Topic_2_Ch_5_Radiation

Topic 2: Energy and Radiation Balances

Chapter 5: Radiation

  • Radiation Fundamentals

    • Speed of light (c) is constant for all forms of radiation:

      • Relationship: c = λ ν (where λ = wavelength and ν = frequency)

    • Shorter wavelengths correlate with more energy, while longer wavelengths correlate with less energy.

    • Energy quantification: Q = h ν or Q = h c/λ

  • The Electromagnetic Spectrum

    • All radiation types travel at the speed of light and in a vacuum.

    • All objects emit radiation based on their temperature.

    • Energy transfer occurs via all forms of radiation.

Emission of Radiation

Radiation Laws

  • Planck's Law

    • Relates temperature of a substance to its emitted radiation.

  • Stefan–Boltzmann Law

    • Emission rate (E) proportional to the fourth power of temperature (T):

      E = ε σ T^4

    • E = flux density (W·m^–2),

    • ε = emissivity (1 for black bodies),

    • σ = Stefan-Boltzmann constant (5.67 × 10^–8 W·m^–2·K^–4).

  • Wien's Law

    • Maximum emission wavelength inversely related to temperature.

  • Planck's Law (Detailed)

    • Radiation comprises energy bundles called photons.

    • Shorter wavelengths = higher energy per photon.

Shortwave vs Longwave Radiation

  • Black body approximation for both Earth and Sun:

    • Sun (T = 5,800 K): emission mainly 0.15 - 3.0 µm (Shortwave)

    • Earth (T = 288 K): emission mainly 3.0 - 100 µm (Longwave)

Radiation Interaction with Surfaces

Absorption, Reflection, and Transmission

  • Incident radiation can:

    1. Be absorbed (a)

    2. Be reflected (α)

    3. Be transmitted (t)

  • Equation: a + α + t = 1 (or 100%)

Radiation in the Atmosphere

Scattering and Absorption

  • Radiation Interaction

    • Absorbed radiation heats the atmosphere.

    • Scattered/reflected radiation can reach Earth's surface as diffuse radiation.

    • Direct radiation reaches the surface without interaction.

  • Scattering Types

    1. Rayleigh scattering

    2. Mie scattering

  • Absorption Characteristics

    • Longwave radiation absorbs more strongly than shortwave due to selective gases.

    • Key absorbent gases:

      • Oxygen, ozone, water vapor (strong in UV)

      • Water vapor, CO2, methane, nitrous oxide (greenhouse gases for longwave)

The Greenhouse Effect

  • Solar radiation transmits well through the atmosphere; Earth's longwave radiation is absorbed by greenhouse gases.

  • Without the atmosphere, Earth's temperature would drop by 33 K.

Temperature Structure of the Atmosphere

  • Three maximum temperatures occur due to absorption at specific wavelengths:

    1. Upper thermosphere (λ = 0.1–0.2 μm)

    2. Upper stratosphere (λ = 0.2–0.3 μm)

    3. Lowest troposphere (heat from Earth's surface)

Solar Radiation

  • Solar Constant: Average solar radiation at top of the atmosphere - approx. 1361 W·m^–2.

  • Sphericity Effect: Causes variation in Sun angles based on curvature.

    • Low latitudes: higher Sun angles; High latitudes: lower Sun angles.

Sun Angle Determination

  • Illustrated by two definitions:

    1. Altitude angle

    2. Zenith angle

  • Influenced by latitude, longitude, time of year, and time of day.

  • Lower altitude means lower radiation intensity due to beam spreading and depletion.

Annual Variations by Latitude

Seasons and Solar Energy

  • Seasons defined by:

    • Altitude of the Sun above horizon

    • Intensity of Sun energy

    • Duration of day length.

  • Earth’s Orbit Details:

    • 23.5° tilt from the perpendicular ecliptic plane.

    • Constant angle and orientation during orbit.

Milankovitch Cycles

  • Influential factors impacting climate variability:

    1. Eccentricity: 100,000-year cycle affecting distance from the Sun.

    2. Tilt variation: 40,000-year cycle affecting seasonality.

    3. Direction of tilt: 26,000-year cycle dictating seasonal intensity at perihelion and aphelion.

Conclusion on Seasonal Variations

  • Sphericity affects solar intensity across latitudes and leads to varying seasons.

    • Seasonal changes impact duration and intensity of Sun received by Earth, influenced by multiple physical characteristics of Earth and its orbit.

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