6-84-S290-EPUnit 6 Atmospheric Stability Subsidence Inversion Form when an extensive layer of atmosphere slowly sinks beneath a large ridge of high pressure.
  • 85. 6-85-S290-EPUnit 6 Atmospheric Stability Lowering Subsidence Inversion Subsidence is a slow process that can occur over several days.
  • 86. 6-86-S290-EPUnit 6 Atmospheric Stability The top of mountain ranges will experience the warm, very dry conditions of the subsidence inversion first. Poor smoke dispersal conditions may also develop below a lowering subsidence inversion. Temperature Sounding
  • 87. 6-87-S290-EPUnit 6 Atmospheric Stability Subsidence Inversions Subsidence Inversions Subsidence Inversions Strongest in late summer and autumn, on the North and East sides of strong high pressure ridges. Sometimes remains over a region for weeks at a time. Aloft Aloft
  • 88. 6-88-S290-EPUnit 6 Atmospheric Stability Winds on flat terrain are normally light in speed underneath large high pressure ridges and subsidence inversions. In mountain regions, these same atmospheric conditions can produce warm and dry downslope winds called foehn winds. light winds light winds Light winds HH gusty winds gusty winds Foehn Winds Subsidence and Foehn Winds 6-88-S290-EP
  • 89. 6-89-S290-EPUnit 6 Atmospheric Stability EXERCISE 4 Stability and Its Effects On Wildland Fire Behavior
  • 90. 6-90-S290-EPUnit 6 Atmospheric Stability End of Part I