The Final Flashcards
Weather
The state of the atmosphere at a given time and place.
Climate
The sum of all statistical information about weather in a place or region.
Climatology
Allows for the study of atmospheric processes and their impact beyond present-day weather.
Three properties of climatology
Extremes, normal, and frequencies.
Vertical structure of the atmosphere
spheres are separated by pauses marked by a change in the vertical gradient of temperature, either causing a reversal of cooling or warming with height.
Modern Composition of Atmosphere
78% Nitrogen (N), 21% Oxygen (O), 1% Argon (A)
Constant Gases
relatively long residence times in the atmosphere. Includes Nitrogen, Oxygen, Argon, and Helium
Variable Gases
Changes in quantity from place to place and over time. The most common are water vapor, carbon dioxide, and Ozone.
The Atmosphere (general)
Made up of thin gaseous veil surrounding Earth.
Held down by the force of gravity.
Includes essential gases needed for life.
Hydrosphere
Where all of Earth’s water flows and is stored
Water in this sphere exists in three states: gas, liquid and solid.
Lithosphere
Earth’s crust and portion of the upper mantle directly below the crust form this sphere.
Biosphere
The living portion of Earth’s surface
Aka “ecosphere” exists wherever life is sustained.
Two protective layers of atmosphere
Ionosphere - Extends through the thermosphere, absorbing gamma rays and x-rays, changes ions to atoms, where the Northern Lights are.
Ozonosphere - portion of the stratosphere that contains increased levels of ozone. Ozone absorbs certain wavelengths of ultraviolet radiation.
Troposphere
Lower portion
Temperature decreases with height.
75% of atmospheric mass
Nearly all water vapor and aerosols
Deeper in tropics: Shallow at poles
All-important weather phenomena
Thickest around equator
Stratosphere
Above the troposphere
properties of air are independent of turbulence
concentration of ozone
ozone absorption of UV radiation heats the stratosphere
higher temperature results
Mesosphere
Coldest
Thermosphere
High temps but very low pressure
O2 and N2 absorb solar shortwave energy.
So little atmosphere that you do not feel heat, low heat content.
Atmospheric Conditions
Air is a mixture of discrete gases.
O2 and N2 make up 99% of atmosphere - largely irrelevant to weather conditions.
CO2 present in minute amounts
CH4 present in even more minute amounts.
Both CO2 and CH4 concentrations have risen in recent centuries.
Rising Greenhouse gases
CO2 is 1.21 times more abundant than in the 1960s.
CH4 is 1.5 times higher than in 1750 from 700 to 1745 ppb. CH4 rise has recently slowed: 200 ppbv/decade in 70s, 0-130 ppbv/decade now.
Still, CH4 is more potent than GHG, 20x the CO2 effect.
Warming from a 20% rise in CO2 is like a 1% rise in CH4.
Water Vapor
Near 0-4% by volume
Source of all clouds and precipitation
Hugely important for heating the atmosphere.
Its change of phase from solid to liquid to gas or releases heat without temperature change.
The latent is moved with water and is a critical energy source that drives storms.
Aerosols
Ejected and suspended particles, transported by atmospheric motions and kept aloft.
Insolation and Heating
More than 99.9% of the energy that heats Earth’s surface comes from solar radiation
Not evenly distributed, varies with latitude, time of day, and season of year.
Unequal heating of Earth results in winds, and ocean currents which in turn moves heat from the tropics to the poles.
Energy
Capacity to do work.
Kinetic - motion
Potential - stored kinetic
Temperature
how warm to a relative standard
formally: the average kinetic energy of the molecules of some object
When an object gains energy, molecules speed up.
temperature either rises or there is a change in state.
Heat
transfer of energy into or out of an object because of the temperature difference between an object and its surroundings
Flows from high to low until equal
heated objects take on internal energy, typically as molecules increase.
Mechanisms of heat transfer
Conduction
Convection
Radiation
Conduction
Direct transfers between molecules in contact
Objects can be good or bad conductors’ metals and stones are good: wood and air are poor.
Here, only active for contact of Earth’s surface and air just above
Convection
transfer involving the movement or circulation of a substance.
fluids flow and carry heat with their motions.
convection cells in boiling water
thermals used by hawks, vultures, and hang-gliders
Radiation
emission and propagation of energy in the forms of waves or particles and through some material or space
does not require medium to travel
spread across a wide range of electromagnetic spectrum, waves of different sizes
short waves are more energetic and potentially damaging, solar radiation is a shortwave radiation
Laws of radiation
- All objects emit unless at absolute zero
- hotter objects emit more energy
- hotter objects emit in shorter wavelengths
- good absorbers are good emitters
Planck’s Law
all objects above absolute zero emit radiation over various wavelengths
spectrum of radiation depends on temperature.
Stefan-Boltzmann Law
Intensity of radiation increases with temperature.
What happens to incoming solar radiation?
- Absorbed: molecules vibrates faster, temp. increases
- Transmitted: passes through the object
- Redirected: reflection or scattering
Reflection is bouncing back at the same angle and intensity.
Scattering weakens the rays in different directions.
Albedo
The fraction of radiation that is reflected off an object.
Varies in wavelength.
Total planetary albedo in the shortwave portion of the spectrum includes reflection from the surface of the Earth plus reflection off clouds and the atmosphere itself.
Varies widely for different surfaces.
What happens to sunlight when it strikes Earth?
some are absorbed by the outer atmosphere.
some make it through the troposphere.
parts bounce back to space.
part is absorbed by the atmosphere and clouds.
part heats the surface.
Earth-sun Relations
Sun angle varies by latitude because Earth is spherical
The larger the solar angle, the more intense the insolation
Motions causing variations in solar radiation
rotation - Earth spinning about its axis, causes the daily cycle
revolution - movement along an orbital path around the sun - causes seasons
tilt - seasonal variations of heating
Solstices
When earth’s axis tilts towards or away from the sun
Equinoxes
When earth’s axis tilts neither toward nor away from the sun
Elliptical orbit
Sun is not centered
plane of elliptical: flat plane on which the Earth travel as it revolves around the sun.
Aphelion
July 4th - Earth is the farthest distance from the sun
perihelion
January 3rd - Earth is the closest distance from the sun
Solar noon
the time of the day when the sun is at its highest position in the sky
Isotherm
a line that connects points on a graph that have the same temperature
Isotherm Contour Map show:
- temperature in space
- temperature gradient in space or how temperature changes with distance and direction
Controls on temperature
- Latitude
- Differential heating of land and water
- Ocean currents
- Elevation
- Geographic position
- Clouds and albedo
Latitude
variation in sun angle
variation in length of daylight
Differential heating of land and water
What is a fluid and convection redistribute heating from solar radiation
Water, being more transparent, distributes heat vertically
Specific heat is three times higher for water than land
evaporation of water carries away heat from wet surfaces
Ocean currents
responsible for about 1/4 of latitudinal redistribution of heat, wind is responsible for the other 3/4
Warm currents keeps temperatures relatively moderate at unexpected latitudes
Cold currents moderate tropic heat
Elevation
Temperature drops about 6.5 C per km rise in the troposphere
Air is thinner - atmosphere loses the ability to absorb and radiate - resulting in rapid heating and cooling
Geographic position
difference in temperature because of prevailing winds
Land receiving wind from ocean tend to have milder temperatures
Land sending wind to sea receive more extreme temperatures
Mountain ranges also affect temperature
Cloud cover and albedo
cloud cover associated with seasonal rains prevent solar radiation from reaching the surface
clouds also keep it warm from absorbing and reradiating longwave radiation emissions from Earth’s surface
Water and temperature
maritime - moderate temperatures
high specific heat
radiation penetrates
Mixing
high evaporation (cooling)
Land and temperature
continental - extreme temperatures
Low specific heat
opaque surfaces
no mixing of land
low evaporation
Specific Heat
amount of heat needed to raise the temperature of 1 gram of substance by 1 degree Celsius
water has uncommonly high specific heat
takes more energy to warm water than warm rocks, soil, plant biomass, roads, etc.
The Global Water Cycle
powered by energy from the sun
drives evaporation into the atmosphere
moisture and associated energy are carried by winds
precipitation and dew return it to oceans and land
some of this ends up as runoff, meaning leaving continental surfaces via rivers
Water molecules
water molecules consist of two hydrogen and one oxygen
Oxygen is a negative charge
Hydrogen is a positive charge
attraction between water molecules is called hydrogen bonding
Ice has the strongest bond, molecules firmly bonded in a hexagonal form
Energy absorbed in a change of state
melting
evaporation
sublimination
Energy released in a change of state
Freezing
condensation
deposition
latent heat
term for how much energy is required or released by a change in phase
associated with a change in state, not a change in temperature
stored energy
Mixing ratio
mass of water vapor/mass of air in total
Absolute humidity
mass of water vapor/volume of air in total
specific humidity
mass of water vapor/mass of water vapor or mass of total air
Vapor pressure
another measure of water vapor in air is the pressure it exerts on the air
parcels with water vapor exert higher water vapor pressures on the air
Saturation
the amount of water that can be held by air is controlled by the temperature
Saturation is when a parcel of air cannot hold anymore water
Saturation Vapor pressure
the vapor pressure exerted by water molecules for air in a saturated state
relative humidity
actual vapor pressure/saturated vapor pressure
changes in two ways
1. add or subtract moisture (changes in numerator)
2. changing the temperature (changes in denominator)
approaches to saturation
- addition of water vapor by evaporation
- cooling to the dew point temperature
Dew-point temperature
temperature to which a parcel would need to be cooled to become a saturated parcel
determined by the air parcel’s absolute water content (aka mixing ratio)
Adiabatic temperature changes
results from expansion and compression of air
expansion = cooling
compression = warming
Dry adiabatic rate
10 C per 1km
air parcel rising upward
experiences successfully lower pressure
cools and expands adiabatically
Wet adiabatic rate
5 C per 1km
If it’s cooled to its dewpoint
condensation begins
this releases the heat from gas to a liquid changing of phase
slows the rate of cooling with continued rise
What causes air parcels to rise upward
- Orographic lifting
- Frontal wedging
- Convergence
- Localized Convective lifting
Orographic lifting
air is forced to rise over a topographic barrier
Frontal wedging
warmer, less dense air forced over cooler, denser air
Convergence
horizontal airflow piles up and is forced upward
Localized convective lifting
unequal surface heating causes local pockets of hot air that then rises
Stability
air’s tendency to rise, sink, or stay where it is, controlled by the parcel’s temperature compared to its surroundings
If the parcel is cooler than the surrounding air it sinks and is called stable.
Stability enhanced when
the Earth’s surface is radiatively cooled after sunset
an air mass is cooled from below when passing over a cold surface and there is subsidence within an air column
Instability
If the parcel of air is warmer than the surrounding air it rises
Instability is enhanced when
solar heating is intense
an air mass is heated from below when passing over a warm surface
lifting mechanisms are activated
cloud tops are radiative cooled
Clouds
visible aggregate of minute droplets of water, tiny crystals of ice, mixture of both
Necessary conditions for clouds
- Saturation
- surface for condensation
High clouds
low temperature, small water vapor source, thin, white, icy
cirrus - high (> 6km), white, or thin - separated or detached - delicate veil-like patches or wispy fiber, often feather
Middle clouds
Prefix is alto, typically water droplets
cumulus (2-6km) globular individual cloud masses - flat bases and rising domes or towers - cauliflower like