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Thomas Kaempfer's Snow Page
Note: This is my snow research page. For recreational fun in the snow, check out
my snow adventures in the picture gallery.
Observation of Snow Metamorphism by
X-ray Computed Micro-Tomography
Project Summary
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Goal :
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Undesturbed observation of the metamorphosing
micro-structure of natural snow samples subjected to different temperatures
or temperature gradients. Simultaneous measurement of heat flow (heat
conductivity) and structural analysis. The experiments
provide input for micro-structural numerical models of snow
metamorphism and snow physics and will, in combination with the
numerical simulations, improve our understanding of snow
metamorphism and the relation of the snow micro-structure to snow properties.
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Method :
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A desktop X-ray micro-tomography (SCANCO mu-CT 80) with a
resolution down to 18 mu-m is set up inside a cold room. It is
instrumented to control the temperature, a possible
temperature gradient, and simultaneously measure heat flux through
a snow sample. Time-laps series of metamorphosing snow can be
recorded.
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Collaborators :
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Martin Schneebeli, Bernd Pinzer, SLF Davos Sergey Sokratov, Moscow State University
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Sponsor :
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Swiss National Science Foundation and SLF Davos, Switzerland
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Duration :
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2003-2006
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Introduction
Snow is a highly porous medium consisting of an ice matrix and porous space
containing water vapor. With time, snow undergoes metamorphism and its
microstructure evolves. There is a strong interaction between the snow
microstructure and snow pack properties. Understanding snow metamorphism is
thus crucial for predicting mechanical properties used in avalanche
forecasting, chemical composition associated with the interpretation of ice
cores data, or thermophysical properties important for modeling the energy
balance of snow-covered landscapes.
It is common to distinguish between isothermal and temperature
gradient metamporphism. The former can be regarded as a sintering
process of individual ice crystals and the dominating driving force
is the sintering stress. In the later, a temperature gradient across
the snowpack induces a water vapor gradient in the pore-space due to
the dependency of saturation wapor pressure in air on
temperature. The dominant mechanisms are then sublimation and
condensation and associated water vapor diffusion.
Methods
A snow sample holder with fine temperature control
that fits into a Scanco micro CT80 computer-tomograph was built at
SLF (Figure). This setup allows for
non-disturbed, time-laps imaging of metamorphosing snow and is the
method of choice to observe temperature gradient
metamorphism. Experiments can be performed for several days without
removing the sample from the tomograph.
For isothermal metamorphism experiments, due to the considerably
longer time-scale, the snow samples are stored in controlled
isothermal environments for several weeks and only moved to the
micro-CT for short measurement periods.

Figure:
X-ray computer micro-tomograph (Scanco micro-CT 80) installed in
SLF Davos' Cold-lab (left) and the snow sample holder allowing for
temperature gradient control (right).
Results
Metamorphosing snow under temperature gradient
If snow is subjected to a temperature gradient, the heat flow
induces mass flow and thus an evolution of the ice-pore network (Figure); on the other
hand, the microstructure influences heat flow as heat transport is governed by
conduction in the ice and pores as well as phase change processes and water
vapor transport in the pore space.
Controlled experiments in the snow-breeder inside the micro-CT at SLF
Davos allow for the continuous observation of the dynamic sublimation
and growth processes within the ice-matrix. Under strong temperature gradients,
kinetic growth forms as facets develop (Figure).

Figure:
Micro-CT image of a 4x4x4 mm cube of a snow pack collected in the
field and consisting of rounded grains sintered together (left) and
the same snow after 10 days under a temperature gradient of 50 K/m at
T=-3.4 C (right).
Isothermaly metamorphosing snow
Isothermal metamorphism of snow is a sintering process
between the ice grains forming the snow. Under the absence of temperature
gradients, the driving force for snow metamorphism is the sintering stress,
which tends to reduce the surface free energy of the complex
ice-air interfaces and of the grain boundaries between the ice
crystals. The energy reduction of the porous structure is
achieved by mass redistribution. Mass transport processes include
surface diffusion, volume diffusion, grain boundary diffusion, viscous flow,
plastic flow, and evaporation-condensation with vapor
transport.
Four snow samples for isothermal metamorphism experiments at different
temperatures were prepared in a similar way and from the same initial
snow. During the whole experiment, except for the short times when the samples were
measured, each sample resided inside a temperature controlled environment.
At the beginning of the experiment and roughly every month during one year,
each sample was analyzed. The visual inspection is shown in the
figure below. For the three warmer samples, rounding of the forms and
coarsening is observed, proceeding at different rates depending on
the temperature. At -54 degrees C, nearly no metamorphism is
seen. These observations are confirmed by structural analysis and are
presented in more detail in Kaempfer and Schneebeli (2007).

Figure:
Evolution of the 3D structure of the ice matrix during isothermal
metamorphism. The samples at temperatures of -1.6. -8.3, -19.1,
-54 degrees C (from left to right) at different
measurement times (0, 34, 75, 118, 162, 211, 317 days) from the
beginning to the end (top to bottom) of the
experiment. The shown cubes are 200x200x200 voxels
(2x2x2 mm) large. Framed images have the same specific surface area.
Heat conductivity
The evolution of the heat conductivity was analyzed for several snow
samples undergoing metamorphism under different conditions
(temperature, temperature gradients) and were published by Schneebeli and
Sokratov (2004).
Publications
[2007] Kaempfer, Th. U. and M. Schneebeli,
Observation of Isothermal Metamorphism
of New Snow and Interpretation as a Sintering Process,
J. Geophys. Res., 112 (2007), D24101,
doi:10.1029/2007JD009047
Preprint as pdf
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[2004] Kaempfer, Th. U., S. A. Sokratov, M. Schneebeli,
The effect of the
structural evolution of snow on heat transfer,
Proceedings of 3rd International Symposium on Two-Phase Flow
Modelling and Experimentation, Pisa, Italy (2004), ed. G. P. Gelata, P. Di Marco,
A. Mariani, R. K. Shah, Edizioni ETS, Pisa, ISBN 88-467-1075-4.
Preprint as pdf
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References
[2004] Schneebeli, M. and Sokratov, S. A.,
Tomography of temperature gradient metamorphism of snow and
associated changes in heat conductivity,
Hydrol. Process.18(18) (2004), pp. 3655-3665, doi:10.1002/hyp.5800
Microstructural Heat Conductivity Simulations through Snow and Firn
Project Summary
Post-doctoral work within the snow physics group of the
Swiss Federal
Institute for Snow and Avalanche Research, SLF, Davos,
Switzerland, under the direction
of Martin Schneebeli. Followup project with Zoe Courville and Mark
Hopkins at CRREL, Hanover, USA, as research scholar through an appointment to the Research
Participation Program admistered by the Oak Ridge Institute
for Science and Education.
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Goal :
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The relation between heat flow through snow and firn
and microstructure is crucial for the comprehension and modeling of
thermophysical, chemical, and mechanical properties of
snow. The accuracy of heat conductivity measurements in the
field using devices as the needle-probe are unclear. We
investigate heat conduction through snow and firn using heat
flux measurements combined with a
microstructural numerical approach.
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Method :
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At SLF Davos, a snow sample subject to a given temperature
gradient can be measured by X-ray micro-tomography (CT) and the heat
flow through it simultaneously measured. At CRREL we have
data-sets of field heat conductivity measurements combined with
CT-images of firn. Simple 3D heat conduction simulations allow
for an assessment of the problems and an investigation of the
relation between microstructure and heat conductivity.
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Collaborators :
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Martin Schneebeli, SLF Davos
Zoe Courville, Mark Hopkins, CRREL Hanover
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Sponsor :
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Swiss National Science Foundation, SLF Davos, Switzerland
United States
Department of the Army AT-24 Research Program
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Duration :
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2003-2006 (SLF), 2007 (CRREL)
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Introduction
Current heat transport models
relate the effective heat conductivity of snow empirically to
the snow density. However, measured heat conductivities differ up to
five times between
measurements made in snow that is similar both in density and in crystal
type. It is thus necessary to find more relevant
parameters related to the snow microstructure that govern
the heat conductivity.
So far, the microstructural complexity always required
simplifications, as for example uniformly packed ice spheres.
Only recently did tomographic reconstructions lead to 3D representations of
the real snow
structure at the micro-scale.
We use the snow microstructure imaged by computed X-ray
micro-tomography (micro-CT) to study heat transport through
snow.
We subject a snow sample to a constant temperature gradient, measure
the passing heat flux, and determine the effective heat
conductivity of the snow. Simultaneously, we
image the snow microstructure by micro-CT, discretized the ice matrix by finite
elements or finite differences, and solve the heat transport equation
corresponding to the experimental
setup.
For firn, we measured the heat conductivity in the field using a
needle-probe and subsequently determined the micro-structure using
micro-CT in the laboratory.
Results

Figure:
Simulation of the temperature distribution during a needle-probe
heat conductivity measurement in
firn. The structural input to the simulation is a micro-tomography
image.
Publications
[2005] Kaempfer, Th. U., M. Schneebeli, S. A. Sokratov,
A Microstructural
Approach to Model Heat Transfer in Snow,
Geophys. Res. Lett., 32, 2005, doi:10,1029/2005GL023873.
Preprint as pdf
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A 3D Microstructure Based Photon Tracking Model
of Radiative
Transfer in Snow
Project Summary
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Goal :
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Solar radiation is a key component of the energy budget of snow
covered landscapes. An understanding of the interaction of solar radiation
with snow is essential to the study of the snow thermodynamics,
chemistry, hydrology, ecology, and remote sensing. We developed a microstructure
based photon tracking algorithm to study radiative transfer in
snow.
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Method :
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The
three-dimensional snow microstructure is provided either by a discrete element
model defined by shape, size, and spatial arrangement of individual ice grains
or by an X-ray micro-tomography image of a snowpack. The model uses refraction,
Fresnel reflection, and absorption laws and the only optical input parameters
are the complex index of refraction and absorption coefficient. The model follows
individual photons through the microstructure, a porous network of ice and air,
applying the fundamental optics laws at the ice-air interfaces and within the
ice. By firing
tens of thousands of photons, a detailed examination of the spectral
radiance and irradiance above, below, and within the snowpack is possible.
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Collaborators :
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Mark Hopkins, Don Perovich, CRREL Hanover
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Sponsor :
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United States
Department of the Army AT-59 Research Program
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Duration :
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2005-2006
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Introduction
Solar radiation is a key component of the energy budget of snow covered landscapes. Even a thin
snow-cover reflects most of the incident sunlight and transmits little. An understanding of the
interaction of solar radiation with snow is essential to the study of the thermodynamics,
chemistry, hydrology, ecology, and remote sensing of snow covered sea ice or
landscapes.
To
investigate this interaction we developed a microstructure based photon tracking algorithm.
The
three-dimensional snow microstructure is provided either by a discrete element
snow model or by an X-ray micro-tomography (micro-CT) image of a snowpack. The
model uses refraction,
Fresnel reflection, and absorption laws and the optical input parameters
are only the complex index of refraction and absorption coefficient. The model follows
individual photons through the microstructure,
applying the fundamental optics laws at the ice-air interfaces and within the
ice. By firing
tens of thousands of photons, a detailed examination of the spectral
radiance and irradiance above, below, and within the snowpack is possible.
Methods
Snow representation
Discrete element modeling (DEM) is a technique for explicitly modeling the dynamics of
assemblies of grains and allows for the use of
complex particle contact physics. In particular, by
defining appropriate collision rules, the DEM handles naturally the
travel of a photon through an
ice matrix formed of sintered snow grains. Our microstructural snow
model is based on a DEM approach that uses
axisymmetric particle shapes and is ideal for an efficient study of
the impact of physical properties
such as mean grain size or density on the optical properties.
The photon tracking model can be applied to non-regular particle
shapes and to experimentally imaged
snow by using a more universal 3D representation, a binary voxel (3D pixel)
image. This
is typically the image format produced by a micro-CT
scan. However, a voxel representation
cannot be directly used for optical
computations due to the staggered ice-air interfaces. A smoothing
algorithm applied to the ice-air interface overcomes this problem.

Figure:
Left: 3D representations of a model snow sample (from top, clock-wise): Cylindrical DEM, with
triangulated surface, voxel representation, and voxel based triangulation
after smoothing. DEM grain radius is 0.5 mm. Right: micro-CT image of
snow with small rounded grains and density of
170 kg m-3, after smoothing the ice-air interfaces (resolution
40 micro-m, side length of cube 4 mm).
Modeling light transmission through snow
At visible and near infrared wavelengths, radiative transfer in snow is governed by two
processes: absorption and scattering. Absorption is well
understood and has a strong wavelength dependence. Scattering in snow results
from differences in the real indices of
refraction, n, between ice ( n ~ 1.31) and
air ( n ~ 1.0), with little
wavelength dependence but strong coupling to the intricate and highly
variable microstructure. There has been considerable theoretical work on
scattering in snow and it is typically represented by
parameterizations.
For the wavelength considered the snow grain radii are much larger than the
wavelength size parameter and we can model light transmission through snow
using a photon tracking approach. We consider a ray of given initial
irradiance and incident zenith angle as an assembly of
photons. The interaction of the ray with a single
snow grain (Figure) is
governed by the following optical laws.
These laws are implemented in a probabilistic sense and to model a ray of
light a large number of photons (typically 10000) is
fired into the snowpack. Ultimately, each photon
has three possible fates: exit at the top, exit at the bottom, or be absorbed
inside the sample.
The input parameters needed for the model are the complex index of refraction
for ice and the angle, intensity, and position of the incident ray.

Figure:
Left: Schematic of ray tracing for an incident ray on a single
grain (real numbers = radiance, integers = # photons/1000). Right:
Photon tracking at 470 nm (yellow) and 1000 nm
(red) through a
cylindrical DEM snowpack.
Results
Results from the photon tracking model were compared to a 4 stream discrete
ordinates model that has been validated against observations (Figure). We used
spherical particles with 0.5 mm radius as well as cylindrical
particles.

Figure:
Photon tracking (PT) compared to a 4-stream discrete ordinates
method continuum model (sample density 270 kg m-3,
snowpack thickness 7.8 cm, incidence angle 60 degrees).
The photon tracking model, with its ability to examine in detail the angular distribution of
reflected light, is also well suited for studies of the
reflectance distribution function (Figure). This study can represent
the direct solar beam on a
sunny day or the beam from a laser altimeter. The typical forward scattering
of snow is predicted.

Figure:
The directional-conical reflectance factor (DCRF) at
470 and 900 nm for incidence zenith angles
of zero and 65 degrees. The model was run on a spherical DEM model snowpack
with grain radius of 0.1 mm, a density of 270 kg m-3, and a depth of 30 cm.
Publications
[2007] Kaempfer, Th. U., M. A. Hopkins, D. K. Perovich,
A 3D Microstructure
Based Photon Tracking Model of Radiative Transfer in Snow,
J. Geophys. Res., 112, 2007, doi:10.1029/2006JD008239.
Preprint as pdf
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Modeling Heat and Mass Transfer in Snow at a Microstructural
Level
using a
Phase-Field Approach
Project Summary
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Goal :
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Snow is a highly porous medium consisting of an ice matrix and porous space
containing water vapor. With time, snow undergoes metamorphism and its
microstructure evolves. There is a strong interaction between the snow
microstructure and snow pack properties. Recently, computed X-ray micro-tomography
emerged as a tool to observe snow metamorphism at a
microstructural scale. A numerical model operating at similar length
scales and based on fundamental physics is highly desirable to study
metamorphism in detail.
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Method :
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Snow metamorphism under an imposed temperature gradient is governed by heat and
mass conservation laws, with possible phase change at ice-air
interfaces. We use a phase field model that treats the multi-phase system with
complicated interface
conditions by tackling the problem continuously, inclusive of the interfacial
region. This approach overcomes the problems associated with topology
changes commonly found in interface tracking methods.
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Collaborators :
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Mathis Plapp, Ecole Polytechnique, Paris, France
Mark Hopkins, CRREL Hanover
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Sponsor :
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United States
Department of the Army Fundamental Research Program
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Duration :
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ongoing
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Introduction
Snow is a highly porous medium consisting of an ice matrix and porous space
containing water vapor. With time, snow undergoes metamorphism and its
microstructure evolves. There is a strong interaction between the snow
microstructure and snow pack properties. Understanding snow metamorphism is
thus crucial for predicting mechanical properties used in avalanche
forecasting, chemical composition associated with the interpretation of ice
cores data, or thermophysical properties important for modeling the energy
balance of snow-covered landscapes. The link between heat transport and
metamorphism is particularly strong. On the one hand, heat flow through snow
induces mass flow and thus an evolution of the ice-pore network (Figure); on the other
hand, the microstructure influences heat flow as heat transport is governed by
conduction in the ice and pores as well as phase change processes and water
vapor transport in the pore space.

Figure:
Difference of two micro-tomography images of a snowpack evolving
under a temperature gradient: the temperature gradient induces a water vapor gradient in
the pore space that drives mass flow (blue represents sublimated,
green freshly condensated ice during one day).
Phase field models treat multi-phase systems with complicated interface
conditions by tackling the problem continuously, inclusive of the interfacial
region). This continuous variation across the interface is realized
using an order parameter, the phase field function, which describes the phases
thermodynamically.

Figure:
Sharp interface (left) and diffuse interface (right) with the phase
field function phi.
In a classical formulation the basic equations have to be written for each
medium and the interface boundary conditions must be explicitly tracked. In
diffuse-interface theory the basic equations, with supplementary phase field
terms, are deduced from a free energy functional for the whole system and
interface conditions do not occur. In fact, they are replaced by a partial
differential equation for the phase field.
Methods
Snow metamorphism under an imposed temperature gradient is governed by heat and
mass conservation laws, with possible phase change at ice-air interfaces. In
the diffuse interface approach, we use the phase field function to continuously
express the physical parameters as the heat conductivity or water
vapor diffusivity by interpolation. The conservation equations,
including one for the phase field parameter, are deduced from a free
energy functional of the two-phase system.
Results
We applied the phase-field model to a
2D section of an X-ray micro-tomography image of natural snow. We extracted a 3
voxel thick section from the tomography image (Figure) and combined it into one
plane to obtain the computational domain.

Figure:
Construction of 2D computational domain.by extracting and combining 3
slices of an X-ray micro-tomography image of snow.
We subjected the snow sample to a vertical temperature gradient of and observed
the heat and mass fluxes and the evolution of the ice-matrix.
The temperature distribution is considerably disturbed from a linear one, due
to the different heat conductivities of ice and air (Figure, left). Even though
the ice matrix is not fully connected, we observe that the heat fluxes
concentrate along the ice structure (Figure, center). Moreover, strong
inhomogeneities in the heat fluxes in the pore space are observed, leading
consequently to similar inhomogeneities in the induced water vapor fluxes. Such
effects have also to be expected in 3D. Using the phase field function , we can
easily follow the microstructural evolution including topological changes and
identify regions where the ice matrix sublimates or regions of crystal growth
(Figure, right).

Figure:
Phase field computation on a 2D slice of tomographed snow: A vertical
temperature gradient was imposed, the ice matrix is shown in overlayed white.
Temperature distribution (left), heat fluxes (center), and ice matrix after one
day compared to the initial condition (right).
Publications
[2007] Kaempfer, Th. U. and M. Plapp,
Modeling Heat and Mass Transfer in Snow at a Microstructural Level using a
Phase-Field Approach - First Results,
Proceedings of the 64th Annual Meeting of the Eastern Snow
Conference (2007), May 2007, St. Johns, Newfoundland, Canada.
Preprint as pdf
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[2009] Kaempfer, Th. U. and M. Plapp,
Phase-field modeling of dry snow metamorphism,
Phys. Rev. E, 79, 2009, doi:10.1103/PhysRevE.79.031502.
Preprint as pdf
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Modeling of Destructive Metamorphism in Thin Snow and Impact
on Optical Snow Properties.
Project Summary
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Goal :
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We extend our micro-structure based snow model to include
sintering mechanisms as grain-boudary and surface diffusion
on an grain-scale level. These mechanisms become dominant in a
snow-pack under
little or no temperature gradient and are also particularly
important during the initial, destructive metamorphism from
dendritic to rounded grain snow. The impact of destructive
snow metamorphism on the physical properties of a snow pack with
emphasis on optical properties will be studied.
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Method :
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Multi-phase field models are emerging for the simulation of sintering
powder particles. We will apply and further develop such models for metamorphosing
snow and we will couple them to the existing heat and mass transfer
model and the discrete element and optics modeling framework.
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Collaborators :
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Mark Hopkins, CRREL Hanover
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Sponsor :
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United States
Department of the Army Fundamental Research Program
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Duration :
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ongoing
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