K

GEOG 110 01

Week 1

08/25/2025 Homework Reading (Chapter 1)

  • Weather is the state of atmosphere at a specific place and time described quantitatively by temperature, humidity, cloudiness, precipitation, and wind.

  • Meteorology is the study of the atmosphere and the life cycle of weather systems.

  • Climate refers to weather conditions averaged over a specific time — commonly 30 years — along with extremes.

  • Weather maps graphically portray atmospheric conditions across a broad region.

    • Symbols identify high-pressure systems (anticyclones) and low-pressure systems (cyclones).

  • Climatology is the study of climate, its controls, and spatial and temporal variability.

    • Description of the climate

      • Random terms:   

        • Maximum temperature: The highest air temperature recorded over a 24-hour period.

        • Minimum temperature: The lowest air temperature recorded over a 24-hour period.

        • Dewpoint/Front Point: The temperature to which air must be cooled at constant pressure to become saturated with water vapor and for dew to begin forming on relatively cold surfaces.

        • Relative humidity: A measure of the actual concentration of the water vapor component of air compared to the concentration the air would have if saturated with water vapor.

        • Precipitation amount: Depth of rainfall or melted snowfall over a 24-hour period.

        • Air pressure: The weight of a column of air over a unit area of the Earth’s surface.

        • Wind direction and wind speed: According to meteorological tradition, wind direction is the compass direction from which the wind blows.

  • An air mass is a huge volume of air covering hundreds of thousands of square kilometers that has relatively uniform temperature and humidity properties in its horizontal extent.

    • Typically associated with a large high pressure system and its specific characteristics depend on the types of surfaces over which the air mass forms (its source region) and travels.

    • Four basic types of air masses:

      • Cold

      • Dry

      • Cold and Humid

      • Warm and Humid

  • A front is a narrow transition zone between air masses that differ in temperature, humidity, or both.

    • Forms where contrasting air masses meet, and the associated air movements often give rise to the cloudiness and precipitation.

      • Most common fronts”

        • Stationary

          • Literally a stationary front

          • On both sides of a stationary front, winds blow roughly parallel to the front but in opposite directions.

        • Cold

          • Advances by sliding under and pushing up the less dense warm air and the leading edge of cold air at the Earth’s surface is plotted on a weather map as a cold front.

        • Warm

  • Cloud patterns on a visible satellite image are of particular interest to atmospheric scientists.

  • Weather radar complements satellite surveillance of the atmosphere by locating and tracking the movement of areas of precipitation and monitoring the circulation within small-scale weather systems such as thunderstorms.

Sky Watching

  1. Clouds are tiny water droplets.

  2. A cloud near the surface is fog.

  3. Stratiform Clouds: form horizontal layers. Cumuliform clouds: appear puffy.

08/27/2025

Weather

  • Present conditions

  • Changes constantly

  • Conditions are almost never “normal”

Climate

  • Average conditions for a specified place and time

  • “Normal” represents average of past 30 years of weather data

    • Because if you go more than 30 years climate change occurs. Its a slow moving thing but it changes slowly all the time.

  • Extremes are noted using the entire weather record.

  • Location is what controls climate.

    • How far is it from the equator?

      • The closer you get to the poles the colder is gets.

      • How close are you to the water because that also determines weather?

Time Keeping

  • Local time (“sun time”)

  • Standard time (time zones)

  • Z-time, GMT, and UTC

    • Z-Time = Zulu Time

      • Time on the prime meridian (standard time in London)

    • UTC = Universal time coordinated

    • All of these are basically the current time on the prime meridian (standard time in London)

  • All weather maps are marked for a specific time

    • All data is collected at a certain time anywhere, that’s why it is useful for everyone to have a standard time when collecting it.

      • Personal: Kind of like how most scientists use the metric system so they all recognize it all over.

  • Times of WX data collection are standardized in order to produce synoptic maps. “Synoptic” means “seen at one time”.

Anticyclone / Cyclones

  • The air pressures go down evenly on the isobars.

    • Isobars are the lines circulating the high or low air pressure markers.

      • The mega “H” or mega “L”

  • Anticyclones are clockwise, but in the Southern Hemisphere, they are anticlockwise.

    • The map in class is showing the northern hemisphere.

    • Anticyclone whiteboard notes:

      • Clockwise in northern hemisphere

      • Center of high pressure

      • Diverging from the center

      • Subsiding (sinking air)

      • Clear skies

      • Fair weather

      • Light winds

    • (For anticyclones) Air pressure always spirals outwards. “H” is pushing air outward, away from the middle. It is never going inward.

  • Cyclone

    • Center of low pressure

    • Moves counterclockwise or anti clockwise in the northern hemisphere

    • Converging air toward center

      • On the tree example it goes upward after pulling it in from the sides.

        • Combining air can’t occupy the same area, it needs to keep moving.

    • Rising air

    • Cloudy skies

    • Unsettled/rainy weather

    • Windy

Weather map symbols (cheat sheet)

Air masses and fronts

  • Air masses are large bodies of air that have generally uniform characteristics of temperature and humidity.

  • Fronts are located at contrasting air mass boundaries.

  • Air masses capture the characteristics of their source regions:

    • Cold if they come from high latitude regions: Canada, Artic Ocean, Siberia

    • Warm if they come from tropical regions: Gulf of Mexico/Caribbean, Mexico

    • Humid if they come from ocean source regions: Pacific, Atlantic, Gulf of Mexico

    • Dry if they come from land areas: Canada, Siberia, desserts of US SW, and Mexico

Fronts

  • Warm front: warm air rides up and over colder air at the surface as colder air slowly retreats.

  • Cold front: cold air advances into warm air wedging warm air upward and causing often intense precipitation along a narrow zone ahead of the front.

08/27/2025 Lab

  • Surface analysis

    • Surface map at a synoptic time of the Earth

  • Quiz:

    • Cloud Coverage

    • Wind direction

    • Dew Point

    • Temperature

    • Wind pressure rounded to the nearest 5 knots

08/29/2025

Shape and size of the Earth

  • Equator:

    • 12,756 Kilometers

    • 7926 Miles

    • Circumference: 40,075 Kilometers

  • South Pole

    • Distance to the equator:

      • 12,714 Kilometers

  • North Pole

    • Distance to the equator:

      • 7,900 Miles

The Earth rotates on an Axis

  • Because the earth rotates, it has an axis of rotation.

  • The North and South poles are the places where the earth’s axis intercepts the earth’s surface.

  • If standing at the north pole, the north star, Polaris, is exactly 90° upwards.

    • Polaris moves very little so it is an “anchor” point for our Earth.

    • Polaris/The North Star is at a fixed point in the sky, it will always indicate your latitude.

      • Unless you’re in the Southern Hemisphere.

  • Earth moves roughly 15° every hour.

Latitude

  • Latitude Lines (Parallels)

    • Are parallel to one another (they never meet, and never cross)

    • Are perpendicular to the axis of the Earth

    • Run east to west

    • Get progressively shorter away from the Equator

    • Measure distance north or south of the Equator

    • Have values from 0° to 90°

  • The Equator is 0° latitude.

    • It is the greatest circumference of the earth and makes up a set of points equidistant from both poles.

  • Only the Equator is a great circle among the lines of latitude.

Important Lines of Latitude

  • 0° Equator

  • 23.5° N, Tropic of Cancer

  • 23.5° S, Tropic of Capricorn

  • 66.5° N, Arctic Circle

  • 66.5° S, Antarctic Circle

  • 90° N, North Pole

  • 90° S, South Pole

Why are these particular lines of latitude important?

  • The tropics are latitudes where the sun strikes directly overhead sometime during the year.

  • The Arctic & Antarctic Circles mark the latitude where 24 hours of daylight, or 24 hours of darkness, occur in each hemisphere during the Solstices.

  • And the Poles mark Earth’s rotational axis.

Longitude

  • Lines of Longitude

  •     Join at each pole, but spread out at the Equator

    • Are perpendicular to the equator

    • Are known as meridians

    • Run north and south

    • Are all the same length, and are all great circles

    • Measure distance east and west of the Prime Meridian

    • Have values from 0° to 180°.

    • The Prime Meridian is an arbitrary starting point: 0° longitude could have been anywhere on Earth.

Week 2

09/03/2025 Pre-Lab Quiz Studying

  • The geographic grid is a system of lines, intersecting at right angles, used to locate any position on earth’s surface.

  • The rotational axis of Earth is an imaginary line connecting the North Pole and South Pole, and the equator.

  • The great circle is one that divides a sphere in two equal halves (hemispheres); it represents the circumference of the sphere, and is thus the largest circle that can be drawn on it.

  • Small circles do not cut the earth into two equal halves. All parallels of latitude except for the equator are small circles.

09/03/2025 (Class, Lana came in clutch)

Earth-Sun Relationships

  • The Solar Constant

    • Earth receives constant radiation from the Sun

    • At its distance of 150,000,000 Kilometers, top of atmosphere gets 1370 W/m2

      • A Watt (W) is one joule per second (J/S)

  • Bodies radiate according to their temperature

    • Earth captures small amounts of sun radiation.

      • Sun radiates in shorter wavelengths.

        • Due to higher temperatures.

    • Shortwave in (Sunlight)

    • Long wave out (Heat)

      • Earth radiates in all directions.

  • Comparing solar with terrestrial radiation

    • Greater Intensity

    • Shorter wavelengths

  • Earth’s orbit is slightly elliptical

    • Earth is closet to the sun in January and furthest in July

    • The closet point in orbit to the Sun is called perihelion (January 4)

    • The furthest point of orbit from the Sun is called aphelion (July 4)

  • Earth’s orbit at the correct scale

    • At true scale, Earth’s orbit around the Sun is almost a perfect circle.

    • Can the variation in distance be the cause of seasons?

      • No, for 2 reasons:

        • Distance changes out receipt of energy by only 3%

        • Northern Hemisphere has its summer when the southern hemisphere has its winter.

  • The plane of the Earth’s orbit in space is called the Ecliptic.

  • Earth’s Axiel Tilt

    • Viewed on the edge — ecliptic plane appears as a line.

    • Earth’s axis is tilted 23.5°

    • North end of Earth’s axis always point towards Polaris (The North Star)

    • The Earth’s axis is always pointed in the same direction in space

      • No matter what time of year or time of day.

Seasons

  • What causes seasons?

    • Summer has higher sun angles

      • More intense radiation which causes more warming power than in winter.

    • Summer has longer days

      • The sun is able to warm the earth’s surface for a longer period each day in winter.

  • Northern Hemisphere Summer

    • Sun’s most direct rays are in the northern hemisphere.

    • Latitudes in northern hemisphere are getting longer periods of daylight.

      • Tropic of Cancer is getting more sun rays than a Tropic of Capricorn

  • What about distance of the Earth to the Sun?

  • The Four Seasons

    • Seasons determined by the Earth’s tilt and where earth is in its orbit around Sun.

      • Northern Hemisphere gets maximum radiation (highest sun angles and longest days) in June.

      • Southern Hemisphere gets maximum radiation in December.

  • The Solstices and day length

    • June Solstice — June 21st

      • Beginning of Northern Hemisphere’s summer / Southern Hemisphere’s Winter

        • Days in Northern Hemisphere are longest for the year.

        • Days in Southern Hemisphere are shortest for the year.

        • Northern Hemisphere sun angles are high and Southern Hemisphere sun angles are low.

    • December Solstice — December 21st

      • Beginning on Northern Hemisphere Winter and Southern Hemisphere Summer

        • Days in Northern Hemisphere are shortest for the year.

        • Days in Southern Hemisphere are longest for the year.

        • Northern Hemisphere sun angles are low and Southern Hemisphere sun angles are high.

  • The Solstices and Equinoxes.

09/03/2025 (Lab)

  • How do you know how far east/west you are in the ocean?

    • If you know your local time, looking at the sun.

      • Lets say it’s noon where you are, compare it with time in some other place in the world (prime meridian, Zulu Time)

        • If east of it subtract time

        • If west add time

  • 15° of Longitude is equal to 60 minutes of time.

09/05/2025

The Atmosphere is made of?

  • The atmosphere is a mixture of

    • individual gas molecules

    • Suspended microscopic particles of solid and liquid

    • and falling precipitation

  • How ‘big’ is it?

    • The Earth’s atmosphere is commonly defined as extending to 480 km (300 miles) above sea level.

    • Space is internationally accepted as beginning at the Karman Line-100Km ( 62 Miles). 99.999% of the atmosphere lies below this altitude (1.6% of Earth’s radius).

    • The international space station orbits at about 408KM (254 Miles)

How “big” is the atmosphere?

  • 99% of atmospheric particles are contained in the lowest 30km (18.6. miles) of the atmosphere - or the lowest 6% of the atmosphere’s total height as a whole.

  • However, there is considerable mass contained in the atmosphere: mass contained in the atmosphere: 5.15 quadrillion tons (5.15 × 1018 kilograms). The force of this mass pushing downward on the Earth’s surface is what we call atmospheric pressure.

Atmospheric Gasses

  • Gasses can be exchanged between Earth and the atmosphere (it is a system) through geological or biological processes. So some gasses can vary:

    • Permanent gasses

      • Stable proportion of atmospheric mass.

      • Most common is nitrogen, oxygen, and argon.

    • Variable gasses:

      • proportion varies in time and space

      • most common is water vapor and carbon dioxide.

Composition of Atmosphere near surface

  • Remember:

    • Nitrogen is 78.08

    • Oxygen (round to 21%)

    • Argon is 0.93

  • Remember:

    • Water Vapor is H20V [The little “v” indicates it is water]

      • This is 0% to 4% by volume

        • It is never actually 0%, it gets hella close though

        • Goes up to around 4%

    • Carbon Dioxide 0.400% or 400 parts per minute (400 out of 1,000,000 are carbon dioxide molecules)

Oxygen and Carbon Dioxide

  • Oxygen (O2) is 2nd most abundant gas and is of course required for animals to breathe and convert (oxidize) food into energy.

  • Carbon Dioxide is a very small part (0.4%) of atmosphere, so it is often expressed as parts per million (PPM) - now about 425 PPM (compared to 285 PPM per-industrial level).

Ozone

  • In the upper atmosphere, ozone is created and destroyed due to ultraviolet radiation - which ultimately protects us from harmful UV radiation

    • O2 + UV —> O + O —> O2 + O —> O3

Water Vapor

  • Water Vapor ( water in its gaseous state) is always mixed into our lower atmosphere.

    • Invisible gas. Clouds and fog are actually tiny droplets of water.

    • You can feel humidity on a hot (or even cold) day.

    • Varies in time and space - from 0.2% by volume in cold, dry climates to nearly 4% in humid tropics.

    • Massive source of stored energy.

Aerosols and Particulates

  • Aerosols are tiny solids or liquids suspended in the atmosphere,

    • Sulfur dioxide

    • Smoke

  • Particulates are a kind of aerosol more specific to solid particles

    • Ash, dust, pollen

  • These are important due to their roles in absorption or reflection of energy and formation of precipitation.

Week 3

09/08/2025

Some units of measurement

  • Temperature in °C

    • 0°C = Freezing point

      • Can go a lot lower and go into the negatives for physics

      • On Kelvin Scale 273K° is freezing

    • 15°C = Earth average temperature

  • Meter for length

  • Square meters for area

    • Surface could be 1 meter on the side

      • Total area than would be 1 square meter

    • Area is “A”

  • Cubic meters “m3” = volume “V”

  • Kilograms (Kg) = Mass

  • Mass (m) * Acceleration (a) = Force (F)

    • F(Kg * (m/s)/s) kgms-2 = 1 newton

    • Can measure the force as pressure

Vertical Structure

  • Earth’s surface = 15°C

  • Earth’s atmosphere is divided into four major layers, based on temperature trend from bottom to top:

    • Troposphere

      • Tropopause = -60°C

    • Stratosphere

      • Stratopause = 0°C

    • Mesophere

      • Mesopause = -90°C

    • Thermosphere

      • Upper Thermosphere = >100°C

  • Direction of temperature

    • Negative in troposphere and mesophere

    • Positive in stratosphere and thermosphere.

Change in Density

  • Mass of air, and therefore density both decrease with increasing altitude.

Change in Pressure

  • In the upper atmosphere, less mass results in lower force. So, pressure is lower.

  • Greater mass in lower atmosphere increases force, so pressure is greatest at the sea level.

Troposphere

  • The troposphere is where nearly all weather takes place, primarily due to the presence of nearly all water vapor and atmospheric particulates.

  • Warm at the bottom due to the absorption of sunlight at the earth’s surface.

  • Air temperature decreases with rising altitude.

    • About 6.5°C / 1000m (3.6°F / 1000ft)

    • This is called average tropspheric lapse rate of normal lapse rate.

  • Shallowest of the layers, but about 80% of mass and considerable mixing particularly due to its negative temperature trend and its abundant water vapor.

Tropopause

  • The tropopause is the boundary between the troposphere and the stratosphere.

  • It is located where the temperature ceases to decrease with increasing altitude (Temperature trend becomes isothermal).

    • Average about 11km above sea level.

    • Up to 17km at equator.

    • About 9km at poles.

Stratosphere

  • Air temperature increases with increasing altitude (a positive relationship).

  • Notice that the coldest air in the stratosphere is lowest in elevation - this layer is stratified by temperature.

  • At these upper elevations, most heating is due to the absorption of UV radiation by oxygen and ozone.

  • Ozone maximum is in the lowest sratosphere but most of the warming is at the top, where most UV is absorbed.

  • The stratosphere is more than triple the thickness of the trophosphere but it only accounts for 20% of atmospheric mass.

  • Within the stratosphere lies the ozone layer at about 20-30km.

  • Even at its maximum, ozone only occurs at about 10 PPM, but it protects life from harmful UV radiation.

Mesosphere and Thermosphere

  • Only 0.1% of atmospheric mass is in these two zones combined.

  • In the mesophere most heating comes from the absorption of UV radiation near the stratopause and any remaining heat disperses with altitude (note the decrease in temp with altitude).

  • In the thermosphere, molecules absorb raw sunlight, so they move very fast but are so sparse that high temps are misleading.

  • Heat content includes kinetic energy (speed) and mass.

  • A normal thermometer wouldn’t be able to detect the high temperatures.

09/10/2025 (Absent)

Transfer of energy in the Earth - Atmosphere System

  • Methods of energy transfer

    • Conduction

      • Transfer of heat on an atomic/molecular level by physical contact.

        • Example: making cookies and accidentally touch oven grate and burn your fingers (conduction of heat from the grate to your finger).

    • Convection

      • Transfer of organized flow of molecules and the energy that they contain.

        • Example: Rising columns of warm air on a sunny day.

    • Radiation

      • Transfer of heat by electromagnetic waves

        • Example: Cooking smores on campfire and you toast the marshmallow on the stick, but it cooks without using the fire.

Conduction and Convection

  • Convection

    • Organized movement of molecules and the energy that they contain.

      • Warming air gains heat (expands and rises)

      • Cool air loses heat (contracts and shrinks)

  • Conduction

    • Transfer of heat energy by direct contract of molecules.

      • Heat energy (vibration of atoms) passes from one place to another.

Body Radiates According to Their Temperature

  • Rate of radiation

    • Hotter = faster and more intensive

  • Type of radiation

    • Hotter = shorter wavelengths

Temperature and Heat

  • Temperature

    • Measure of molecule kinetic energy

      • Warm weather is more energetic than cold

  • Measuring temperature

    • Proxy measurement (expression) or molecular motion

      • Kelvin Scale

      • Celsius Scale - water boils at 100°

      • Fahrenheit Scale

  • Heat

    • Energy transfer

      • Example: pan of water on a hot stove, energy goes from the stove, through the pan, and into the water.

      • Heat moves from the warmer object to colder object.

  • Thermal Gradients

    • Rate at which heat flow is controlled in part by the difference in temperature between 2 objects.

      • If 2 objects have larger differences in temperature, and they are close together, thermal gradient is steep, and energy will move fast.

    • Heat moves whenever energy is going from one object to another.

      • Always moves down the thermal gradient (warm to cold)

    • Heat does not move when temperature is the same.

  • Heat Capacity

    • Specific Heat - Amount of heat required to change the temperature of a specific amount of substance by 1°.

      • High Heat Capacity means substance is slow to change temperature, because it takes a lot of heat to increase temperature by 1°.

      • Temperature changes fastest when materials have low heat capabilities.

Earth’s Energy Budget

  • Earth’s Radiation Balance

    • Input 100% - incoming shortwave radiation from the sun

    • 34% - reflected shortwave

      • Planetary Albedo (Reflectivity of the Earth)

    • 66% - Radiated longwave (thermal infrared) from Earth

      • Most terrestrial radiation is absorbed by the Earth’s surface.

    • 47% - absorbed by Earth’s surface

    • 19% absorbed by the atmosphere

Energy Transfers in the Earth-Atmosphere system

  • Radiated Earth is either reflected (scattered), transmitted, or absorbed.

  • Reflected radiation is lost to the system (like it was never there)

  • Transmitted radiation just passes through.

  • Absorbed radiation will raise the temperature of whatever is absorbing it.

09/10/2025 (Lab)

The Scientific Method

  • Hypothesis

    • A hypothesis can fail without being wrong.

      • If the evidence does not support the hypothesis it fails.

        • You can still collect more evidence to make it correct.

    • “Just because your hypothesis wasn’t supported by the evidence, that doesn’t mean it is wrong”.

  • Discussion

    • Where you basically yap/explain.

    • Explain why or why not you’re throwing away your hypothesis.

      • The north should be colder than the south but you might’ve just gotten bad data.

    • Some people may trust their data more than their hypotheses, sometimes they trust the hypothesis more than the data.

    • “How you’re results line up with your hypotheses, and what you expected, and what you got.”

      • You need to put some reasons why your results didn’t line up with your hypothesis. If they did, you still gotta do a discussion to explain why.

    • “Why these results occurred”

  • Analysis of results

    • “What you found”

  • Conclusion

    • “Even though I rejected my hypothesis, here’s what I know to be true”

  • Sharing

    • Starts with peer review

      • Sending manuscript to a journal/publishing house

        • Editor than sends it out to peer review

          • They look at everything

        • Publishers can retract it if they don’t think it is correct

  • Hypothesis

    • A prediction

    • Formal prediction on what you think is going on.

    • If you make one after the experiment is done, it’s either accepted or failed.

      • Test either supported or failed to support hypothesis.

    • YOU WILL NEVER EVER PROVE YOUR HYPOTHESIS

      • Don’t ever use the word “prove” when it comes to your hypothesis.

      • “Nothing is ever proven, not ever, not ever”

  • Theory

    • A conceptual model on how something works

    • Newton’s so called “laws” were laws because the math worked so well.

      • That’s why it became what they call a “law”.

  • Fact

    • Something that is measurable

  • Belief

    • Not measurable

    • “Based on something else”

  • Observation

    • Recorded data

      • Use the data to draw a conclusion

  • Bias

    • Happens when you don’t separate belief and facts

    • Everyone develops bias without realizing.

  • Replicable

    • Needs to be this

  • Fasifiable

    • Most relates to the hypothesis

Week 4

09/15/2025

Latent Heat

  • Water is the only substance that exists in all three states of matter within normal temperature range of Earth’s atmosphere. When water undergoes a phase change, heat is either either released to, or taken from, the environment around it. This is known as latent heat exchange.

  • Heat = Energy when professor is yapping

  • As humans we feel sensible heat, such as a hot 100° day. We cannot feel latent heat, but we can feel the effects of latent heat exchange.

  • If you go into a pool on a hot day and emerge in a nice breeze, your skin feels cool. The air is evaporating water from your skin, which requires energy to be absorbed by the evaporating water. Evaporating molecules require heat, and they get it from your body, leaving your skin cool.

Heat

  • Heat = Energy

  • Types of heat

    • Sensible heat

      • Changes in this register in a thermometer.

      • Heat you can feel

    • Latent Heat

      • Changes occur when water changes state.

      • Heat that you can feel through evaporation. 

  • Energy Absorbed —> Sensible Heat

    • Or —> Latent Heat

    • Primarily Sensible

  • Energy Absorbed by Larol —> Sensible (increased temperature)

    • Or —> Latent Heat

    • Primarily Sensible

  • Energy absorbed by water —> Sensible

    • or —> Latent (evaporation)

      • Most of the energy will go to evaporating water

Latent heats of water

  • Ice to water at 0°C: 90 cal/g

  • Water to water vapor at 100°C: 540 cal/g

  • Water to water vapor of 0°C: 590 cal/g

  • Ice to water vapor at 0°C: 670 cal/g

Outline

  1. Latitude

  2. Land/sea distribution

    1. Water heats slowly, and cools slowly.

    2. It stores huge quantities of heat nearby coastal lands thus maintain a near constant temperature - moderate summer, moderate winter.

    3. Why does water moderate temperatures?

      1. Heat capacity of water is greater than that of land - more energy is required to heat 1 gram of water by 1°C.

      2. Water is transparent: energy can spread through a greater volume of water.

      3. Water mixes constantly, transferring heat within it.
        water is constantly evaporating and thus cooling.

  3. Ocean currents

    1. Continental Temperatures are much more extreme than maritime temperatures.

    2. Maritime summers are cool, but their winters are mild.

    3. Compare winter temperature in Minneapolis (-4°F) with those in Seattle (40°F)

    4. Surface ocean currents transfer warm water from low to high latitudes and cold water from high to low temperatures.

    5. Ocean currents move in GYRES (specific large currents that circulate water) within a basin, pushed by the surface winds. 

    6. Cold currents cause air temperatures above them to be lower. Nearby coastal regions are likely colder. An example is the California Current, or the Peru Current. 

    7. Warm currents cause air temperatures above them to heat up. Nearby coastal regions might be warmer and more humid. An example is the Gulf Stream-North Atlantic Drift. 

  4. Elevation

  5. Land form barriers

  6. Human activities

Temperature Distribution at Earth’s surface

Annual Temperature Changes

Vertical Temperature Patterns

09/17/2025

Outline

  • Controls of Earth’s Surface Temperatures

    1. Latitude

    2. Land/sea distribution

    3. Ocean currents

    4. Elevation

      1. With the troposphere temperatures decrease with increasing altitude or elevation.

      2. We can see the impact of this in snow-capped mountains, including those found at and near the equator.

      3. The 5 Peruvian cities below are all at 15°S. Mean daily temperature decreases as elevation as elevation increases, while temperature range increases.

    5. Land Form Barriers

    6. Human activities

  • Temperature distribution at Earth’s surface

  • Annual Temperature Changes

  • Vertical Temperature Patterns

Isotherms

  • Isotherms are lines of equal temperature.

    • Each place on the line has the same temperature.

    • Look for steep temperature gradients or closely-spaced lines.

    • Look for gentle temperature gradients or widely-spaced lines.

    • Temperature varies with latitude: why?

      • The further you are from the equator the colder it becomes. 

Geographical Temperature Patterns at Earth’s Surface

  • Isotherms are shown: lines of equal temperature

    • Each place on the line has the same temperature

    • Look for steep temperature gradients or closely-spaced lines.

    • Look for gentle temperature gradients or widely-spaced lines.

  • Temperature varies with latitude: why?

  • Average temperatures adjusted for elevation by adding 6.5°C for every 1000 meters of elevation (i.e. temperatures are adjusted to sea-level equivalent)

  • Maps show January and July to represent seasonal extremes of temperature, after a lag of 30-40 days beyond each solstice.

Summary of Seasonal Temperature Maps 

  • Isotherms show impacts of latitude & seasonality.

  • Steepest temperature gradients occur in the winter hemisphere.

  • Continental extremes of temperature: warmth moves pole-ward in summer, cold moves equator-ward in winter.

  • Steeper temperature gradients are found on east coasts in winter, west coasts in summer.

  • Ocean currents are apparent: warmer on east coasts, cooler on west coasts.

  • Southern hemisphere is the “water hemisphere” - so there is less variation in temperature.

Temperature lag means that peak warmth or peak cold is delayed after the respective solstice, especially over water.

The Normal Lapse Rate.

  • We have already seen that the temperatures of the atmosphere change with elevation. These rates of change are called lapse rates.

  • The average rate of temperature change in the troposphere is the normal lapse rate, and it amounts to 6.5°C/1000m. 

    • Remember that number.

  • By convention, we usually leave off the negative sign, but remember that the normal situation in the troposphere is cooling with increasing altitude.

Temperature Inversions.

  • A temperature inversion is when the temperature increases with altitude rather than the normal trend of decreasing with altitude.

  • Inversions cause at ground level are called surface inversions

    • Upper level inversions are anything above the ground level. 

Types of Inversions: A Summary

  • Surface

    • Radiation: Radiational cooling at night. 

    • Topographic: Cool air is heavy, and flows to low elevations like valleys. 

    • Advection: Cool air blows in from another location and displaces warmer air above the incoming cold air. 

    • AT THE GROUND LEVEL

  • Upper Air

    • Subsidence: Sinking air warms by compression. 

    • ABOVE GROUND LEVEL

09/19/2025

Pressure.

  • Pressure is defined as a forced applied over an area, for example, pounds per square inch.

  • Air pressure is the weight (force) of air above a surface (area).

  • In the metric system we use a force unit of newtons per square meter of area (1N/m2 = 1 pascal).

  • Sea-level pressure is 101,325 Pa, which is equal to 1013.25hPA [Pa = Pascals] (or mb).

  • Pressure is the weight of molecules above some level in the atmosphere.

Atmosphere Pressure.

  • Notice how altitude affects air pressure:

    • Higher in the atmosphere there are few molecules above us, therefore the pressure goes down in that direction.

    • Lower Altitudes = higher pressures.

  • Notice also that air density and air pressure have the same shape when graphed against altitude:

    • Density is defined as the amount of mass in a volume of space, like kilograms per cubic meter.

    • Higher pressures mean higher density of molecules.

Discovering Air Pressure.

  • It has long been known that water can be sucked up a tube, as a siphon, but only so far (33 feet).

  • In 1643, Evangelista Torricelli, a student of Galileo, came up with a hypothesis: the weight of the atmosphere is equal to the weight of a 33 feet column of water.

  • Torricelli did an experiment with mercury, and predicted that it would rise to only 2.5 feet (because it is 13.6 times denser than water (33/13.6 = 2.5)).

    • Mercury is a lot denser than water.

  • He was right: The mercury only rose to a height of 0.76 meters (=2.5 feet/3.28ft/m).

  • Because his tube was sealed at the top and open on the bottom, it could only be air pressure that was supporting the mercury column.

  • French mathematician and physicist, Blaise Pascal, put Torricelli’s hypothesis to a further test in 1648. He had his brother-in-law carry a mercury barometer up a mountain to see if the level of mercury in the column fell.

  • It did, confirming Torricelli’s idea that the weight of the overlying atmosphere was balancing the weight of mercury in the tube.

Measuring of Air Pressure.

  • Average Air Pressure at Sea Level

    • 14.7 lbs/inch2

    • 29.2 inches of mercury (Hg)

    • 760 mm Hg

    • 101,325 Pa (1 Pa = 1 N/m2)

    • 1013.25 hectopascals (hPa)

    • 1013.25 millibars (mb)

Variations in Surface Air Pressure

  • Air pressure on the earth’s surface varies according to:

    • Elevation/altitude

      • Higher locations have lower pressure

      • Maps of atmospheric pressure are adjusted so that all locations are mapped as if they were sea-level

    • Vertical motion (convection)

      • Rising air causes low pressure

      • Subsiding air cases high pressure

When we look at weather maps, the effect of elevation has been taken into account, so the only thing that is affecting pressure is vertical motion.

Week 5

09/22/2025 (Absent).

What causes Vertical Motion of Air?

  1. Thermal causes (action is at the earth’s surface)

    1. Warm air expands, becomes less dense and rises.

    2. Cold air contracts, becomes more dense and subsides (sinks).

  2. Dynamic causes (action is aloft — near the troposphere)

    1. Diverging air high above the surface (aloft) causes air to be lifted or to rise.

    2. Converging air aloft causes air to subside.

Thermally-induced Pressure Variations.

  • Warm surfaces cause air to expand.

    • When air expands, it becomes less dense, and so it rises.

    • Rising air always creates surface low pressure.

  • Cold surfaces chill air and causes it to become more dense, so it sinks.

    • Subsiding air always produces surface high pressure.

Dynamically-induced Pressure Variations.

  • Divergence aloft causes air below to rise.

    • Rising air always creates surface low pressure.

  • Convergence aloft pushes air downward to the surface.

    • Subsiding air always produces surface high pressure.

Cells of High and Low Pressure.

  • Whenever air converges at the surface it is also rising.

    • Rising air creates low pressure and is associated with cyclones.

  • Whenever air subsides, it causes divergence at the surface.

    • Subsiding air creates high pressure and is associated with anticyclones.

Mapping Pressure Distributions.

  • Maps of surface air pressure use lines of constant pressure, called isobars, to depict the pattern of surface air pressure variations.

  • A pressure gradient occurs when pressure changes across a distance. Air always moves down pressure gradients - away from highs and toward lows.

  • A center of high pressure is called an anticyclone.

  • Air is not only sinking in the anticyclone, but it is also diverging away from the center of high pressure.

  • A center of low pressure is called a cyclone.

  • Air is converging toward the middle of low pressure as it rises.

Cyclones and Anticyclones.

  • Air in the vicinity of the high pressure center is subsiding. All high pressure centers are called anticyclones.

  • Air near a low pressure center is rising. All low pressure centers are cyclones.

Pressure Gradients.

  • A pressure gradient is the change of pressure per unit distance (e.g. mb/100km).

  • Pressure gradients are “steep” when there is large change in pressure per unit distance.

  • Cyclones are often zones of steep pressure gradients, while anticyclones always have shallow gradients.

Pressure and Altitude.

  • We can think of altitude in terms of pressure.

Wind.

  • Wind is the horizontal motion of air.

  • Wind has speed and direction.

  • Wind speed varies according to the steepness of a pressure gradient, which is the difference in pressure per horizontal distance (e.g. ∆P(hPa)/100km).

  • Wind direction is the combined result of two things:

    • Direction of the pressure gradient (always perpendicular to isobars and from higher to lower pressure).

    • Coriolis deflection due to earth’s rotation.

09/24/2025

Wind.

  • Wind is the horizontal motion of air.
    Wind has speed and direction.

  • Wind speed varies according to the steepness of a pressure gradient, which is the difference in pressure per horizontal distance.

  • Wind direction is the combined results of two things:

    • direction of the pressure gradient (always perpendicular to isobars and from higher to lower pressure)

    • Coriolis deflection due to earth’s rotation.

Wind Speed.

  • Wind speed is a direct results of the steepness of the pressure gradient.

Wind Direction.

  • On a non-rotating earth, wind direction would simply be the most direct path from high pressure to low pressure, that is, straight down the pressure gradient.

  • However, because the earth rotates, our frame of reference for direction is also rotating.

  • This means that what appears to be a straight line when seen from an observer in space is a curved path for us on earth.

  • This is turning from a straight line to a curved path is called the Coriolis Effect.

Coriolis Effect.

  • When see from above the North Pole, the earth is rotating counterclockwise, but when viewed from above the South Pole, the earth is rotating clockwise.

    • Northern Hemisphere = counterclockwise

    • Southern Hemisphere = clockwise

  • This means that the Coriolis deflection is to the right in the Northern Hemisphere, and to the left in the Southern Hemisphere.

  • The dashed arrows show the direction of the pressure gradient (the “intended” direction of the wind).

  • The solid arrows show the actual direction due to Coriolis.

  • Notice:

  1. The amount of deflection increases with latitude so…

  2. …There is a maximum deflection at the Poles and …

  3. …Zero deflection on the equator.

Coriolis Effect: Know these four rules.

  • The direction of Coriolis deflection is determined by hemisphere:

    • Northern/rightward

    • Southern/leftward

  • The maximum of Coriolis deflection is determined by latitude:

    • Maximum at the poles

    • Zero at the equator

    • Coriolis increases with latitude

  • Coriolis effect also increases with wind speed.

  • Finally, Coriolis always acts at right angles to the wind direction: if the wind is blowing, Coriolis is always “trying” to deflect it to the left or right.

The Coriolis Force.

  • Coriolis is just as often referred to as a “force” as it is an “effect”.

  • For those of you who appreciate equations, here is the equation for computing the magnitude of the Coriolis Force.

    • CF = -2Ωsinφ V

      • Where Ω is the rate of the earth’s rotation in radians per second (its constant, so you can ignore this for our purposes)

      • φ is the latitude in degrees

      • and V is the velocity (speed) of wind in meters per second.

Wind Speed and Direction: A Summary.

  • Wind speed is dictated by the steepness of the pressure gradient (i.e. the spacing of isobars on a pressure map).

  • Wind direction is a combination of:

    • The direction of the pressure gradient

    • The amount and direction of deflection (left or right) due to Coriolis.

    • Coriolis deflection is in turn controlled by:

      • Wind Speed

      • Latitude

  • Notice in the list above, how the pressure gradient controls wind speed, and then wind speed determines the amount of Coriolis deflection. Let’s pursue that idea…

Geostrophic Balance.

  • The initial tendency of the air is to move down the pressure gradient.
    However, as soon as it moves, it is deflected away from that path by Coriolis.

  • In the Northern Hemisphere, the air incurs a rightward deflection until it is moving at right angles to the pressure gradient.
    This wind resulting from this balance is called geostrophic flow. It results from the pressure gradient form and the Coriolis force being exactly balanced when the wind is flowing parallel to isobars.

Finding Geostrophic Wind Direction: Three Easy Steps.

  • Find the direction of the pressure gradient from higher to lower pressure.

  • Turn to the right for the Northern Hemisphere (Left for the Southern Hemisphere).

  • When the wind is parallel to isobars, the flow is geostrophic.

Effects of Friction.

  • Geostophic flow is actually never quite achieved, but it almost is at high altitudes.

  • Two things prevent pure geostrophic flow:

    • Friction

    • Curvature of isobars.

    • Both of these are most important near the surface of the earth, but friction in particular.

  • You will remember that the strength of the Corioilis Force is dependent on wind speed.

  • Friction slows the wind, and therefore Coriolis Force is reduced. The pressure gradient, however is not affected.

    • Notice how the wind now will cross isobars where geostophic wind never would.

Geostrophic flow in the upper trophosphere.

    • The red arrows in this diagram show the direction, and they are sealed to be longer where the pressure gradient is steeper as in the NE part of the map.

    • Geostrophic winds are the green arrows. Notice how they are also scaled to indicate wind speead according to their length.

      • These arrows are called vectors, and they show magnitude and direction at each point represented by the center of each circle.

Geostrophic wind compared to frictional wind.

    • This map is the same as the last one, except that the pressure arrows have been removed, and the friction arrows have been added.

    • The green arrows show wind without friction, and the black arrows show slower winds, now crossing isobars toward lower pressure.

How to determine wind direction on any pressure map.

  • Look for areas of higher pressure and lower pressure. The pressure gradient will be perpendicular to isobars, and pointing toward lower pressure.    

  • Imagine an arrow pointing down on the pressure gradient. 

    • Now turn the arrow to the right (if this is a place in the northern hemisphere) until the arrow is parallel to the nearby isobars. This is the geostrophic wind. 

  • If this is a surface map, there is friction to consider. Take your geostrophic wind arrow and turn it slightly (about 30°) toward lower pressure. 

09/24/2025

  • Use cos(x) to solve circumferences of latitudes

    • cos(60°) = 0.5

      • 0.5 * [Earth’s circumference] 40,000km

        • 20,000 km is the circumference at 60° latitude

Week 6

09/29/2025

A few words about wind terminology.

  1. Winds are always named for where they come from, usually a direction.

  • Wind from the north is a north wind or northerly

  • A wind from the south is a south wind or southerly.

  1. If a shoreline or a slope faces into the wind, then it is windward.

  2. If it is a side facing away from the wind, then it is leeward.

  3. Winds that dominate from a particular direction are called prevailing winds.

  • For example, we live in a zone of prevailing westerlies, meaning that most of the time the winds come from somewhere out of the west.

  • In the tropics, the winds are prevailing easterlies: the Trade winds.

Circulation around northern hemisphere low pressure.

  • Notice the circulation patterns around the northern hemisphere (low pressure):

    • Counterclockwise and converging towards the center.

  • Remember 1-2-3 rules for determining wind direction:

    • (1) Point down the pressure gradient.

    • (2) Turn to the right (Geostrophic wind)

    • (3) Back off about 30° (surface wind)

Circulation around northern hemisphere high pressure.

  • Notice the circulation patterns around the northern hemisphere (high pressure)

    • Clockwise and diverging away from the center.

  • In the northern hemisphere:

    • Clockwise is anticyclonic (highs)

    • Counterclockwise is cyclonic (lows)

Facts about centers of low pressure.

  • The are zones of rising air.
    They are associated with clouds and precipitation.

  • They are cyclonic.

  • They are centers of convergence at the surface.

  • They are associated with divergence aloft.

Facts about centers of high pressure.

  • They are zones of subsiding air.

  • They are associated with clear skies and calm weather.

  • They are centers of divergence.

  • They are associated with convergence aloft.

Circulation around centers of high and low pressure. 

  • Around high pressure, circulation is said to be anticyclonic.

  • Around low pressure, circulation is said to be cyclonic.

  • In the northern hemisphere, cyclonic is counterclockwise; anticyclonic is clockwise.

    • Southern hemisphere

      • Cyclonic is clockwise

      • Anticyclonic is counterclockwise

Ridges and troughs. 

  • These are places where pressure reaches a high (ridge) or low (trough) in a zone that does not quality as a center of high or low pressure.

Ridges. 

  • The pressure goes down on both sides of the ridge.

  • The ridge marks a line of relatively high pressure in between two lows.

  • Just as with any zone of high pressure, a ridge is a zone of divergence and subsidence.

Troughs.

  • The pressure goes up on both sides of the trough.

  • The trough marks a line of relatively low pressure in between two highs.

  • Like any zone of low pressure, a trough is also a line of convergence and rising air.

Cyclones.

  • Vertical direction of air is rising or upward.

  • Centers of low pressure.

  • Rotation is counterclockwise in Northern Hemisphere.

  • Rotation is clockwise in Southern Hemisphere.

  • Horizontal direction of flow is converging or inward to center.

Anticyclones.

  • Vertical direction of air is subsiding, descending, or downward

  • Center of high pressure

  • Rotation is clockwise in northern hemisphere.

  • Rotation is counterclockwise in southern hemisphere.

  • Horizontal direction of flow is diverging or outward from center.

10/01/2025

Jet Streams.

  • Subtropical Jet (STJ)

    • Located above the STH

    • Zone of convergence aloft

  • Polar Front Jet (PFJ)

    • Located above the polar front

    • Produced by steep Pg aloft (200-300mb level)

Upper level winds and jet streams

  • Pressure gradient aloft is controlled by air temperatures: warmth in tropics; cold in polar regions.

  • Warm air = high pressure aloft

  • Cold air = low pressure aloft

10/03/2025

Jet Streams.

  • Subtropical Jet

    • Located above the STH

    • Zone of convergence aloft

  • Polar Front Jet

    • Located above polar front

    • Produced by steep Pg aloft (200-300 mb level)

Upper Winds and Jet Streams

  • Pressure gradient aloft is controlled by air temperatures: warmth in tropics; cold in polar regions.

  • Warm air = high pressure aloft

  • Cold air = low pressure aloft.

  • Kansas has clear skies in the powerpoint photo

Week 7

10/06/2025

Principal monsoon areas of the world

  • Monsoons are seasonal reversing wind systems.

  • They are most well developed in the vicinity of large continental land masses.

Maximum Poleward Positions of the ITCZ

  • Large continents also cause the ITCZ to migrate far from the equator during the summer season in each hemisphere.

  • Typical maximum poleward positions of the inter tropical convergence zone at its seasonal extremes.

  • The greatest variation variation in location is associated with monsoon activity in Asia and Australia.

  • We are focusing on the Eastern hemisphere since our action on the western hemisphere isn’t as strong.

December - February

  • Northeast trade winds bring stable, dry conditions to southern Asia during the winter months.

  • It is very cold in central Asia during the winter.

  • Asia does have a very dry winter though. 1=

June - August

  • Wet summer monsoon

  • Summer rains are brought to Southern Asia by the Equatorial Westerlies. Note the extreme latitudinal position of the ITCZ during the summer monsoons.

Monsoon Precip in India

  • Sudden onset and a more gradual end of summer monsoon rains.

African Monsoon System

  • Very unstable and rainy winds.

  • Drops a lot of the precipitation on the coast than decreases the more central Africa you go.

  • In the winter time

    • Wind coming from the north east (no water coming from that direction)

    • No water coming from the Middle East, no moisture.

    • Around 30° S is very dry because that belt of latitude is typically very dry.

    • NE trade winds during the winter.

Northern Australia Monsoon

  • Summer

    • North west trade winds

    • Equatorial north westerlies bring rainy summer.

  • South

    • South easterlies trades bring dry weather in winter.

Sea and Land Breezes

  • Sea Breeze

    • In the afternoon, the land is warmer than the ocean surface, and warm air rising from the land is replaced by an onshore sea breeze.

  • Land Breeze

    • At night, as the land cools, the air over the ocean is now warmer than the air over the land.

    • The ocean air rises. Air flows offshore to replace it, generating an offshore flow (a land breeze).

Valley and Mountain Breezes

  • Valley Breeze

    • Air rises from the valley up warm slopes.

  • Mountain Breeze

    • Air cools and flows down from the mountain peaks.

    • Any cold, dense, down-slope wind is called a katabatic wind.

Chinook Winds

  • Wind blows against a mountain range.

  • Air is forced up windward slopes, causing condensation and precipitation.

  • Latent heat is released and becomes sensible during condensation.

  • This warms the air on the leeward sides.

  • Leeward slopes are warm and dry.

Principle Ocean Currents.

  • North Atlantic

    • Gulf Stream

    • North Atlantic Draft

    • Canary

    • North Equatorial

  • South Atlantic

    • Brazil

    • Benguela

    • South Equatorial

  • North Pacific

    • Kuroshio (Japan)

    • North Pacific Drift

10/08/2025

The Water Cycle

In a single minute, through precipitation or condensation, the atmosphere gives up more than a billion tons of water, and an equal amount of water evaporates and sublimates back to the atmosphere as water vapor.

Heat involved with changes of state of water.

  • Talking about in lab today

  • Focusing on liquid to gas and than gas to liquid.

The Hydro Logical Cycle

  • Follow the energy

    • Solar energy is absorbed by water molecules.

    • Water uses that energy to become water vapor, and water vapor carries the energy into the atmosphere as latent heat.

    • Water vapor condenses as the air cools, so it releases the latent heat as sensible heat into the atmosphere.

    • The atmosphere loses sensible heat by radiation IR (long wave) to space.

Humidity

  • What is it?

    • Its source is evaporation from the earth’s surface.

    • It is limited in amount by air temperature (primarily).

  • What controls it?

  • How do we measure it?

    • Actual measures

    • Relative humidity

    • Proxy measures

      • Dew point temperatures

      • Wet bulb temperatures

Water vapor

  • Is a gas

  • Percent by volume

    • varies from 0 to 4 percent

Definitions

  • An air parcel

    • has known volume, pressure, temperature and density

  • Humidity

    • The amount of water vapor in an air parcel at a particular time and place

  • Vapor is a gas in air, just like other atmospheric gases.

  • Air parcels can only contain a certain amount of water vapor - their capacity for vapor is determined by temperature.

    • Warm air has more rapidly moving molecules, so has low density and high volume compared to cold air - thus is has more “space” for water vapor molecules - it has a high capacity for vapor.

      • We say warm air has a high capacity for water vapor

        • Has a lot of room for water vapor

    • Cold air has high density and low volume, so less room and a low capacity for vapor.

      • Can’t hold very much water vapor, has a low capacity for water vapor.

      • “Low capacity for water vapor”

  • If moisture is available, vapor content will be higher in warm air than in cold air.

  • Saturation is reached when air has reached its maximum capacity of vapor.

  • Saturation capacity increases as temperature increases, as seen in the saturation curve.

    • “As temperature goes up capacity goes up”

Air Parcels

  • Think of air parcels as containers of air with invisible walls.

  • Air molecules occupy the space, and their kinetic energy is known by their temperature: faster molecules mean a warmer air parcel.

  • Faster air molecules would also exert more force on the walls of the container, so that means that the pressure is greater, because pressure is the cumulative force of molecules per unit area.

  • Molecules has mass, so the mass of molecules in a volume is what we call density.

  • So we characterize any air parcel by its: (When professor is asking for the air parcel below is what he wants)

    • Volume (V)

    • Temperature (T)

    • Pressure (p)

    • Density (m/V = p)

      • p = greek letter rho

How do we measure humidity?

  • Actual measures

    • Vapor pressure, e(mb)

    • Vapor pressure measures the contribution of water vapor molecules to total atmospheric pressure.

    • It is measured in millibars (or hectopascals) just like any other gas pressure.

    • They curve (class example) represents the maximum vapor pressure (i.e. saturation vapor pressure) at various temperatures.

  • Mixing ratio, w (g/kg)

    • The mixing ratio, w, is the mass of water molecules per kilogram of dry air.

      • Water Vapor (g) / dry air (kg)

    • w is the mix of water with the non-water portion of an air parcel

  • Specific humidity (q, g/kg)

    • q is the mass of water vapor per kg of air (including the water vapor).

  • Vapor Density, pv, (g/m3)

    • Vapor density is the grams of water vapor in a cubic meter of air.

    • p with a “v” subscript will represent water vapor.

  • Relative humidity, RH (%)

    • Actual humidity content / capacity at current air Temperature (x100)

      • REMEMBER

Week 8

10/15/2025

Review

  • Dry Bulb Temperature, T (°C):

    • The ambient temperature of the air.

  • Dew Point Temperature, Td (°C):

    • The temperature to which air must be cooled to produce condensation.

  • Wet Bulb Temperature, TW (°C):

    • The coolest temperature that can be achieved due to evaporation of water into the air.

Getting air to its dew point

  • To bring air to its dew point temperature, it must be cooled to the point where its capacity equals its vapor content.

  • Drier air must be cooled more than air with a higher vapor content.

Two ways to cool the air

  1. Remove sensible heat from the air

  2. Increase its volume (exchanged sensible heat for work).

  • Remove heat:

    • This is a diabetic process because it involves a change in the heat content of an air parcel.

  • Increase its volume:

    • This is an adiabatic process because there is no change in the heat content of an air parcel. Energy just changes form from thermal to work.

Adiabatic Cooling

  • When an air parcel rises, the pressure around it is reduced.

  • This lower pressure allows the air parcel to expand.

  • The work of expansion is taken from the thermal energy of the molecules, and so the temperature goes down.

  • The air parcel is cooler, but it still has the same amount of heat as before.

Adiabatic Warming

  • When an air parcel descends, the air pressure around it increases.

  • This higher pressure squeezes the air parcel into a smaller volume.

  • The work done by compression adds to the thermal energy of the molecules, and so the temperature goes up.

  • The air parcel is warmer, but it still has the same amount of heat as before.

Amount of lifting and cooling to LCL

  • When vapor content is high, dew point temperature is high: T and Td are close together.

    • Such an air parcel might be lifted and cooled to dew point temperature easily.

  • When vapor content is low, dew point temperature is low: T and Td are far apart.

    • Such an air parcel would have to be lifted a long distance to cool by this many degrees. It may never reach saturation if lifting is insufficient.

Lapse Rates

  • A lapse rate is the rate of temperature change with altitude.

  • Lapse rates take the form of: ∆T/∆z

    • Units are C°/1000m (or °F/1000feet)

      • Up is cooler

      • Down is warmer

Two Types of Lapse Rates

  • Environmental:

    • Rate of temperature change with altitude in the troposphere. The ELR is measured with altitude in the troposphere. The ELR is measured with a weather balloon. The average environmental lapse rate is 6.5°C/1000m.

  • Adiabatic:

    • Rate of temperature change for a vertically moving air parcel due to its change in volume. The ALR is not measured, but calculated based on thermodynamic principles.

Lapse Rate Terminology

  • High (Or steep lapse rates)

    • High to low at a steep slope

  • Low (Or small lapse rates)

    • High to low at a lower slope

  • Isothermal (Or no lapse rates)

    • No slope, straight vertical line

  • Inversions

    • Low to high line (increasing slope, not decreasing)

Adiabatic Lapse Rate Changes at the Lifting Condensation Level

  • When unsaturated air is lifted:

    • it initially cools at the DALR (the dry rate)

    • if lifted enough it will reach its level of condensation (LCL)

    • further lifting will cause condensation and cooling will be at the wet (saturated) rate

10/17/2025

Stability Defined

  • Stability is the dgeree to which an air parcel resists vertical motion.

  • Buoyant air parcels will rise. They are unstable.

  • Buoyancty results from the air parcel being less dense than the surrounding air, and so it rises.

Buoyancy

  • Buoyancy is caused mainly by temperature difference between the air parcel and the surrounding air.

    • If the air parcel is warmer than surrounding air, it is less dense, and it will rise.
      If the parcel is the same temperature of the surrounding air, it has the same density, and so it will remain in place.

    • If the parcel is colder than the surrounding air, it will be more dense and sink.

Stable Air

  • When the air is stable, skies and generally clear, or the clouds that do form are flattened.

Unstable Air

  • When the air is unstable, clouds tend to build upward, and often precipitation will be the results.

Assessing Stability

  • To assess stability, we need to know about the environmental lapse rate (ELR).

  • The ELR changes during the day and from place to place, so weather balloons must be sent up frequently so that it can be measured.

  • Once we know the ELR in an area, then we can find out the stability of the atmosphere in that area.

  • Compare the ELR to the Adiabatic lapse rate

    • Remember the ELR is the temperature profile of the troposphere at a particular place and time.

    • The ALR measures the temperature change of a rising air parcel, and is either 10°/km (DALR) or the WALR (~5°/km), depending on whether the position is below of above the LCL.

Stable Air

  • If the ELR shows a relatively slow change in temperature with altitude compared to the adiabatic lapse rate, the air is stable.

  • Under these conditions, if an air parcel is forced upward, it will immediately be colder than the surrounding air.

  • If it is colder, it is more dense, and it resists upward motion.

Unstable Air

  • If the ELR shows a relatively fast change in temperature with altitude compared to the adiabatic lapse rate, the air is unstable.

  • Under these conditions, if an air parcel is forced upward, it will immediately be warmer than the surrounding air.

  • If it is warmer, it is less dense, and once nudged upward, it continues to rise.

Conditional Stability

  • Having water vapor and an ELR that is intermediate between the DALR and the WALR can create conditions of conditional stability.

  • Notice here that the DALR is steeper than the ELR, but the ELR is steeper than WALR.

All Lapse Rates Compared

  • Stability is determined by the ELR with respect to adiabatic lapse rates.

  • When the ELR is steeper than adiabatic conditions are unstable.

  • When the ELR is low or positive, conditions are stable.

  • Test Question: About conditional stability, where are the environmental lapse rates have to be?

    • Between dry and wet

Increasing Instability

  • A steeper ELR creates more unstable conditions. This happens because:

    • There is cooling aloft and/or

    • warming at the surface (which usually happens during the day ).

  • Remember that addition of water vapor also makes air more unstable.

Increasing Stability

  • Warming aloft increases stability by reducing the amount of cooling with altitude. This happens when air is descending in regoins of high pressure.

  • An inversion is a more extreme version of this.

  • Cooling at the surface stabilizes the air. Cold air at the surface has no tendency to rise.