Snowpack Properties, Evolution and Ablation

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Snowpack Properties, Evolution and Ablation

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Title: Snowpack Properties, Evolution and Ablation


1
Snowpack Properties, Evolution and Ablation
  • The discussion in the preceding lectures has
    emphasized the various processes of metamorphism
    that control the snow bulk properties.
  • Thermal properties that depend only on density
    (specific heat, latent heat) are well defined.

2
  • However, those that depend on conductivity or
    permeability of the snowpack are affected by
    sintering, particle size, ice layers and depth
    hoar.
  • The specific and latent heats of snow are the
    simplest thermal properties to determine since
    the contributions from air and water vapour can
    be discounted each property is simply the
    product of the snow density and the corresponding
    property for ice.

3
  • The temperature dependence of the specific heat
    of ice given by Dorsey (1940) is
  • C 2.115 0.00779T
  • where C is the specific heat (kJ kg-1 K-1), and T
    (oC) is temperature.
  • The latent heat of melting of ice at 0oC and
    standard atmospheric pressure is 333.66 kJ kg-1.

4
  • For one-dimensional, steady-state heat flow by
    conduction in a solid the thermal conductivity is
    the proportionality constant of the Fourier
    equation
  • F -K dT/dz
  • where F is the heat flux (W m-2) and dT/dz is the
    temperature gradient.
  • The thermal conductivity of snow (K) is a more
    complex property than specific heat because its
    magnitude depends on such factors as the density,
    temperature and the microstructure of the snow.

5
  • The thermal conductivity of ice varies inversely
    with temperature by about 0.17 oC-1 the same
    may be expected for snow.
  • A temperature gradient could induce a transfer of
    vapour and the subsequent release of the latent
    heat of vapourization, thereby changing the
    thermal conductivity value.

6
  • In non-aspirated dry snow the heat transfer
    process involves conduction of heat in the
    network of ice grains and bonds, conduction
    across air spaces or pores, convection and
    radiation across pores (probably negligible) and
    vapour diffusion through the pores.
  • Because of the complexity of the heat transfer
    processes, the thermal conductivity of snow is
    generally taken to be an apparent or
    effective conductivity Ke to embrace all the
    heat transfer processes.

7
  • The degree of surface packing (for example,
    hardness) also affects the flow of heat through
    snow, probably because a surface crust of low air
    permeability inhibits ventilation in the upper
    snow layer.
  • The thermal conductivity of snow, even when
    dense, is very low compared to that of ice or
    liquid water therefore snow is a good insulator.
  • This is an important factor affecting heat loss
    from buildings and the rate of freezing of lake
    and river ice.

8
  • Typical numerical models of snow use three
    prognostic variables to define a snowpack snow
    depth, snow water equivalent, and temperature.
  • From snow depth and snow water equivalent, one
    can infer the snow density from
  • ?s ?w(w/s)
  • where w (m) is the snow water equivalent, s (m)
    is the snow depth, and ?s and ?w are the snow and
    water densities, respectively.

9
Source Sun et al. (2004)
10
  • Apart from snow depth and snow water equivalent,
    the heat content or temperature of the snowpack
    is required to describe the system completely.
  • The snow temperature is directly related to its
    heat content H (J) by
  • T H/(?w w C).
  • The energy balance of a snowpack is complicated
    not only by the fact that shortwave radiation
    penetrates the snow but also by water movement
    and phase changes.

11
Source Lynch-Stieglitz (1994)
12
  • The energy balance of a snow volume depends upon
    whether it is a cold (lt 0oC) or a wet (0oC,
    often isothermal) snowpack.
  • Recall the energy balance of the snowpack
  • Q QP QH QE QG ?QS QM.
  • A term is added here to the energy balance to
    consider the heat transported by precipitation
    (QP), either snowfall or rainfall.

13
  • In the case of a cold snowpack, such as is
    commonly found in mid-latitudes during winter
    with little or no solar input, QE and QM are
    likely to be negligible.
  • Similarly, heat conduction within the snow will
    be small because of the low thermal conductivity
    of snow and the lack of solar heating, so that
    ?QS and QG are also negligible.
  • The energy balance therefore reduces to that
    between a net radiative sink Q and a convective
    sensible QH heat source.

14
  • Although snowcover reduces the available energy
    at the surface because of its high albedo to
    solar radiation and high emissivity of longwave
    radiation, its insulative properties exert the
    greatest influence on soil temperature regime.
  • Snow acts as an insulating layer that reduces the
    upward flux of heat, resulting in higher ground
    temperatures than would occur if the ground was
    bare.

15
  • In Canada, average ground temperatures are about
    3oC warmer than average air temperatures.
  • In the case of a wet snowpack during the melt
    period, the surface temperature will remain close
    to 0oC, but the air temperature may be above
    freezing.
  • Since snow is porous, liquid water infiltration
    is also important in transporting energy within
    the snowpack and into soils.

16
  • If meltwater freezes within the snowpack, there
    is latent release, warming snowpack layers to the
    freezing point.
  • Most of the energy exchanges between snow and its
    environment occur at the atmosphere or ground
    interfaces however, because snow is porous, some
    radiation and convective fluxes that occur within
    the top few centimetres of the snowpack.

17
  • The important fluxes that can directly penetrate
    the snowpack are radiation, conduction,
    convection, and meltwater or rainwater
    percolation.
  • Temperature regimes in dry snowpacks are
    exceedingly complex and are controlled by a
    balance of the energy regimes at the top and
    bottom of the snowpack, radiation penetration,
    effective thermal conductivity of the snow
    layers, water vapour transfer, and latent heat
    exchange during metamorphism.

18
  • Temperature stratification within dry snowpacks
    is usually unstable (warm temperatures below cold
    temperatures) from formation until late winter
    and spring, as energy inputs from the soil
    boundary exceed those from the atmosphere and
    upper layers.
  • As a result, temperatures become warmer with
    depth, with gradients as high as 50oC m-1 in
    shallow subarctic and arctic snowpacks during
    early midwinter.

19
  • In cold climates with frozen soils, an inversion
    can develop in late winter where the upper
    snowpack warms to higher temperatures than the
    lower layers this reflects higher energy inputs
    from the atmosphere (often due to long sunlit
    periods in the northern spring) than from the
    frozen soil.
  • For a given climate, the thermal regime in the
    snowpack strongly depends on the amount of
    snowfall early in the winter season.

20
  • Heavy snowfall early in the winter will tend to
    maintain the snowpack relatively warm, whereas
    shallow snowcovers will adjust more rapidly to
    the air temperatures.
  • For a deep snowpack a midwinter rainfall would
    increase density and decrease depth.
  • Subarctic and arctic snowpacks can undergo melt
    in upper layers whilst maintaining snow
    temperatures significantly below the freezing
    point in the lower layers.

21
  • Internal heat fluxes in wet snow, or in partially
    wet snow, are principally driven by conduction
    and by latent heat release due to refreezing of
    liquid water.

22
Ref Bartelt and Lehning (2002)
23
Ref Bartelt and Lehning (2002)
24
Source Stieglitz et al. (2003)
25
Source Stieglitz et al. (2003)
26
Source Pomeroy and Brun (2001)
27
Snowpack Ablation
  • In many countries snow constitutes a major water
    resource its release in the form of melt water
    can significantly affect agriculture,
    hydro-electric energy production, urban water
    supply and flood control.
  • The ablation of a snowcover or the net volumetric
    decrease in its snow water equivalent is governed
    by the processes of snowmelt, evaporation and
    condensation, the vertical and lateral
    transmission of water within the snowcover and
    the infiltration of water to the underlying
    ground.

28
  • In turn, water yield and streamflow runoff
    originating from snow are governed by these same
    processes as well as the storage and the
    hydraulics of movement of water in channels.
  • The rate of snowmelt is primarily controlled by
    the energy balance near the upper surface, where
    melt normally occurs.
  • Shallow snowpacks may be considered as a box to
    which energy is transferred by radiation,
    convection, and conduction.

29
  • Early in the melt sequence vertical drainage
    channels develop in the snow contributing further
    to its heterogeneity.
  • The internal structure significantly influences
    the retention and movement of melt water through
    the snow, making a detailed analysis of the
    transmission process extremely difficult.
  • When the pack is primed to produce melt it is at
    a temperature of 0oC throughout and its
    individual snow crystals are coated with a thin
    film of water also, small pockets of water may
    be found in the angles between contacting grains,
    usually amounting to 3 to 5 of the snow by
    weight.

30
  • Any additional energy input produces melt water
    which subsequently drains to the ground.
  • When melt rates are at their highest, 20 (by
    weight) of the pack or more may be liquid water,
    most of which is in transit through the snow
    under the influence of gravity.
  • The amount of energy available for melting snow
    is determined from the energy budget equation.

31
Shortwave Radiation
  • There are two main types of radiation affecting
    snowmelt shortwave and longwave radiation.
  • The amount of solar radiation penetrating the
    earth's atmosphere to be received at the surface
    varies widely depending on latitude, season, time
    of day, topography (slope and orientation),
    vegetation, cloud cover and atmospheric
    turbidity.

32
  • While passing through the atmosphere radiation is
    reflected by clouds, scattered diffusely by air
    molecules, dust and other particles and absorbed
    by ozone, water vapour, carbon dioxide and
    nitrogen compounds.
  • The absorbed energy increases the temperature of
    the air, which in turn, increases the amount of
    longwave radiation emitted to the earth's surface
    and to outer space.

33
  • Short-wave radiation reaching the surface of the
    earth has two components a direct beam component
    along the sun's rays and a diffuse component
    scattered by the atmosphere but with the greatest
    flux coming from the direction of the sun.
  • Figure 9.1 shows the annual variation in daily
    values of solar radiation received by a
    horizontal surface at several latitudes assuming
    a mean transmissivity of unity, implying that all
    the energy reaches the surface.
  • The influence of transmissivity is illustrated in
    Figure 9.2.

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36
Source Gray and Male (1981)
37
  • The time of year obviously is an important factor
    governing the solar radiation flux incident on
    the earth's surface, and hence on the melt rate.
  • As a rule, the longer the spring melt is delayed
    the greater the danger of flooding.
  • This is due partly to increases in the radiative
    flux and partly to the increased probability of
    rain.

38
  • The transmissivity is highest in winter and
    lowest in summer because the atmosphere contains
    more water vapour during summer.
  • It also varies somewhat with latitude, increasing
    northwards.
  • Snow on a south-facing slope melts faster than
    snow on a north-facing slope, the reason being
    that the orientation of the slope affects the
    amount of direct beam solar radiation the area
    receives.

39
  • The results are symmetric about a north-south
    line as might be expected the influence of
    orientation diminishes towards the summer
    solstice.
  • Even on a 10o slope the effect of orientation can
    be significant e.g., at 50oN on April 1, a
    south-facing slope receives approximately 40
    more direct beam radiation than a north-facing
    slope.

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43
Longwave Radiation
  • The net longwave radiation at the snow surface L
    is composed of the downward radiation L? and the
    upward flux L? emitted by the snow surface.
  • Over snow L? is normally greater than L? so that
    L represents a loss from the snowpack.
  • The longwave radiation emitted by the snow
    surface is calculated with the Stefan-Boltzmann
    law on the assumption that snow is a near perfect
    black body in the longwave portion of the
    spectrum.

44
  • In alpine areas topographical variations have a
    significant influence on the longwave radiation
    received at a point, e.g., in a valley the
    atmospheric radiation is reduced because a part
    of the sky is obscured by its walls.
  • However, the valley floor will gain longwave
    radiation from the adjacent slopes in amounts
    governed by their emissivities and temperatures
    the reflected longwave radiation from snow and
    most natural surfaces is almost negligible.
  • Thus in areas of high relief the radiation
    incident at a site includes longwave emission
    from the atmosphere and the adjacent terrain.

45
  • To a first approximation the radiation emitted by
    cloud can be obtained by assuming black-body
    emission at the temperature of the cloud base.
  • Hence, the net longwave radiation exchange
    between the overcast sky and the snow can be
    approximated as an exchange between two black
    bodies having temperatures Ts (snow surface) and
    Tc (cloud base), i.e., L s(Tc4 - Ts4).

46
Sensible, Latent, and Ground Heat Fluxes
  • The convective and latent energy exchanges, Qh
    and Qe, respectively, are of secondary importance
    in most snowmelt situations when compared to the
    radiation exchange, but still need to be
    considered to assess melt rates.
  • Both Qh and Qe are governed by the complex
    turbulent exchange processes occurring in the
    first few metres of the atmosphere immediately
    above the snow surface.

47
  • Heat is transferred to the snow by convection if
    the air temperature increases with height
    (commonly occurring when the snow is melting)
    and water vapour is condensed on the snow
    (accompanied by release of the latent heat of
    vapourization) if the vapour pressure increases
    with height.
  • The ground heat flux QG is a negligible component
    in daily energy balances of a snowpack when
    compared to radiation, convection or latent heat
    components, so that the total snowmelt produced
    by QG over short periods of time can be ignored.

48
  • However, QG does not normally change direction
    throughout the winter months and consequently its
    cumulative effects can be significant over a
    season.
  • In areas where snow temperatures remain near the
    freezing point and ground temperatures are
    relatively warm, melt can be produced as a result
    of QG.
  • Although the amount of water produced may be
    small, its resultant effect on the thermal
    properties and infiltration characteristics of
    the underlying soil may be important.

49
  • Heat exchanges between soils and snow follow the
    simple Fourier equation for heat transfer used in
    heat transfer in snow alone.

50
Rain on Snow
  • The heat transferred to the snow by rain water is
    the difference between its energy content before
    falling on the snow and its energy content on
    reaching thermal equilibrium within the pack.
  • Two cases must be distinguished in this energy
    exchange

51
  • 1) Rainfall on a melting snowpack where the rain
    does not freeze
  • 2) Rainfall on a pack with temperature lt 0oC
    where the water freezes and releases its latent
    heat of fusion.
  • The first case can be described by the
    expression
  • QP ?w Cp(Tr - Ts)Pr/1000
  • where QP is the energy supplied by rain to the
    snowpack, ?w is the density of water, Cp is the
    heat capacity of water, Tr the temperature of the
    rain, Ts is the snow temperature, Pr is the depth
    of rain or precipitation rate.

52
Units
  • QP (kJ m-2 d-1)
  • ? (kg m-3)
  • Cp (kJ kg-1 oC-1)
  • Tr (oC)
  • Ts (oC)
  • Pr (mm d-1)

53
  • When rain falls on a snowpack which has a
    temperature lt0oC, the situation is more
    complicated since the pack freezes some of the
    rain thereby releasing heat by the fusion
    process.

54
Snowmelt
  • The amount of meltwater can be calculated from
  • wm QM /(?w Lf B)
  • where wm is the meltwater (m), Lf (J kg-1) is the
    latent heat of fusion, and B is the fraction of
    ice in a unit mass of wet snow.
  • B usually has a value of 0.95 to 0.97.

55
  • Net radiation and sensible heat largely govern
    the melt of shallow snowpacks in open
    environments.
  • At the beginning of the melt, radiation is the
    dominant flux with sensible heat growing in
    contribution through the melt.

56
  • If a complete set of meteorological measurements
    is not available, then temperature index models
    may be used to predict snowmelt. Index models
    relate melt to air temperatures such that
  • wm Mf (TA - TB)
  • where TA (oC) is the mean air temperature over a
    given time period and TB is a base temperature
    below which melt does not occur (usually 0oC).
  • The melt factor Mf varies from 6 to 28 mm oC-1
    day-1 for snowmelt on the Canadian Prairies.

57
  • Although index models are simple, they should be
    used with caution as the melt factors tend to
    vary from year to year and with location.

58
Streamflow Generation
  • Streamflow generated by snowmelt water that
    directly runs off rather than infiltrating or
    from water that infiltrates and then moves
    downslope through a shallow subsurface soil of
    high permeability.
  • During snowmelt, frozen or saturated soils
    restrict infiltration and evaporation is
    relatively low this promotes a water excess over
    a basin and permits relatively large runoff
    generation for the amount of water applied to the
    ground.

59
  • As a result, peak annual streamflows often occur
    directly after snowmelt.
  • The constituent water of this freshet comprise
    both snowmelt water and water expelled from soils
    by infiltrating snowmelt water, with important
    implications for stream chemistry.
  • For point scales, the influence of snow water
    equivalent on infiltration and runoff generation
    varies for different soil types.

60
  • The effect of a deep forest environment snowpacks
    in promoting warm soils causes forest runoff to
    drop with increasing snow water equivalent for
    deep snow and dry soils.
  • In northern forests, from 40 to 60 of annual
    streamflow is derived from snowmelt, with
    increases in snowmelt runoff of from 24 to 75
    when the forest is removed by harvesting or fire.
  • In cold, semiarid environments (arctic, northern
    prairies, steppes), greater than 80 of annual
    streamflow is derived from snowmelt, even though
    snowfall accounts for less than 50 of the annual
    precipitation.

61
  • Snowmelt in the western cordillera of North
    America and mountain systems of central Asia is
    the major source of water when carried as
    streamflow to semiarid regions downstream.
  • Snowmelt water sustains arctic, alpine, prairie,
    and boreal forest lakes and wetlands, which are
    primary aquatic habitats in their respective
    ecosystems.

62
Ref Barnett et al. (2005)
63
Annual Cycle of River Discharge
64
Annual cycle of mean daily discharge
65
Latitudinal Variation of HJUB Freshets
JD 5(Latitude) -126
Source Déry et al. (2005), J. Climate.
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