Chapter 5 Solar Thermal: Basics COPY Flashcards

1
Q

Primary energy demand is increasing continuously during last 50 years, how does it look like in the next years?

A
  • In OECD countries stagnation is observed
  • China and India are the emerging markets with the largest increase
  • In the near future steady increase is projected

Worldwide the energy content is going to reach 18 bio toe

1 toe = 41.87 GJ

Energy content of a coal wagon: 2790 GJ

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2
Q

There are two types of solar thermal power plants?

A
  • Using concentrated incident solar radiation on an absorber (CSP – Concentrated Solar Power)
  • Without using concentrated solar radiation
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3
Q

Explain what a photon is and give some of its properties

A

Photon (derived from Greek: phōs - “Light”) is an elementary excitation of the quantized electromagnetic field

It exhibits properties of both waves and particles —> Wave-particle duality

Photons are massless –> m = 0 kg

Photons move at the speed of light –> In vacuum this is 𝑐0 ≈ 300 000 Km/s

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4
Q

How does frequency and wavelength relate to each other?

Give also the relationship between energy and the freq of a photon!

A

All wavelengths have the same propagation speed, 𝑐0 in vacuum so

𝑐0 = lambda * f

Planck’s constant describes the relationship between energy and frequency of a photon

Energy of an photon: 𝐸 = ℎ ⋅ 𝑓

Planck’s constant ℎ = 6.636 × 10−34 𝐽𝑠

–> The shorter the wavelength (or higher the frequency), the greater is the Energy of the photon

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5
Q

Give the spectral range and name few of its ray types!

A
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6
Q

What are the four interactions between electromagnetic wave and a material?

A
  • Absorption
  • Reflection
  • Transmission
  • Emission
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7
Q

The darker the body:

  • The higher is the degree of absorption alpha ?
  • The lower the degree of absorption alpha ?
A
  • The higher is the degree of absorption alpha
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8
Q

The emissivity for perfect mirrors is equal to ?

A

0

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9
Q

Complete the following table

A
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10
Q

State Planck’s Law and explain what does it state!

A

Planck’s law describes the spectral density of electromagnetic radiation emitted by a black body in thermal equilibrium at a given temperature T.

  • The wavelength of maximum intensity decreases with increasing temperature
  • The higher the temperature, the higher is this maximum intensity
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11
Q

What did Stefan-Boltzmann law add to the Plancks Law?

A

The law specifies the thermal power emitted by an ideal black body as a function of its temperature

So for a non black body: we add to the equation the emissivity variable €(T)

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12
Q
A
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