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International Journal of Fieldwork
Studies, 2003 1 (1)
An Experimental Optical Instrument for the Determination
of Snow Accumulation in Alpine Environments
Derrick J. Lampkin
Department of Geography and Regional Development,
Department of Hydrology and Water Resources, University of Arizona,
Building 11, University of Arizona, Tucson, Arizona, United States.
Abstract
Variability in regional climate can affect snow
covered amount, and timing of water yields. Substantial changes
in regional snow cover extent can have an impact on the availability
of water resources in the Southwest U.S. There is a need for improved
ground-based instrumentation that can monitor snow accumulation
distribution across spatial scales ranging from a meter to tens
of square meters in area. An experimental, prototype instrument
was developed to monitor ground accumulated snow using coupled optics
and voltage measuring sensors. The system was deployed on January
29, 2002 and March 18, 2002 atop Mt. Bigelow in the Santa Catalina
Range, north of Tucson, Arizona. Results indicate that snow accumulation
equal to or greater than 3cm occurred on the January 2002 deployment
at the Ecm1 site. This was validated by the sonic depth sounder
measuring ~ 2cm of snow at the Wtm2 site. Results during the March
test indicate little accumulation and subsequent melt at Ecm1 site.
Near surface air temperature, coupled with relative humidity, net
radiation, and near surface soil temperature at Ecm1, indicate conditions
were sufficient for accumulation and ablation of snow.
Key Words
Alpine Snow Cover, Instrumentation, Snow Hydrology, Optical
sensor, Experimental, Alpine Vegetation
Résumé
Variabilité dans les climats regionaux peut affecter la
couverture de neige, et le timing des rendements d'eau. Changements
substantiaux dans la couverture regionale de neige peuvent avoir
un impact sur la disponibilité de resources d'eau dan le
sud-ouest des États-Unis. Un instrument est necessaire pour
controler l'accumulation de neige à travers sur des superficies
d'un mètre à des dizaines de mètres carrés.
Un prototype experimental a été developpé pour
contrôler la neige accumulé qui utilise des détecteurs
voltaïque et optique couplé. Le system a été
déployé le 29 janvier 2002 and le 19 mars 2002 sur
le mont Bigelow dans les montagnes Santa Catalina au nord de Tucson,
Arizona. Les résultats indiquent que l'accumulation était
equivalente à 3cm ou plus pendant le déployement du
janvier 2002 au site ECm1. Ces résultats ont été
validés par des mesures en profondeur soniques de approximativement
2cm au site Wtm2. Les résultats du test de mars
indiquent peu d'accumulation et fonte subséquente au site
ECm1. La température au sol, l'humidité relative,
la radiation nette, la température du sol á la surface
au site Ecm1 indiquent que les conditions étaient suffisantes
pour de l'accumulation et de l'ablation de neige.
Mots clefs
Couverture de neige alpine, Instrumentation,
Hydrologie de neige, Détecteur optique, Experimental, Végétation
alpine
Rezumat
Diferentele regionale climatice pot afecta
grosimea stratului de zapada, si periodicitatea topirii acesteia.Schimbarile
regionale substantiale la nivelul extinderii stratului de zapada
pot avea impact asupra resurselor de apa din sud-vestul Statelor
Unite. Exista necesitatea imbunatatirii echipamentului de sol in
vederea monitorizarii distributiei acumularilor de zapada pe suprafete
incepand cu cele de un metru patrat pana la cele de zeci de metri
patrati dintr-o zona. A fost pus la punct un instrument prototip,
care monitorizeaza experimental acumularile de zapada la sol, utilizand
senzori optici si de masurare voltaica. Sistemul a fost pus in functiune
pe 29 Ianuarie 2002 si pe 18 Martie 2002 pe varfulBigelow din lantul
Santa Catalina, nordul Tucson, Arizona. Rezultatele indica faptul
ca acumularile de zapada din Ianuarie 2002 se afla in jurul valorii
de 3 cm sau peste la locatia Ecm1. Acestea au fost validate prin
masuratori sonice care au indicat 2 cm de zapada la locatia Wtm2.
Rezultatele testului din Martie 2002 indica acumulari mai mici si
topiri subsecvente la locatia Ecm1. Temperatura aerului la nivelul
stratului de zapada impreuna cu umiditatea relativa, radiatia neta,
temperatura aerului la nivelul solului la Ecm1 au indicat conditii
suficiente pentru acumulare de zapada si ablatie.
Cuvinte cheie
Strat de zapada alpin, Instrumente, Hidrologia zapezii, Sensor
optic, Experiment, Vegetatie alpina
Introduction
An understanding of global and regional changes in climate and
the assessment of water resources requires that we monitor the temporal
and spatial variability of snow cover from local to global scales
(Dozier, 1989). Seasonal snow cover comprises about 30% of the Earth's
land surface, while 10% is perennial cover by glaciers (Dozier,
1989). Variability in regional snowfall can be indicative of changes
in the Earth's global climate.
Frozen reservoirs of water in alpine environments of the mid-latitudes
are important in the management of water resources, particularly
in locations such as the southwestern United States. Substantial
changes in regional snow cover extent can have an impact on the
availability of water resources in the Southwest. A thorough understanding
of various characteristics about alpine snow cover, such as density,
depth, accumulation, and temporal variation in extent, are vital
to the effective management of this resource.
There are established methods for assessing snow cover characteristics.
Alpine snow cover data have been collected by various field-based
methods. These methods include snow gauges to measure snow water
equivalence, graduated stakes and aerial markers to capture snow
depth, automated data collection apparatus, manual data acquisition,
and snow surveys (Goodison et. al., 1981). Current field-based techniques
for determining snow accumulation, suffer from a lack of either
spatial or temporal resolution. This research will improve acquisition
of snow accumulation data through the use of an automated optical
system, which will use a coupled laser-sensor system. The system,
composed of these fundamental components, can be replicated to assess
an integrated depth of accumulation across an area.
Background
Optical methods have been used to capture information about alpine
snow cover. Lundberg and Johansson (1994) used two pairs of transmitter-receivers
fashioned from a light-diode and photo-detector. They were designed
to monitor and discriminate solid phase precipitation. Warren and
Gunn (1968) used a pulsed light source detector to estimate hourly
snow accumulation. Their work involved the use of a pulsed light
source operating in the visible region of the EM spectrum with peak
intensity at 0.45µm. A transmitter and receiver were arranged
between two buildings with a distance of 71 m and elevated 20m above
ground. Warner and Gunn's (1968) work extended the work of Lillesaeter
(1965), which involved the use of a narrow light beam and receiver
to determine an empirical relationship between beam attenuation
and the extinction. Lundberg and Johansson (1994), Warren and Gunn
(1968) and Lilleseater (1965) used optically instruments to determine
solid phase of precipitation, but failed to record information about
snow accumulation on the ground.
Method
a) Theoretical Basis and Design
The instrument uses a laser that operates in the 630-680nm range
of the electromagnetic spectrum (EM). The basic component of the
system is a laser/sensor array, which measures snow accumulation
through ground-accumulated snow interrupting the beam, causing a
subsequent drop in measured voltage, over moderate spatial and temporal
resolutions. The instrument does not measure particle type or snowfall,
but strictly ground-accumulated snow. Additionally, the prototype
system cannot resolve accumulations derived from lateral redistribution
of snow due to wind flow. Therefore, all measurements effectively
represent peak accumulation between laser and sensor towers, derived
from vertical input from the atmosphere, as well as canopy intercepted
snow fall, and laterally redistributed accumulations. Separating
measurements into their constituent input components will be a focus
of future work.

Figure 1. Characteristic growth modes of columnar
and planar ice crystals from Ono, (1970).
A primary concern regarding such a system is its degree of sensitivity
to accumulating snow grains, which vary in size and accumulation
rate. Precipitating ice crystals form as small hexagonal plates
that can grow along the six prism faces (a-axis) or perpendicularly
along the two basal planes (c-axis) (Fassnacht et. al., 1999). Work
by Ono (1970), describes the change of ice crystal shape with temperature.
Plates, stellar, and dendrites grow along the a-axis, while columns
and needle-shaped crystals grow primarily along the c-axis (Fassnacht
et. al., 1999). The range of values for lengths in both the a and
c axis directions illustrate that the laser wave front would be
sensitive to falling snow. The lower range for the c axis is ~ 0.01mm
(10,000nm) at -7 degrees C and 0.08mm (80,000nm) along the a-axis
(see Figure 1). At this temperature, the smallest dimension along
the c-axis of precipitating snow crystals is 16 times larger than
the laser wave front and 127 times larger along the a-axis. The
instrument should theoretically be sensitive to the attenuation
of the laser beam by accumulated particles within the 630-680nm
range of the EM spectrum, as a result of snow's low transmission
and absorption relative to its high reflectance within the dynamic
range of the laser. Figure 2 displays the basic design of the optical
snow accumulation instrument. The system is composed of an array
of lasers set at user-specified heights above the ground. Each laser
is set to a corresponding light-sensitive sensor, which measures
changes in an amplified voltage derived from an illumined solar
cell. As snow accumulates, each beam is interrupted with a corresponding
decline in sensor voltage. The optical component houses a switch,
and laser diode. The sensor apparatus is composed of a silicon-based
solar cell, which is routed to an operational amplifier as well
as two adjustable resistors (potentiometers). The potentiometers
are used to set limits on the minimum and maximum amplified output
voltage. The laser signal received by the solar cell is amplified
and output voltage is logged by an ONSET HOBO VOLT® data logger.

Figure 2. Conceptual design of the optical system.
Laser and sensor casing dimensions (31cm x 31cm x 16cm) with laser
and sensor instruments contained with protective weather casings.
b) Field Measurements
A single laser-sensor system was deployed in the Santa Catalina
Mountain Range just North of metropolitan Tucson, Arizona. Figure
3 illustrates a map of sites for the deployment of the system. Each
site corresponds to a location of a micro-meterological tower erected
and maintain by Sustainability of Semi-arid Hydrology and Riparian
Areas (SAHRA). Each site contains array of instruments designed
to monitor and quantify hydrometerological fluxes in alpine environments.
Table 1 summarizes the instruments deployed at both the Wtm2 and
Ecm1 sites. The optical sensor was deployed on January 29, 2002
and March 18, 2002 at the Ecm1 site. This site was selected because
it was at the highest elevation and most accessible of all the available
locations. Additionally, the Ecm1 site is a little more than a kilometer
south of the Wtm2 site. Unfortunately, the Ecm1 site's resident
sonic snow depth sounder experienced malfunctions due to tower proximity
to commercial high frequency radio communication towers. Therefore,
snow depth information from the nearest tower to the Ecm1 (Wtm2)
was used to validate the optical instrument measurements.

Figure 3. Topographic map displaying locations
of SAHRA micro-meteorological towers and optical system test site.
Data from WTm2 tower were used to validate optical system results
collected at the ECm1 Site. Map projected in UTM (zone 12). Contour
intervals set at 150 metres.
The optical array was deployed on January 29, 2002 at the ECm1
site at 5:30pm. The single coupled sensor/laser system sits ~ 3cm
above the snow-free surface. Therefore, the lowest resolvable measure
of snow accumulation is ~ 3cm. Any accumulation less than this amount
will not be detected by the system. The datalogger attached to the
sensor and housed within the sensor module was set with a sampling
interval every 0.5 seconds for 1 hour and 15 minutes. This high
sampling rate was mistakenly set due to operator's error, when deploying
the datalogger. The high sampling rate facilitated an increase in
accuracy in temporal resolution, but restricted monitoring through
the entire accumulation event. The laser /sensor modules were deployed
in January 2002, approximately 78cm apart and a distance of 8 meters
south from the micrometeorological tower, near the edge of a clearing
in the canopy. The system was orientated with the sensor tower facing
towards the northwest, while the laser tower was aimed at the sensor
housing with an orientation towards the southeast. The data was
retrieved on January 30, 2002. Deployment of the instrument on March
18, 2002 was at the Ecm1 site with the sensor tower facing due north,
while the laser tower was facing south. The system was placed at
the southeastern edge of the forest clearing about 10 meters south
of the SAHRA instrument tower. The system was activated at 7:00pm
on March 18, 2002 with a total sampling rate every 5 minutes. The
site was characterized by bare ground with a small patch of ice
less than 2cm thick on the southwest edge of the canopy clearing.
The data was retrieved on March 19, 2002.
| Instrument |
Description |
| Air Temperature Relative Humidity |
Model HMP45C temperature & relative humidity
(produced by Vaisala): Sensor mounted inside an RM Young 12
plate Gill Radiation Shield. Sensor Height : a.g.l. 2.74 m |
| Surface Temperature Sensor |
Model Precision Infrared Thermometer (produces
by Apogee): Mounted at an angle using a movable camera mount
Sensor Height: a.g.l. 1.72m perpendicular 2.15 m hypotenuse |
| Wind Speed/Direction |
Model 3001-L Wind Monitor (produced by RM
Young)) : Sensor Height: a.g.l. 3.04 m |
| Net Radiometer |
Model NR-Lite (produced by Kipp& Zonen)
: Domeless Sensor Height: a.g.l. 1.52 m |
| Snow Depth Sensor |
Model SR50-L Ultra Sonic Distance Sensor
(produced by Campbell Scientific): Range: -45 to + 50O C The
snow depth sensor is mounted off of a horizontal arm clamped
to the tower. Sensor Face Height: a.g.l. 2.54 m |
| Soil Thermocouple Array |
Custom soil thermocouple probe (produced
by NOAA Lab) Sensor array has 7 probes. At surface, 2,4,8,16,32,64
cm b.g.s. |
| TDR Probes |
Model CS615 Water Content Reflectometers
(produced by Campbell Scientific ) Sensors are buried ~3.35m
from tower & 0.91m and 1.82m from trees Probe #1 buried
horizontally at 6 cm. b.g.l. in dark Organic Layer Probe #2
buried horizontally at 15 cm. b.g.l. in light colored soil low
in organic matter |
| Barometric Pressure Sensor |
|
Table1. Instruments mounted at SAHRA micro-meteorological
stations
Results
and Discussion
Figure 4 displays results from the optical instrument as well as
validation data from the Wtm2 snow depth sounder and the Ecm1 air
temperature probe for the January 29, 2002 deployment. The air temperature
at the Ecm1 site demonstrates a significant decline with values
dropping below zero. This drop occurs during an increase in snow
depth as measured by the sonic depth sounder at the Wtm2 site. Simultaneously,
there was a significant decline in voltage as measured by the optical
instrument at the Ecm1 site. A substantial decline in voltage occurred
at about 5:16pm. This decline, indicative of a substantial amount
of accumulated snow, is validated by an increase in sonic snow depth
sounder measurements at the Wtm2 site.

Figure 4. Graph of results from 1-29-02 deployment
at the ECm1
site as a function of time, averaged over 15 minute intervals: A)
air temperature from ECm1 tower, B) Snow depth measured at WTm2
site, C) Voltage measured by optical system at ECm1 site.
Results from the March 18, 2002 deployment were more complex. The
site during retrieval was characterized by bare ground, with no
snow present between the laser and sensor towers. There was present
a dusting of snow, less than 1cm, covering the patch of ice that
was present pre-deployment. The soil between the instrument towers
and within the canopy was damp. The sonic depth sounder at the Wtm2
site was of no use as a validation data set because the amount of
accumulation, if any was less than (accumulation < 3cm) the sensor's
ability to detect snow without substantial errors. Therefore, the
use of other data derived from the Ecm1 met tower, such as air temperature,
relative humidity, surface soil temperature, and net radiation were
used to validate the optical instrument results. Figure 5 displays
graphs of optical instrument voltage, as well as the previously
mentioned data as a function of time during the course of the instrument
deployment period. This demonstrates a decline in optical meter
voltage for approximately a two-hour period (13:45-15:45) on March
20th. The decline in voltage was followed by an increase in near
surface air temperature above (0) degrees. During this period there
was a 16% increase in relative humidity. There was also a decline
in net radiation during this period with a negative net radiation
of (-9.0 W/m^2) at 14:30). High relative humidity with rising, but
below freezing temperatures as well as a decline in net radiation,
could indicate conditions that support some snow accumulation. The
two-hour period from 15:45 to 17:45 is marked by a sharp increase
in sensor voltage, ideally indicative of melting accumulated snow
cover. During this time period, near surface soil temperature demonstrates
a sharp increase, while simultaneously the net radiation is low,
but remains positive. For a 3cm thick snow pack, there may have
been a sufficient amount of radiation to melt it, supported by an
increase in near surface soil temperature, possibly brought on by
the onset of percolating warmer melt water. Assuming the equivalent
amount of water within a 3cm depth snow pack for a square centimeter
area is approximately 1gram and given that the conventional latent
heat of fusion for ice would be (79.7 cal/g), an upper estimate
for the amount of energy required to ripen the 3cm thick snow pack
would be estimated as 18W/m2 over the 2 hour period. This is derived
neglecting the volumetric water content. At 16:00h, the net radiation
was about 13 W/m^2. There appears to have been a sufficient amount
of energy to melt the existing snow pack during the time period
that the instrument measured an increase in voltage.

Figure 5. Graph of results from 3-18-02 deployment
at the ECm1 site as a function of time, averaged over 15 minute
intervals: A) air temperature from ECm1 tower, B) soil temperature
from ECm1 tower, C) relative humidity from ECm1 tower, D) net radiation
from ECm1 tower, and E) Voltage measured by optical system at ECm1
site.
Conclusion
The application of an optical based instrument for the determination
of snow accumulation in alpine environments seems plausible. The
prototype instrument composed of a single coupled sensor-laser system,
demonstrated a level of sensitivity required to monitor accumulation
events in the Santa Catalina Mountain Range north of Tucson, Arizona.
The laser, which operated between 630-680nm, was sufficiently attenuated
by snow accumulation measured on January 29, 2002 and March 18,
2002. Ancillary meteorological data acquired during the optical
instrument deployments, confirmed the timing and degree of accumulation
and melt measure by the prototype system.
Development of the system from prototype to operational status
will require several further steps. Short-term goals will involve
laboratory/cold-room testing and calibration of the prototype, improvements
in sensor and field design, as well as expanding the system field
tests using more components. Additionally, a single sensor will
be deployed to determine the influence of diurnal fluctuation of
the incoming radiation field on measured voltages. Intermediate
goals will involve a greater emphasis on the improvement of the
circuit design, as well as more controlled field tests. Intermediate
field exercises will involve acquisition of meteorological data
in conjunction with an expanded sensor/laser network. Several questions
could be addressed by the optical system: Can the optical instrument
improve our understanding of how alpine vegetation canopy influences
the spatial distribution of snow accumulation? How does the near-surface
radiation budget vary as a function of snow accumulation in an alpine
vegetated environment? The optical system coupled with meteorological
data could address to what degree is soil moisture influenced by
successive snow accumulation events?
Acknowledgments
I would like to thank the American Alpine Club, and the College
of Social and Behavioral Science Department at the University of
Arizona for their financial support of this project. I would like
to also thank SAHRA for access to the meteorological data and facilities.
I'd also like to thank Dr. S. Fassnacht for his support.
References
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Goodison, B.E., Ferguson, H.L., and McKay, G.A., Measurement and
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of snow: Principles, Process, Management and Use. Pergamon Press,
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Lillesaeter, O., 1965. Parallel-beam attenuation of light, particularly
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Please cite this paper as:
Lampkin, D.J. (2003) An Experimental Optical Instrument for the
Determination of Snow Accumulation in Alpine Environments, International
Journal of Fieldwork Studies, 1 (1), http://www.virtualmontana.org/ejournal/vol1(1)/snow.htm
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