Diurnal Variation of Soil Heat Flux at an Antarctic Local Area during Warmer Months
Soil heat flux () is one term in the energy balance equation, and it can be particularly important in regions with arid, bare, or thinly vegetated soil surfaces. However, in remote areas such as the Antarctic, this measurement is not routinely performed. The analysis of observational data collected by the ETA Project at the Brazilian Antarctic Station from December 2013 to March 2014 showed that, for the total daily energy flux, the surface soil flux heats the deeper soil layers during December and January and acts as a heat source to the outer soil layers during February and March. With regard to daytime energy flux, acts as a source of heat to the deeper layers. During the night-time, the soil is a heat source to the shallower soil layers and represents at least 29% of the net night-time radiation. A relatively simple method—the objective hysteresis method (OHM)—was successfully applied to determine the surface soil heat flux using net radiation observations. A priori, the OHM coefficients obtained in this study may only be used for short-time parameterizations and for filling data gaps at this specific site.
Energy from the Sun plays an important role in climatic systems as a whole and a specific role in the Earth’s radiation balance. Net radiation and soil heat flux provide the energy for sensible and latent atmospheric turbulent heat fluxes near the surface.
Surface soil heat flux (), defined as the heat exchange between different soil depths, with each layer possessing different temperature values , is a particularly important component of surface energy in regions with arid, bare, or thinly vegetated soil surfaces due to its capacity to work seasonally as a heat source (winter season) or a heat sink (summer season) [2–4]. Therefore, accuracy in the estimation of is important to atmospheric systems . However, such estimates are not readily available, particularly in locations such as the Antarctic, which possesses extreme climatic conditions for measurements in situ and heterogeneity in surface properties.
Bare soils generally have low albedo, whereas ice-covered soils show high albedo [6, 7]. Consequently, these soil types will have different soil temperatures even when in proximity to one another. For this reason, changes in Antarctic soil coverage can lead to local variation in temperature, directly affecting the Antarctic ecosystem .
Prosek et al.  investigating the components of energy balance in a vegetated oasis at the Polish Station (King George Island, Antarctic region) have found that the boundary atmosphere and the soil substrate represent the basic components of the ecotopes of the Antarctic vegetation oasis.
Sturm et al.  discussed the warming in Alaska, of 0.5°C per decade in the last 30 years, and the positive feedback involving biological processes in the winter soil, which have contributed to the conversion of tundra to shrubland.
The objective hysteresis method (OHM) was proposed by Camuffo and Bernardi  to estimate using values of . The OHM model was initially developed for urban areas in an attempt to estimate urban heat storage as a residual term with different sources/sinks of energy such as buildings, vegetation, and the ground responsible for the exchange of sensible and latent heat fluxes [21–23]. However, there is nothing in the formulation of the OHM that limits its application only to urban areas.
This study uses a method of hysteresis to estimate soil heat flux and compare these estimates to direct measurements performed at the Brazilian Antarctic Station “Comandante Ferraz” (EACF) from December 2013 to March 2014. The data used in this study was collected by the ETA Project (Estudo da Turbulência na Região Antártica). To our knowledge, this is the first application of this method to the EACF region. Most of the previously published values are for urban areas and they are not valid for the studied region and time period.
2. Materials and Methods
The measurements were performed at the EACF (62°05′07′′S, 58°23′33′′W, 20 m above mean sea level) at a micrometeorological tower, located on King George Island, which is part of the South Shetland Islands of the Antarctic Peninsula (Figure 1).
The micrometeorological tower is surrounded by surface of different characteristics. Figure 2 presents an overview of the investigated area and shows the soil cover commonly observed, varying from bare soil to snow-covered soil.
During warmer months, the surface is covered mostly by bare soil, with presence of diverse sizes of rocks and gravels (<1 m in width). The occurrence of snow due to atmospheric systems, in these months, is unavailable. Nearby the tower there is a lake (<10 m), commonly frozen during the year, except on some days of summer.
The data used in this study were collected in situ from December 2013 to March 2014 (the warmer months). The net radiation data were obtained using a NR Lite2 Net Radiometer installed in a micrometeorological tower (3.4 m in height, Figures 3(a) and 3(c)) and the surface soil heat flux was measured using a Hukseflux HFP01 at a depth of 0.05 m (Figure 3(b)). The air temperature was measured by temperature sensor Model CS215, mounted with a 6-plate radiation shield, installed at 2.2 m height. The plate louvered construction allows air to pass freely through the shield, serving to keep the probe at or near ambient temperature. The shield’s white colour reflects solar radiation. The soil temperature was measured using a probe 107L at 0.05 m depth. All sensors used in this work are from Campbell Scientific Inc.
The data were stored at 5 min (average) intervals by a CR5000 data logger (Campbell Scientific Inc.) using the local time ( UTC) as the standard time (Figure 3). The data logger was connected to a laptop that automatically transmitted the data, every 30 min, to the Air-Sea Interaction Laboratory at IAG, USP. All data were reviewed and questionable data were removed considering the values located out of the 2-standard-deviation interval centred on the average value of the investigated variable.
The sign convention used for this study is that and are positive when energy is moving up in agreement with the vertical coordinate .
2.1. The Objective Hysteresis Method and Statistical Evaluation of the OHM Application
The estimation of using the objective hysteresis method (OHM) was based on the expression given by where , , and are empirical coefficients related to the response of the surface properties due to solar energy and is the temporal variation of at the surface, discretized in time as . The and coefficients describe the best-fit straight line for the data over the entire day and are therefore constants. The slope of the best-fit straight line is represented by and the intercept with the ordinate is represented by . The coefficient indicates the departure of actual values from the best-fit straight line.
The coefficients play different roles in the equation: is dimensionless and always positive and indicates the intensity of the relation between and ; (s) shows the magnitude of the hysteresis, indicating the direction and the degree of the phase relationship between and . In summary, and are coefficients related to the mean values resulting from the soil characteristics (including the presence of water) and to the magnitude of with its temporal variation .
The coefficient (Wm−2) may be negative or positive depending on the local atmospheric conditions, and it represents the spontaneous heat flux between the soil and the adjacent atmosphere, when and approach zero. In other words, this term represents the average heat flux released from the soil during the transitional periods of the day [20, 22, 24].
Statistical tests were performed to evaluate the application of the OHM model to the EACF region, including a linear regression with slope and intercept, coefficient of determination (), root mean square error (RMSE), and the mean absolute error (MAE).
represents the percentage of the data that is close to the line of the best fit; these variances can be understood by the regression model . The coefficient is given bywhere is the total number of observations, is the “” observation value, and is the “” modelled result. The overbar denotes the time average for the period of evaluation. ranges from 0 to 1, with values near 1 indicating a good fit of the modelled results.
In general, the RMSE is greater than or equal to the MAE for the range of most values because the MAE is less sensitive to extreme values than the RMSE.
3. Results and Discussion
The soil temperature, during the investigated period, was always higher than the air temperature, as observed in cold regions . January presented higher air and soil temperatures with a diurnal amplitude around, respectively, 1.4°C and 5.4°C (Figure 4). Among the investigated months, the diurnal variation of the soil temperature presented larger amplitudes than the air temperature, with maximum amplitude in December in both cases. Unfortunately, there is no data available during the investigated months directly related to the snow presence (surface albedo and emissivity, latent heat, etc.) but, in general, large soil temperature amplitude is characteristic of bare soil. During February and March most of the air temperature values were below zero and the diurnal amplitudes of the soil temperatures are comparatively smaller which could indicate the snow presence during these months. Previous studies have indicated that a characteristic of snow cover would be a long period of relatively stable soil temperatures with smaller amplitude of the temperature signal [13, 29].
Through all investigated months there was a delay between and during the two periods of the day corresponding to the transitional day/night/day periods when the signal of and are inverted, with the soil acting as a source of heat to the shallower soil layers and as a source of heat to the soil (Figure 5).
In general, during the daytime, the energy provided by is shared between and the turbulent fluxes, but during the night-time, the turbulent fluxes are less important and represents a comparatively larger portion of the net radiation. Therefore, at night, the soil played an important role as an energy source to the outer soil layers accounting for approximately 31% of in March and up to approximately 55% of in December (Table 1, Figure 6). High values of occurred near the transitional periods, when was low but, near noon, was approximately 10% of (Figure 6) as observed by several authors in different locations [30, 31].
During the daytime of the studied period, part of the net energy was stored in the soil, with maximum storage of approximately 7.6% observed in December (Table 1). During January, the quantity of net radiation energy flux incident on the surface was more than twice the quantity of incident energy during February, but the proportion of energy stored in the soil was not so different.
In the EACF region, the daily ratio of varied from 4.3% in December to −17.6% in March (Table 1) with the soil acting as a heat source to the deeper soil layers during December and January (positive values of ) and as a source of heat to the shallower soil layers (negative values of ) during February and March (Table 1).
The best-fit coefficients for the investigated months are shown in Table 2 and, a priori, these values are valid for this particular site during this period of study because these coefficients are related to the presence of precipitation, atmospheric system, soil state, and soil characteristics. Using these coefficients (Table 2), the OHM was able to simulate the diurnal variation of during the investigated months, as displayed in Figure 7.
Statistical tests were performed to evaluate the OHM application to the investigated region and all months showed a high degree of statistical agreement between observed and modelled values with slopes near 1, intercept values of approximately zero, and values greater than 0.99. In addition, the RMSE and MAE values were less than 1.85 Wm−2 and 1.33 Wm−2, respectively (Table 3).
From the hysteresis graph of diurnal variation in the observed and modelled values of against the values, it can be seen that the eccentricities of the ellipses from December 2013 and January 2014 were larger than those from February and March 2014 (Figure 7) and during the transitional period, and showed opposite signals (I in Figure 7), with the soil releasing more heat to the shallower layers at the beginning of the day than at the end of the day (Figures 5 and 7).
Despite its importance, measurement of soil heat flux is not performed routinely, particularly in remote areas such as the region investigated here. This study applied an indirect method (OHM) proposed by  to estimate soil heat flux using values of observed net radiation.
This study used 5-minute averages of surface soil heat flux and net radiation observed at the Brazilian Station Comandante Ferraz from December 2013 to March 2014. The observed daily total energy flux indicated that, during December and January, was a source of heat to the soil deeper layers and was a heat source to the soil. However, during February and March, and have inverse directions with releasing heat to the outer soil layers. During the daytime of the investigated months, and heated the soil. During the night-time, represents at least 29% of . Therefore, cannot be ignored in the energy balance equation of the EACF region.
The OHM was able to estimate the surface soil heat flux for each studied month, with all correlation coefficients exceeding 99%.
Future analyses will involve the application of the OHM to all months of the year and investigate the validity of the expressions obtained here for the same months of different years. It is important to note that the coefficients obtained in this study can only be used for short-time parameterizations at a specific site and for filling data gaps.
The authors declare that there are no competing interests regarding the publication of this paper.
The first author acknowledges a scholarship from CAPES. All authors would like to thank the grants of “INCT-APA” (CNPq 574018/2008-5 and FAPERJ E-16/170.023/2008). The second author also thanks CNPq (305357/2012-3 and 407137/2013-0).
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