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Infiltration is defined as
the entry of liquid water into the soil
There are three stages of soil water infiltration:
Stage I: Flux control (Supply control)
Stage II: profile control
Stage III: hydraulic conductivity
Infiltration - Stage I: flux control (supply control (delivery of water to the soil surface))
Controlled by the rate at which water is applied to the surface (flux control); the higher the rate, the shorter stage I
Infiltration - Stage II: profile control
The rate at which the soil absorbs the water is lower than the supply rate; controlled by texture, structure, layering in the profile
Infiltration - Stage III: hydraulic conductivity
As the wetting front increases, the potential gradient tends to one, making the flux of water equal to the conductivity
Evaporation is defined as
the vapor loss from soil or free water directly into the atmosphere
there are three stages of evaporation
Stage I: flux control (demand controlled)
Stage II: profile controlled
Stage III: unsaturated hydraulic conductivity controlled
Evaporation - Stage I: flux control (demand controlled)
The time in stage I decreases with higher atmospheric demand
Controlled by sunlight, heat, wind, humidity > determine the demand for soil moisture from the atmosphere
Evaporation - Stage II: profile controlled
Controlled by texture, organic matter, structure in the profile
Evaporation - Stage III: unsaturated hydraulic conductivity controlled
Unsaturated hydraulic conductivity drops with decreasing water content until the soil reaches an air-dried state
Transpiration:
evaporation from leaves
Evapotranspiration =
evaporation + transpiration
Estimating potential evapotranspiration (PET) - quantifies atmosphere demand for moisture
Penman (1948) developed an equation for PET from weather station data
Data needed includes:
Air temperature
Soil temperature
Wind speed
Net radiation
Relative humidity
Electromagnetic (EM) radiation is emitted by
all objects including soil, plants, and the sun
Radiation is electromagnetic energy that exhibits
wave-like characteristics
The rate of emission and the wavelength of radiation depend on
the temperature of the emitter
Steffan - Bolteman Law
Hotter the object, more intense the radiation
The hotter an object is, the more photons emitted per
square meter per hour and the shorter the wavelength
Wiem’s Displacement Law
As temperature increases, wavelength gets shorter
The EM spectrum includes
TV, radio, radar, microwave, infrared, visible, UV, X-rays, gamma rays
Light that reaches the surface of the earth is mainly
Visible light
Near-infrared species
Radiation balance
Earth radiates long-range radiation, mostly far infrared (IR) radiation
Shortwave radiation passes easily through the atmosphere
Longwave radiation (far-IR) does not pass easily through the atmosphere
There are four things that can happen when radiation encounters matter:
Transmitted - pass through things like air, glass, or water
Scattered - bounced off in all directions; bounces off of dust, clouds, fog scatter light
Reflected - most sources reflect a lot of light
Absorbed
When the radiation is transmitted, scattered, or reflected, it remains radiation; however, when it gets absorbed, it is converted into:
Sensible heat - most often
Chemical energy - photosynthesis
Energy budget for soils
Risw - Rsw = Rabs = Hg + Ha + Hl + Rlw
Risw = incoming shortwave radiation
Rsw = reflected shortwave radiation
Rabs = absorbed and used to do something with
Hg = heat the ground
Ha = heat the air above the ground
Hl = energy used to evaporate water (latent heat of vaporization)
Rlw = long wave radiation emitted by the soil
The net radiation absorbed by any surface is the total arriving minus
the reflected shortwave and emitted longwave radiation
The amount of radiation absorbed is also related to the reflectivity of the surface:
Rabs = Risw (1-x)
X = albedo = fraction of sunlight reflected by a structure
Net radiation absorbed can be estimated by measuring the incoming radiation with a pyranometer and estimating
the reflected radiation from the albedo and emitted long-wave radiation from the surface temperature
In soils, the largest energy loss goes
to Hl (latent heat of vaporization; evaporation)
Energy units for solar energy are J m ^(-2) or W hr m ^(-2)
W = Js ^ (-1)
The amount of surface heating can be calculated from the
heat capacity and thermal conductivity of the soil
Heat capacity is the amount of energy needed to
raise the temperature of 1 gram of matter 1 degree celsius
The larger the heat capacity, the less
the soil changes in temperature when it gains or loses a certain amount of heat
Temperatures tend to be less variable in soils that
are wet and dense
Thermal conductivity is the ease
with which a material or object conducts or transmits heat, mostly dependent on water content
Because water has a high heat capacity and is a better conductor than
air, both soil heat capacity and thermal conductivity depend mostly on theta v
The temperature of the soil depends on depth and surface cover
Variability in temperature is reduced at depth
There is a damping and lag of soil temperature with greater depths
Peak temperature occurs later at deeper depths
Factors that affect heat flux and soil temperature
Radiation intensity
Soil color (albedo)
Soil water and air content - impacts heat capacity and thermal conductivity
Soil aspect - south facing vs. north facing slopes are important to know
Wind and effects of soil cover - vegetation at the surface; mulches
Conduction or diffusive transfer is the principle way in which
heat moves in soil, requires a temperature gradient
Convection is the mass flow or transfer of heat with fluid flow
Not too important within a soil
However, important for exchange within atmosphere of heat, water vapor, and CO2
Turbulence accelerates the vertical movement of
heat and water vapor away from the ground
Evaporation from soil and plant transpiration are
greatly increased during sunny, hot, dry, windy weather
Plant cover reduces
wind speed and turbulence
Mulch and vegetation moderate
soil air temperature
Earth radiates
long-range radiation, mostly far infrared (IR) radiation
Shortwave radiation passes
easily through the atmosphere
Longwave radiation (far-IR) does
not pass easily through the atmosphere