Chapter3: Solar energy Flashcards
Give Five characteristics of the sun:
- Radiative source
- Diameter dS = 1,392 ⋅ 106 km
- Surface temperature Ts = 5777 K
- Core temperature Tc = 15 Mio.K
- Spherical shape
Give 4 characteristics of Earth:
- Spherical shape
- Diameter dE = 1,271 ⋅ 104 km
- Surface temperature Ts = 290 K (varies between -89.2 °C to 56.7 °C)
- Core temperature Tc = 7000 K
Name all the angles that describe the positioning of the sun to the earth! draw a figure:
When do stationary absorbers in Germany perform best?
Stationary absorbers in Germany perform best with an azimuth angle of 0° (South) and an inclination of 35°.
Explain what a photon is and give some of its properties
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
How does frequency and wavelength relate to each other?
Give also the relationship between energy and the freq of a photon!
All wavelengths have the same propagation speed, 𝑐0 in vacuum so
𝑐0 = 𝜆 ⋅ 𝑓 with 𝑓 = 1 /T
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
Give the spectral range and name few of its ray types!
What are the four interactions between electromagnetic wave and a material?
- Absorption: The absorption coefficient 𝛂 indicates how much radiation is absorbed
- Reflection: The reflectance ρ indicates the relationship between incident and reflected radiation
- Transmission: The degree of transmission 𝛕 indicates the relationship between incident and transmitted radiation
- Emission: The emissivity ϵ indicates how much radiation is emitted by the body
The darker the body:
- The higher is the degree of absorption alpha ?
- The lower the degree of absorption alpha ?
- The higher is the degree of absorption alpha
The emissivity for perfect mirrors is equal to ?
0
Complete the following table
State Planck’s Law and explain what does it state!
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
What did Stefan-Boltzmann law add to the Plancks Law?
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)
- Calculate the radian intensity at the earth orbit.
- Determine the total radiation reaching the earths surface.
- Compare this value with the annual energy demand.
Transmission losses in the atmosphere: What factors influence attenuation of solar radiation:
𝜏𝜆 = 𝜏𝜆,𝑅 𝜏𝜆,𝐴 𝜏𝜆,𝑂3 𝜏𝜆,𝑊 𝜏𝜆<em>,G</em>
<em>Where: </em>
- 𝜏𝜆,𝑅: Rayleigh Scattering by Molecules
- 𝜏𝜆,𝐴: Absorption by aerosols
- 𝜏𝜆,𝑂3: Absorption by ozone
- 𝜏𝜆,𝑊: Absorption by Water Vapor
- 𝜏𝜆<em>,G</em>: Absorption by air