Temperature - Soil Physics - Lecture Slides, Slides of Soil Physics

Soil physics is the study of soil physical properties and processes. It is applied to management and prediction under natural and managed ecosystems. (Wikipedia). Keywords in this lecture are: Temperature, Heat Content, Soil Temperature, Soil Hydraulic Properties, Radiaiton, Conduction, COnvection, Stefan Boltzmann Law, Emissivity, Wien,s Law, Solar Radiation, Albedo, Surface Energy Balancy

Typology: Slides

2012/2013

Uploaded on 12/31/2013

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What is temperature?
Measure of the average random kinetic
energy of the molecules of a substance
Physical property that determines the
direction of heat flow between two
substances in thermal contact
T ≠ Heat Content
Heat Content = (T - Tref) x C heat capacity – we’ll
get to it later.
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What is temperature?

  • Measure of the average random kinetic energy of the molecules of a substance
  • Physical property that determines the direction of heat flow between two substances in thermal contact
  • T ≠ Heat Content
  • Heat Content = ( T - Tref ) x C heat capacity – we’ll get to it later. docsity.com

Soil Temperature

  • Critical factor that influences important physical, chemical, and biological processes in soil and plants: - Soil hydraulic properties - Organic matter decomposition and mineralization - Biodegradation of pesticides - Seed germination - Plant growth

Radiation

  • All objects at a temperature T > 0 K

emit radiation: energy in the form of electromagnetic waves

  • Total amount of radiation emitted

strongly depends on T.

  • Stefan-Boltzmann law:

Jt : total energy emitted, W m -

ε: emissivity (unitless)

= 1 for a “black body”; 0.9 to 1.0 for soil

σ: Stefan-Boltzmann constant

= 5.67 x 10 -8^ W m -2^ K-

T : temperature of the emitter (K) Note: by convention, little t is time, big T is Temperature.

Radiation

4

J t = ε T σ

  • Wien’s law

λ m is the wavelength of maximum radiation

intensity

  • λ m is inversely proportional to temperature

Radiation

T

m K m

μ λ

2900

  • Wien’s law
  • Sun Surface Temperature ≈ 5760 K
  • Earth Surface Temperature ≈ 288 K
  • λ m for the sun is about 0.5 μm. 99% of solar radiation is in

the wavelengths 0.3 - 4.0 μm and is called shortwave

  • λ m for the earth is about 10 μm ( range of 3 - 50 μm), and is called infrared or long-wave radiation

Radiation

T

m K m

μ λ

2 9 0 0

Net radiation at the soil surface

  • The global solar radiation as it reaches the land is further partitioned
  • Net radiation at the soil surface: Jn = (J (^) s + Ja) (1-α)+ Jil - Jo J (^) n = net radiation J (^) s = direct beam incoming short-wave J (^) a = diffuse incoming short-wave α = albedo: the fraction of incoming short- wave radiation reflected by the surface J (^) il = incoming long-wave J (^) lo = outgoing long-wave

Albedo (α)

  • Shortwave reflectivity
  • For soils, α varies from 0.1 - 0.4 (unitless)
  • Depends on:
    • Soil color
    • Surface roughness
    • Sun angle (latitude, time of day)
    • Soil wetness
    • Slope and aspect

Surface energy balance

Heat flow in soil

  • Radiation is how energy gets from the sun to the soil surface.
  • Convection and conduction are the two most important mechanisms of heat transport under normal conditions
  • A third mechanism, latent heat movement, will show up in the next lecture.