Solar energy Flashcards

1
Q

Example of solar

A

Environment building- ‘day lighting’ designed narrowly, max distance from window to max sunlight

  • natural sunlight to heat builiding
  • cooling system: 2 windows, hot air rises so heat escapes also window above all doors allows heat to escape into corridor
  • automatic windows open to let hot air out through terminal chimney
  • so operates without energy input& fancy technology
  • highlights importance of good design
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2
Q

What are the 2 ways to harvest heat from the sun?

A
  • solar thermal energy

- photovoltaics

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3
Q

Energy from the sun

A
  • energy is formed by thermonuclear fusion reactions occurring in the sun
  • sun is undertaking a thermonuclear fusion reaction
  • colliding at rate of 4 million tonnes a second
  • hydrogen nuclei creates helium
  • energy that governs that is speed of light E=mc2
  • 3.9 x 1026 W (emitting at this rate)
  • Tiny mass lost = BIG energy emitted
  • Radiates energy from a surface temp of ~5500˚C
  • 4H protons -> He
  • E = mc2
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4
Q

Energy from the sun

A
  • large amount of energy coming to sun, we don’t get all of that, 30% of incoming solar energy is immediately radiated back into space.
  • other 70% comes onto earth gets absorbed into landmass, oceans, seas and is remitted away from earth.
  • in balance if we weren’t going through climate change, the 2 would cancel eachother out, what total amount of energy coming in what equal would goes out
  • diffused solar energy is blue sky, clouds still get solar energy but blocks come in
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5
Q

Earths energy budget

A
  • incoming solar energy 100% (direct solar energy)
  • absorbed by land and oceans 51%
  • absorbed by atmosphere 16%
  • absorbed by clouds 3%
  • reflected by atmosphere 6%
  • reflected by clouds 20%
    -reflected from the earths surface 4%
  • radiation absorbed by atmosphere 15%
  • radiation directly to space from earth 6%
  • ## radiated to space from clouds and atmosphere 64%
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6
Q

Greenhouse effect

A
  • look at diagram
  • incoming wave length are short, going from UV, through visible spectrum and out into the near infared spectrum
  • when earth radiates back out its at a much longer wave length so this is far infared red radiation being emitted by earth and the basis for green effects, greenhosue gases will absorb at that far wave length energy did so essentially act like a blanket rather than letting incoming wave lengths in and the longer wave length to go back
  • we have these gases acting like a blanket around the earth acting as a radiated energy is being loss to space to get a net warming effect.
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7
Q

Energy from the sun is not evenly distributed

A
  • Net solar power input across the globe is >10,000 times our current rate of use of fossil fuels and nuclear fuel
  • have lots of solar panel so in theory could supply all energy demand with solar but there are 2 issues

1) DISTRIBUTION- is variable so higher amounts of radiation received at the equator.
2) PATTERN- pattern of solar radiation compared to energy usage - so if you’re in the UK we have a seasonal distribution so peak usage will be in in the winter, a time the least amount of solar energy is received - you need energy for cooling in the summer and energy to heat in the winter.

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8
Q

How do we use solar energy?

A

Thermal energy
-As it sounds, we use the heat of the sun to do ‘work’

Photovoltaics
-We use a converter (a PV cell) to convert light energy from the sun into electricity

  • sun heats things up and then we use that heat to do something useful.
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9
Q

Residential space & water heating and commercial lighting are biggest uses

A
  • big draws are in heating for space and also residential hot water & solar energy is a good way of reducing these demands
  • BUT in the UK can’t take away all space heating but like the environment building, we can put measures in place to reduce the pressure on the grid on gas heating from other sources
  • EG. commercial lighting has a higher primary energy usage than residential lighting.
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10
Q

Thermal Energy

A
  • Low temperature work:
  • Passive heating and lighting
  • Sun passes through glass, is trapped inside, hot air can’t escape = useful technique ( why design is imperative).
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11
Q

Thermal Energy

A

Low temperature work:

  • ‘Active’ heating
  • Solar water heaters in temperate climes
  • Uses a pump, incorporates storage, and a non-solar -backup so can adjust for supply inconstancy
  • In some countries, up to 90% of water heating
  • typically found on roofs, captures suns solar energy, heating up a water system that passes through an exchange mechanism into a water tank and heats up domestic hot water system.
  • in this case you would need a pump.
  • In UK, frost damages the tans, so tanks are held inside the building
  • But in warmer locations , tanks are set up above thermal units, so this gets rid of need of a pump and can just use hot water to naturally circulate its way through the tank.
  • look at pic
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12
Q

The Flat Plate Collector

A
  • qDEL= qABS - qLOSS
    (look at diagram)
  • not complex and efficient in tapping off energy from the sun.
  • efficient in terms of cost
  • low maintenance, essentially all you need is a bock with a sheet of glass, glass allows suns radiation to pass through.
  • process of transminisity- how much energy will get through ( as naturally some will reflect off) - try to maximise this, then hits a black surface as black absorbs energy and transfers into pipes of fluid running through
  • insulating blocks at the back to capture heat and stop it being re-emitted (trying to avoid too many loses through the glass)
  • can fill plain of glass with argon rather than air (as it is low conducting) or use a vacuum to prevent heat loss across barrier.
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13
Q

Solar window Orientation

A
  • moves from technology and the focus is more upon design.
  • depending on the county you’re in, you can use the direction of the building , the simple solar gain through a window as one way to tap into solar energy.
  • if a country is cold in the winter & warm in the summer you can maximise over hang to gain solar energy in the winter when sun is lower in the sky & protect solar gain in the summer.
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14
Q

Spectrally- selective glass

A
  • where technology comes in, is to maximise performance of glass. EG. use partly natural properties of glass & trying to enhance properties to change its transmitivity (amount of light it lets in) and amount of sunlight that goes back out.
  • in this example, glass has been coated to allow visible light to pass through it (short- wave length)
  • near infrared (allows excessive heating in summer to be reflected and for infrared ( given back to atmosphere ) is prevented from escaping - so lets the useful energy into the system and the bad out.
  • look at pic!!!!!!!!!
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15
Q

Passive solar heating types

A
  • look at diagram
  • technology we’ve know for a long time to maximise suns energy for heating.
  • design techniques we can use, focus on the nature of the glass (what it lets in) and thermal mass needs to be considered.
  • if a building is made up of concrete, it absorbs heat and neutralises energy, once the sun stops heating through the window, concrete allows energy to be released gradually over time so buildings cool down.
  • so thermal mass (amount of stuff in a building) is important for solar heating.
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16
Q

Concentrating solar power

A

High temperature work:

  • Solar steam engines
  • Heat is concentrated in parabolic reflectors (heliostat field)
  • mirrors have a directional turn to face the sun, aimed at tower, tower has a collector used to heat up synthetic coil or salt solution, transfers, generates steam and drives turbine, gets power.
  • look at diagram
17
Q

Parabolic trough

A
  • has a single focal point
  • this system moves to get the sun
  • mirrored through/ running down middle in pipe system which collects heat focused on it.
  • a fluid will transfer through that pipe network, will become highly heated and then can be used to generate steam, steam goes through the turbine and generates electricity through electromagnet.
  • need a condenser on the other side to condense steam back down, creating a vacuum.
18
Q

Problems of a parabolic trough

A
  • only creates energy for certain points in the day so idea is to have a conventional fossil fuel attached on the side.
  • for when you don’t have solar gas on, it can kick in, so using conventional but reducing dependency of ff (fossil fuels).
19
Q

Ivanpah, nr Las Vegas (370 MW)

A
  • an extreme, opened in 2014, ended up being 390 MW occupied 14km2 of land.
  • 300,000 mirrors around towers at 120m high.
  • in desert in San Francisco
  • total cost $2 million
  • at top of the towers are collectors that have sodium salt in them and energy from the sun, melts sodium salt so get temps of 550oc
  • get enough energy to glow in the dark
  • 2/3 of 1 unit at drax, drax has 6 and they can run at all at once, not intermittent
20
Q

Stiring engine

A
  • Abengoa’s PS10 nr in Seville
  • 11 MW development near Seville
  • dome concentrated in certain point to generate heat and drive engine
21
Q

Global cummulative growth of STE capacity

A
  • growth looks fast, standard exponential with renewables
  • 2014 total global capacity was 4GW so that is drax
  • this won’r generate as much as drax as it can run at all times.
  • only 2 countries invested in the technology - Spain and the US
  • limited roll out if this technology despite having access
22
Q

What is STE?

A

-Solar thermal energy (STE) is a form of energy and a technology for harnessing solar energy to generate thermal energy or electrical energy for use in industry, and in the residential and commercial sectors

23
Q

Impacts of STE (solar thermal energy)

A
  • virtually unknown
  • land-use
  • can run in places like deserts where you don’t have competition for land
24
Q

How do we use solar energy?

A

Thermal energy
-As it sounds, we use the heat of the sun to do ‘work’

Photovoltaics

  • We use a converter (a PV cell) to convert light energy from the sun into electricity
  • taken up more widely, means we can convert light energy directly into electricity rather collecting, heating upstream etc
  • do it with semi- conductors technology(silicon based) often coupled with battery to even out supply pf electricity.
  • one constraint- v low efficiency , technology only harvests 15% of suns energy that hits photovoltaics other 85% of energy is wasted.
25
Q

Photovoltaics

A
  • Producing electricity from the sun
  • A coated wafer of silicon or other semiconductor.
  • Current is produced based on types of silicon (n- and p-types) used for the layers.
  • Battery needed as storage
  • 10-15% efficiency
26
Q

Photovoltaics

A
Domestic small-scale
-‘on grid’ units
-Up to 75% of household needs
-2500kWh/year
Centralised networks
-Private companies
-Gaining promotion in some countries (India and Spain)
27
Q

2 ways photovoltaics are being developed

A

1) small-scale systems come off grid, some on-grid, in theory can supply 75% of household needs
(significant contributions to household)

2) rise of solar parks, generating electricity on a bigger scale (common in Germany) feeding into the system.

28
Q

what is an electric field?

A

feeds energy to electrons to excite the, so they get extra energy and start moving across semi- conductor, go round in a circle and feed a electrical current - how we generate electricity.

29
Q

Photovoltaic systems

A

silicon is the basis for all photovoltaic systems- have 4 electrons in outer-shell would like to have 8, so forms a grid with other silicons with strong covalent bonds and you get a strick lattice.

  • doesn’t conduct electricity well as electrons and tightly stuck in that lattice structure
  • in theory light is made up of photons (discrete parcels of energy) silicon requires wave length to electron and silicon).
  • if you get photons hitting silicon at that wave length you excite the electrons and they can move out of this lattice structure, making a free electron and a hole where the electron used was, problem is electron would fall back down as you lost energy from the system.
  • so to make a semi- conductor we need to do doping, we do this with 2 elements one is phorous ( 5 electrons in outer shell) put one phorous atom for every 1,000 silicon, if we do that we have 4 covelant bonds and are free electrons - called a ‘n’ types semi- conductor, it is negative because it has an extra electron,electrons carry a negative charge.
  • if for a p time conductor or positive semi conductor , put boron into the system, only has 3 electrons, so when it sits in the system has 3 covelant bonds and 4th one has a hole in it, then bring two types of material together, so spare electrons in n types semi conductor jump across and fill in the holes in the p -type semi conductor
  • vital to look at page (particularly whats in purple)
30
Q

Covalent bond

A

is a chemical bond that involves the sharing of electron pairs between atoms. These electron pairs are known as shared pairs or bonding pairs, and the stable balance of attractive and repulsive forces between atoms, when they share electrons, is known as covalent bonding.

31
Q

Lattice

A

Structure and bonding. Ionic bonds are the electrostatic forces of attraction between oppositely-charged ions. The oppositely-charged ions are arranged in a regular way to form a giant ionic lattice.

32
Q

Silicon

A
  • For silicon, over half of the incoming solar energy is wasted because photons either don’t have enough energy or they have more than is needed to create hole-electron pairs,
  • those photons of electrcity have a specific wave length- 1.1 micro meters thats the perfect wavelength to excite the electrons and simulate electrical currents
  • energy light has lots of different wavelengths, if it has a longer wave length, it doesn’t have enough energy to make that reaction occur, so light energy is lost.
  • so 20% of solar energy that comes in is lost, can’t ract with PV cell, everything to the left has too much energy , goes through excited process, excess will be lost as heat.
  • only at specific wave lengths we get efficient PV cells, everything else is inefficient - max energy from sun means most we could get from PV cell is 30%, at the moment in the lab giving 20-25%, sitting on roof 15% average but never past 30%.
33
Q

Organic and nano photovoltaics can be printed onto flexible plastic rolls… …and prices for conventional panels are falling fast

A
  • photovoltaics are expensive, price started to collapse as industrial production ramps up so becoming economically viable
  • scale-able technologies can go from one cell to whole fields of them
  • become flexible eg. thin coatings on material so it takes away from the visual impacts.
34
Q

Photovoltaics

A
  • Isolated use in developing countries
  • Use in remote locations (e.g. satellites in orbit)
  • don’t lose 30% that goes into space, high energy capture in space
  • availability shows photovoltaics to be good for off-grid applications, particularly in developing countries with no electricity grids.
  • idea of photovoltaics in space that would then beam energy down to the earth’s surface, 50km solar PV orbiting earth
35
Q

Global shipments of photovoltaics are mostly destined for grid-connected, residential, rooftop systems

A
  • look at graph
  • most use has been on roofs& connected to grids

ADVANTAGE

  • using grid like large battery, when you generate too much electricity you can put it into the grid so its sold on to other consumers ( takes off load put on fossil fuel plants).
  • When you don’t have enough solar pv can pull on grid to compensate so still have electricity available.
36
Q

photovoltaics?

A
  • At 10% average efficiency: can do better than that already
  • PV cells installed over 0.1% of the earth’s surface (1.3% of the earth’s desert surface area) could match all current global energy needs. - 1/1000th of earths surface to meet all current global energy needs not just electricity energy
  • For the UK, a 1.4% surface area PV grid (35,000 km2) could match all current UK electricity consumption.- 1/2 of all buildings have orientation that would allow for solar pv on roofs.
  • UK not good at solar as they are not in the position for it!!!
37
Q

IEA review- global cumulative growth of PV capacity

A
  • cumulative growth on capacity year on year has been nearly 50% since 2003, what generates exponential increase
  • total capacity 120 for solar PV - why concentrated PV hasn’t been introduced as it’s more scalible
  • low cost
  • economically viable
38
Q

Recent policy changes

A
  • A ‘frenzy’ of PV installations after FiT policy announcement
  • > 100,000 new panels installed
  • Increase of 1000%
  • The ‘gold rush’ on solar panels may cost the government up to £100 million
  • UK wenr through various policy changes- 2011 policy to put PV panels& encourage households to invest in photovoltaics - give incentive’s (payments)
  • rapid increase 1000% in about 12 months in number of panels installed
  • offered 41p per KW hour to generate electricity when avergae wholesale price 9p kWh so subsides 4 times market cost
  • got wise to that and decided to bring it back in 2014 to 14p
  • 2017- 4p per kWh subsidy guarantee from gov
  • political fall out in how its been run
  • Germany v successful with PV by having a sustained feed in tariff, policy encouraging people to potentially carry out micro-generation on a long-term sustainable basis, in UK went boom&bust & over compensated people for a year and then reined it in, created huge industry & market industry but collapsed and prices tumbled.
39
Q

environmental impacts of solar PV

A
  • nearly none
  • concerns about what happens at the end of life ( very difficult) to recycle (disposal issues).
  • very flexible
  • economic pay back of PV is 2-3 years
  • expensive not competitive with other renewables eg. wind
  • good to note water maintenance made primarily of silicon which is abundant and non- toxic and some panels have cubinum in them (heavy metal).
  • look at policy change example slide