2 - Earth's Energy Budget and Atmosphere Flashcards
Potential energy formula
Ep = mgh
Ep = potential energy
m: mass
g: constant
h: height
Kinetic energy formula
Ek = (1/2)mv^2
Ek: kinetic energy
m: mass
v: velocity
Factors that affect the sun’s energy are…
Distance and inclination (23.5 deg)
Earth’s rotation is…
Counterclockwise
True or False:
Northern hemisphere > Southern hemisphere
True (in terms of heat production by the sun)
Solstices and equinox
Winter solstice: Dec 21
Spring equinox: May 20
Summer solstice: June 21
Autumn equinox: September 22
Surface inclination and radiation
When lights hit an inclined surface, some rays don’t hit the surface…
If completely horizontal, all rays will miss the surface
Ultimately, the distance affects how much energy the surface receives (the further away, the less energy)
Air
Nitrogen: 78%
Oxygen: 21%
Others: 1%
What happens when we mix gases?
Loss of their original property to become another form
Space: how big is big enough?
Take in account pressure and temperature
Pressure: force exerted on an area
Temperature: microscopic reality, movement of the particles
Volume: space enclosed in a surface
What is temperature?
A measure of the average speed of a molecule movement in a substance
Higher temp. = faster movement
Lower temp. = slower movement
Can be derived using kinetic theory of gasses
Process of radiation
100% of sun’s energy emitting on the atmosphere
- Only 50% reaches the surface of the Earth, the rest gets absorbed/reflected (clouds, atmosphere, etc.)
- 7% of the 50% is convected and conducted (hot air rising and transferred)
- 23% of the 50% goes in water vapour that ends up condensating
- 20% of 50% is lost in radiation (8% goes back in the hemisphere and 12% goes out of the atmosphere)