Introduction and Greenhouse Effect Flashcards
Name four low carbon energy sources
Fossil fuels with CCS, solar, hydroelectric, wind
Name some low energy carbon sources that aren’t the main four
Nuclear, wave, tidal, geothermal, biomass
Why do we depend on fossil fuels so heavily?
They have a large power delivery
What is currently the biggest renewable energy source?
Hydroelectric
Where do the vast majority of energy sources come from?
Directly or indirectly from the sun
How does the energy in fossil fuels come from the sun?
Fossil fuels are stored solar energy as they are ancient biomass. The biomass has decayed and transformed over millions of years and stored the energy as carbon.
How much of the energy from the sun is converted in wind energy?
1-2%
How does wind power ultimately come from the sun?
Areas that receive more solar energy are hotter and the air less dense. This air rises and is replaced by cold air from neighboring regions and this is what causes wind.
How much more solar energy is converted into wind energy than into biomass by all the plants on Earth?
50 to 100 times
How does wave power ultimately come from the sun?
The wind that has been generated by the sun, generates waves due to the friction of the air moving over the surface of the sea.
How does hydroelectric power ultimately come from the sun?
Solar radiation drives the water cycle through evaporation of surface water. The water then falls on higher areas which provides it with the gravitational potential energy needed for hydroelectric power.
What are the three exceptions to energy coming from the sun?
Nuclear power, geothermal and tidal power.
How does biomass ultimately come from the sun?
Biomass uses solar radiation for photosynthesis by reacting with the chlorophyll in the plants (along with water and CO2) to create sugars that are converted into starch. This is a light-activated chemical reaction that generates high energy HC chains which we can then break down and release the energy from to produce electricity.
Describe where the energy comes from in nuclear power.
The energy comes from destruction or change of the fuel itself
Describe where the energy comes from in tidal energy.
The gravitational pull of the moon causes high tides when that side of the Earth is closest to the moon. This then drops as the Earth turns and gives tides.
Describe where geothermal energy comes from.
The core of the planet is hot because of the gravitational potential energy from the formation of the planet - plus a little bit of nuclear fission which happens to keep the core of the planet warm)
Why are fossil fuels not considered a renewable energy?
We are extracting it much faster than it is being made.
How much energy does the sun radiate to the Earth in kwh?
1.744x10^14 kwh per hour
How much energy does the sun radiate that reaches the Earth in watts?
1.744x10^17 watts
What is the conversion for Mtoe to kWh?
1 Mtoe = 1.163x10^10 kWh
What is the average worldwide energy consumption in 2017 in Mtoe and kWh?
13511 Mtoe = 1.57x10^14 kWh
How much of our consumed power was derived from fossil fuels in 2017?
80-90%
What was the annual energy consumption in 2012 in watts?
1.2x10^13 W
What does Mtoe stand for?
Mega tonne of oil equivalent
Can the energy from the sun provide us with our current energy demands?
Yes, but we are not using it properly.
Define direct radiation
When light does not interact with the atmosphere (what you see if you look directly at the Sun)
Define indirect radiation
Light that has been scattered in the atmosphere (on a day when you cannot see your shadow, all the radiation has been scattered and no direct radiation reaches you)
Define scattering
The term used to describe several processes such as reflection and refraction that can alter the direction that light is travelling
Define absorption
Electromagnetic radiation is taken up my molecules in the atmosphere through the transference of the energy to the electrons within the molecules, resulting in the generation of heat.
What emits electromagnetic radiation and what does it depend on?
Electromagnetic radiation occurs from all objects, the amount and wavelength depends upon its temperature (eg. the Sun is very hot so emits UV, visible light and IR)
Do hot or cool objects emit shorter wavelengths?
Hot objects
What temperature are the Sun and Earth and what wavelengths do they emit?
500 nm - short (Sun, 5525 K)
10,000 nm - long (Earth 290 K)
How can you tell how hot a piece of steel is?
By its colour
Why does the Earth’s surface cool down quicker on clear nights?
Because clouds (containing water) are strong absorbers and emitters of IR radiation
Why are nights colder at higher elevations?
There is less atmosphere to act as a ‘blanket’ and limit the amount of radiation leaving Earth.
What are the four parameters that determine scattering and absorption, what are they all a function of, and what do they give us in combination?
Refractive index (n), reflectance (R), transmission (T), absorbance (A). They are all functions of wavelength and in combination give us the greenhouse effect.
Define Rayleigh scattering
For wavelengths around 10^-4, particles are small compared to the to the wavelength of light
Why is the sky blue and sunsets red?
Rayleigh scattering is more effective at scattering shorter wavelengths (blue) so this is what we see during the day. At dusk and dawn when the Sun is further away, the blue light is so scattered by the time it reaches our eyes that all we see is the red that is left.
Define Mie scattering
This type of scattering depends on the shape of the molecule that is doing the scattering and occurs in particles about the same length as the wavelength of light (a few 100 nm), eg in fine clouds
Define geometric scattering
Occurs when the particle is much larger then the wavelength of light, (greater than 10x the wavelength), eg large water droplets in clouds
Which equations tell us how light is reflected and transmitted at a material interface?
The Fresnal equations
What do R, n1, n2, and T refer to in the Fresnal equations at near-normal incident radiation?
Reflected, refractive index of reflected radiation, refractive index of transmitted radiation, transmitted
Give the Fresnal equation for reflected radiation for near-normal incidence.
R = ((n1-n2)/(n1+n2))^2
Give the Fresnal equation for transmitted radiation for near-normal incidence.
T = 1-R