Energy Production (topic 8) Flashcards

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1
Q

Sankey Diagrams

A

Width of the arrows = power or energy

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2
Q

Effinciency equation

A

Efficiency = useful output / total input

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3
Q

Energy density equation

A

Energy density = energy released / mass of fuel used

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4
Q

How to generate electricity

A
  1. Energy source
    • steam (heat)
    • fossil fuel (heat)
    • nuclear (heat)
    • wind (Ek)
    • wave (Ek)
    • hydroelectric (Ek)
  2. Turn a turbine with magnets. Electromagnetism.
  3. Generate electricity
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5
Q

Nuclear energy

A
  1. Nuclear energy (start with U235 uranium)
  2. Thermal energy (add a neutron and chain reaction starts)
  3. Kinetic energy
  4. Turbine

Fuel rods expel neutrons to other fuel rods which causes a chain reaction. There are control rods in between each fuel rods to absorb neutrons and control the reaction.

**Control rods absorb neutrons. Usually made of carbon or an element that can absorb neutrons.

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6
Q

Power equation that works for any case

A

Power (P) = energy / time

power = W or J sec^-1
energy = J
time = sec

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7
Q

Power equation for wind energy

A

Power = (1 / 2) A p v^3

where
Power = W or J sec^-1
A = cross sectional area of air (m^2) (pi r^2)
p (ro) = density of air (kg m^-3)
v = speed of air (m s^-1)

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8
Q

Power equation for solar energy

A

I = power / area

where
I = intensity of radiation (apparent brightness) (W m^-2)
power = luminosity of the star (W or J sec^-1)
area = surface area of a sphere (m^2) (4 pi r^2)

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9
Q

Wien’s displacement law

A

lambda max = (2.9 x 10^-3) / T (kelvin)

where
lambda max = wavelength that gives peak intensity
T = temperature of a blackbody with similar temperature

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10
Q

Blackbodies

A

A perfect absorber / emitter of radiation

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11
Q

Peak wavelengths

A

Hotter wavelengths have higher peaks and are more toward the left of the graph while cooler wavelengths have lower peaks and are more toward the right of the graph.

I vs lambda or intensity vs wavelength graphs

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12
Q

Stefan-Boltzmann law

A

P = eσAT^4

where
P = power (W or J sec^-1)
e = emmisivity (=1 unless otherwise told)
σ = Stefan-Boltzmann constant
A = surface area of a sphere = 4 pi r^2 (m^2)
T = surface temperature (K)

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13
Q

Albedo equation

A

Albedo = total scattered power / total incident power = I(out) / I(in)

**high albedo (1) -> very bright, reflects lots

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14
Q

Total incident energy

A

Total incident energy = energy intensity x area x time

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15
Q

Electrical energy obtained

A

Electrical energy obtained = total energy x efficiency

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