Introduction

Snow albedo is an important parameter in controlling the radiation budget in the cryosphere. The mechanism of ice– albedo feedback is strongly related to the snow albedo process. In the case of optically deep snow, the visible and near-infrared albedos mainly depend on the respective snow impurities (water-insoluble solid particles) and snow grain size as factors of snow itself (Reference Warren and WiscombeWarren and Wiscombe, 1980; Reference Wiscombe and WarrenWiscombe and Warren, 1980). The highest albedo is expected for new snow without impurities. However, once the snow is contaminated with absorptive impurities for light, the visible albedo decreases preferentially. Solar energy absorbed by snow in the visible wavelengths increases the snow temperature and thus increases the snow grain size through crystal metamorphism. The increase in snow grain size reduces the near-infrared albedo and also reduces the visible albedo of snow contaminated with impurities, because the degree of visible albedo reduction due to snow impurities depends on snow grain size also (Reference Warren and WiscombeWarren and Wiscombe, 1980). The overall process of this albedo reduction is in essence a snow ageing effect. The theoretical understanding of such a snow albedo process has been advanced with radiative transfer models (Reference WarrenWarren, 1982; Reference Aoki, Aoki, Fukabori and UchiyamaAoki and others, 1999). From those investigations, a snowfall is only one process to increase snow albedo, along with the effects of solar zenith angle and cloud cover (Reference Aoki, Aoki, Fukabori and UchiyamaAoki and others, 1999).

The source of snow impurities affecting snow albedo is the atmospheric absorptive aerosols (Reference Warren and WiscombeWarren and Wis-combe, 1980; Reference Aoki, Aoki, Fukabori, Hachikubo, Tachibana and NishioAoki and others, 2000). Reference Hansen and NazarenkoHansen and Nazarenko (2004) recently demonstrated that long-range transport of strongly absorptive aerosols such as black carbon could be a cause of snow albedo reduction. Possible snow albedo reduction by black carbon contamination was revealed by radiation measurements on the snow surface at Barrow, Alaska, USA, (Reference AokiAoki and others, 1998) and in Japanese urban areas (Reference Motoyoshi, Aoki, Hori, Abe and MochizukiMotoyoshi and others, 2005). Reference Koch and HansenKoch and Hansen (2005) showed that the predominant sources of Arctic soot today are in south Asia (industrial and biofuel emissions and biomass burning). Natural insoluble aerosols such as mineral dust are also principal snow impurities during the melt season due to the effect of Asian dust. The process of aerosol deposition on the snow surface could accelerate snowmelting and thus global warming.

Reference Roesch, Schaaf and GaoRoesch and others (2004) compared surface albedos at spatial and spectral resolution retrieved from moderate-resolution imaging spectroradiometer (MODIS) data with those simulated with the general circulation model (GCM) and found that neglecting albedo variations leads to significant errors in the simulated regional climate and horizontal fluxes, mainly in mountainous and/or snow-covered regions. Reference Nolin, Frei, Beniston and VerstraeteNolin and Frei (2001) calculated the energy budget on the snow surface using snow albedo parameterization as a function of snow grain size and reported that the variable albedo was significantly more realistic and representative than the constant albedo value. To accurately simulate future climate conditions on the Earth, a physically based snow albedo model that calculates the effects of the snow physical parameters on the albedo employed in the land-surface models (LSMs) or GCMs is necessary. There are very few physically based snow albedo models. Reference Marshall and OglesbyMarshall and Oglesby (1994) developed the snow albedo parameterization in the GCM, taking into account the effects of snow grain size and snow impurities, and Reference Flanner and ZenderFlanner and Zender (2006) developed a theoretical model to predict the effects of snow ageing (snow grain size) and albedo evolution for dry snow. However, snow sub-models that estimate albedo empirically are mainly used in LSMs or GCMs at present. To develop a physically based snow albedo model, the effects of snow physical parameters on snow albedo should be investigated from field measurements taken under different snow conditions.

The effects of snow impurities and snow grain size on broadband albedos were identified from long-term radiation budget measurements on the snow surface and snow-pit work at Kitami, in a dry snow area of Japan (Reference Aoki, Hachikubo and HoriAoki and others, 2003), and at Shinjo, in a wet snow area of Japan (Reference Motoyoshi, Aoki, Hori, Abe and MochizukiMotoyoshi and others, 2005). Since 2003, we have carried out similar observations with more detailed snow-pit work for a vertical profile of snow grain size and aerosol monitoring in Sapporo, Japan. The snow conditions (depth and wetness) in Sapporo are midway between those of Kitami and Shinjo. Using these data during the winter in 2003/04, Reference Aoki, Motoyoshi, Kodama, Yasunari, Sugiura and KobayashiAoki and others (2006) showed the effects of atmospheric aerosol deposition to the snow surface on albedo reduction, especially for the heavy Asian dust event in March 2004. For the present study, we analyzed data from Sapporo taken during two winters in 2003–05 and investigated variations of snow physical parameters and their effects on albedo.

Observation Conditions, Instruments and Analyses

The observation site was the meteorological observation field (43˚04⁰56’’N, 141˚20^˚30’’ E; 15ma.s.l.) of the Institute of Low Temperature Science, Hokkaido University, located in an urban area of Sapporo. The ground condition at this site was flat grassland. Field measurements of the radiation budget and basic meteorological components made with an automatic weather station have been performed since September 2003 and continue at present (June 2006). For this study we analyzed data taken during the two winters (November–April) in 2003–05.

In the radiation budget observation, upward and downward radiant flux densities were measured with pyranometers (CM-21, Kipp & Zonen) in the shortwave region (λ = 0.305–2.8 μm), with an RG715 cut-off filter dome in the near-infrared region (λ = 0.715–2.8 μm) and with a pyrgeometer (CG-4, Kipp & Zonen) in the longwave region (λ = 4.5–42 μm). Flux densities in the visible region (λ = 0.305–0.715 μm) were calculated as the difference between the flux densities for the former two regions of the solar spectrum. The reason we measured the radiation for two spectral regions in the shortwave spectrum is that the major LSMs and GCMs divide the shortwave spectrum into visible and near-infrared regions in their radiation schemes. Each radiation component was sampled every 10 s, and 1 min averaged values were stored in a data logger. The air temperature (T _a) was measured with a platinum resistance thermometer, and snow depth (d _s) with a supersonic snow gauge, every minute. For analyses of albedos and meteorological components, 30 min averaged values from 1131 to 1200 h LT (local time), including the local solar noon, were used to keep the observational conditions uniform, except for solar zenith angle (θ0). The snow surface temperature (T _s) was calculated from the measured upward longwave radiation using equation (1) in Reference Aoki, Hachikubo and HoriAoki and others (2003) with a snow emissivity of 0.97. Some data for T _a, T _s and d _s are missing due to a malfunction of a data logger. The missing periods are November 2003 to 13 March 2004 and 15–19 April 2005 for T _a, all of the first winter and 15–19 April 2005 for T _s, and all of the first winter and 18 March–13 April 2005 for d _s. Instead of the missing T _a, air-temperature data measured by the Sapporo District Meteorological Observatory (SDMO; 43˚03^˚30’’N, 141˚19^'42’’ E; 17ma.s.l.), located 3 km south-southwest of our site, were used. There were no alternative data for the missing T _s. The values of d _s were determined from snow-pit work (twice a week), and the values for the days without snow-pit work were interpolated using the data from SDMO.

Snow-pit work was performed approximately twice a week to determine the snow types, temperature and density for all snow layers, as well as the snow grain size for each snow layer from the surface to a depth, d, of 10 cm. Snow samplings were taken for two snow layers (d = 0–2cm and 0–10 cm) to measure the mass concentration of snow impurities. The time of day for the snow-pit work was almost always around 1100 h LT. The collected snow samples were filtered using Nuclepore filters, and the mass concentration of snow impurities was estimated by weighing the Nuclepore filters with a balance.

Results and Discussion

Variations of snow physical parameters

Figure 1 presents the observed results for snow types obtained from the snow-pit work. The maximum snow depth was just above 1m in both winters. The yearly peaks of the daily maximum snow depth and yearly maximum snow depth averaged over the past 30 years (1971–2000), as measured by SDMO, were 75 cm (around 20 February) and 101 cm respectively. Comparing our results with these records, the snow accumulation conditions at our observation site during the two winters did not deviate much from average conditions. In Figure 1, the measured snow depth increases until the end of February or the beginning of March, and decreases in March and April. We refer to the former period as the ‘accumulation season’ and the latter period as the ‘melt season’. Observed snow types in the upper layers in the accumulation season consisted of new snow, lightly compacted snow and compacted snow, while the lower layers consisted of granular snow. The formation of a lower granular snow layer is due to upward soil heat flux from the underlying ground. The measured ground temperatures were almost 0˚C except at the beginning of the snow season. Granular snow was also sometimes observed at the top layer even in the accumulation season. Internal snow types observed in Sapporo in the accumulation season were quite different from those observed at Kitami (43˚49^˚21’’N, 143˚54^'13’’ E; 85ma.s.l.) by Reference Aoki, Hachikubo and HoriAoki and others (2003), where faceted crystals (solid-type depth hoar) and depth hoar were observed in the middle and lower layers of the snowpack. Although Sapporo and Kitami are located at similar latitudes and at low altitudes, with a distance of 220 km between the two sites in Hokkaido, the internal snow types show a significant contrast in both snowpacks. At Kitami, the locational characteristics of cold temperatures and less snow cover produce a snow temparature gradient conducive to the formation of depth hoar (Reference Hirashima, Nishimura, Baba, Hachikubo and LehningHirashima and others, 2004), while snow temperature gradient in Sapporo was small due to high air temperature and deep snow.

Fig. 1.

Snow-pit work results showing the vertical profiles of snow types during the winters of 2003/04 (a) and 2004/05 (b) in Sapporo.

The melt season in the 2003/04 winter began 2 weeks earlier than in the 2004/05 winter. Significant submerged snow layers were observed at the bottom layers in the snowpack during the melt season in the first year (Fig. 1a). The snow disappearance date in the first winter was 2 weeks earlier than in the second winter. The difference in the onset of the melt season between the two years was caused by an air-temperature difference in February (Fig. 2). Following that, temperatures in the 2003/04 winter were higher than in the 2004/05 winter, and thus rapid melting along with submerged snow layers occurred. T _s was measured only during the 2004/05 winter (Fig. 2b). When T _s increased up to 0˚C, granular snow was observed.

Fig. 2.

Air temperature, T _a (solid line with dots), and snow surface temperature, T _s (solid line with crosses), averaged for 1131–1200 h LT, and solar zenith angle, θ ₀ (dashed curve), at 1145 h LT during the winters of 2003/04 (a) and 2004/05 (b). Due to a data-logger malfunction, some data are missing: for November 2003 to 13 March 2004 and 15–19 April 2005 for T _a, and during the first winter and 15–19 April 2005 for T _s. Air temperatures at 1200 h LT measured by SDMO are plotted instead of the missing T _a, while there were no alternative data for T _s.

Figure 3 presents the snow grain size and mass concentration of snow impurities for two different snow layers, measured from snow-pit work and snow sampling. The measured snow grain size is defined in the same way as r ₂ in Reference Aoki, Hachikubo and HoriAoki and others (2003), namely one-half the branch width of dendrites or one-half the dimension of the narrower portion of broken crystals. This dimension corresponds with the optically equivalent snow grain radius (Reference AokiAoki and others, 1998, Reference Aoki, Aoki, Fukabori, Hachikubo, Tachibana and Nishio2000). Measured values of snow grain size at the snow surface were generally smaller than those for d = 0–10 cm. This is because the snow grain size at lower positions (older snow) has increased compared with surface snow due to crystal metamorphism, such as a sintering or a melting for a longer time. These values were on the order of 1.0mm for granular snow and were one order of magnitude smaller for new snow and (lightly) compacted snow. The latter size is the same order as the mean convex radius (0.1– 0.2 mm) measured at many different sites in Antarctica (Reference Gay, Fily, Genthon, Frezzotti, Oerter and WintherGay and others, 2002) and is larger than the effective radius (area-weighted mean radius) (0.024 mm) measured at the South Pole (Reference Walden, Warren and TuttleWalden and others, 2003).

Fig. 3.

Snow grain size measured from snow-pit work and mass concentrations of snow impurities measured from snow samples during the winters of 2003/04 (a) and 2004/05 (b). Each snow physical parameter was measured for the various snow layers, which are denoted by snow depth d from snow surface. The definition of snow grain size is the same as for r ₂ in Reference Aoki, Aoki, Fukabori, Hachikubo, Tachibana and NishioAoki and others (2003).

Values of snow impurities for the top layer (d = 0–2 cm) were generally higher than those for d = 0–10 cm because the snow impurities are supplied by the depositions of atmospheric aerosols, as suggested by Reference Aoki, Aoki, Fukabori, Hachikubo, Tachibana and NishioAoki and others (2000). For new snow and (lightly) compacted snow during the accumulation season, concentrations in the d = 0–2 cm and d = 0–10 cm layers were 2–8 and 0.7–8 ppmw, respectively. They increased remarkably during the melt season, especially for granular snow, and sometimes exceeded 100 ppmw. The abrupt rise in March 2004 was due to the heavy Asian dust event on 11–12 March (Reference Aoki, Motoyoshi, Kodama, Yasunari, Sugiura and KobayashiAoki and others, 2006).

Figure 4 presents broadband albedos averaged for 1131–1200 hLT (close to the local solar noon) for the visible, near-infrared and shortwave regions, along with the snow depth. Each albedo remained stable during the accumulation season compared with the melt season. The difference in albedo between accumulation and melt seasons corresponds to the difference in snow types between those seasons. During the accumulation season, the short-term variation of the near-infrared albedo exceeded that of the visible albedo. Reference Aoki, Motoyoshi, Kodama, Yasunari, Sugiura and KobayashiAoki and others (2006) explained, based on the data from the 2003/04 winter, that these variations are due mainly to the effects of snow physical parameters and the cloud cover. The primary snow physical parameters affecting the albedo are snow impurities (mainly for the visible region) and snow grain size (for the near-infrared region) (Reference Warren and WiscombeWarren and Wiscombe, 1980; Reference Wiscombe and WarrenWiscombe and Warren, 1980). According to the theoretical simulation for cloud effects on snow albedo conducted by Reference Aoki, Aoki, Fukabori and UchiyamaAoki and others (1999), the shortwave albedo was increased by 0.04 (θ0 = 66˚ at winter solstice)–0.07 (θ0 = 34˚ at snow-cover disappearance) by cloud cover for a snow grain radius of 0.05 mm. This simulation includes both the effects of cloud cover, which changes the spectral distribution of incoming radiation and the sky-averaged incidence angle to a value larger than θ0, while snow albedo may still increase depending on cloud condition and snow grain size. Therefore, the short-term albedo variations would contain the effects of not only snow physical parameters, but also cloud cover.

Fig. 4.

Visible (crosses), shortwave (filled circles) and near-infrared (open circles) albedos averaged from 1131 to 1200 h LT, and snow depth, d _s (solid curve), during the winters of 2003/04 (a) and 2004/05 (b). Due to a data-logger malfunction, some data for d _s are missing for the entire period of the first winter and 18 March–13 April 2005. The plotted δ _s values for the missing periods were determined from snow-pit work, and the values for the days without snow-pit work were interpolated using data from SDMO.

During the melt season, the albedo decreased with snow depth. This tendency is remarkable for the near-infrared albedo. The visible albedo sometimes recovered to high values around 0.9 due to new snowfalls, but could not maintain this for a long period. During the melt season, both the snow grain size and the mass concentration of snow impurities increased significantly (Fig. 3) except for days when the surface was covered by new snow. Changes in these snow physical parameters reduce the albedo. The other factors affecting snow albedo are θ0, the snow depth and liquid water in the snow. During this period, the value of θ0 varies from 50.6˚ (1 March) to 34.5˚ (12 April) at the local solar noon (Fig. 2). The simulated shortwave albedo reduction due to a change of θ0 is <0.02 for a snow grain radius of 1 mm under a clear sky (Reference Aoki, Aoki, Fukabori and UchiyamaAoki and others, 1999), so this effect is not essential. Reference Aoki, Motoyoshi, Kodama, Yasunari, Sugiura and KobayashiAoki and others (2006) explained, based on the data from the 2003/04 winter, that the effects of snow depth should appear during the last several days before the snow disappearance date, and that liquid water would enhance the effect of snow grain size on albedo reduction because increasing the liquid water could increase the optically equivalent snow grain size. These explanations are also plausible for the results from the 2004/05 winter. In the next subsection, we quantitatively examine the effects of snow grain size and impurities on the albedo based on comparisons with theoretically calculated albedos.

Effects of the snow physical parameters on broadband albedos

The relationships between broadband albedos and snow impurities for two different sampling layers are illustrated in Figure 5. The measured visible albedos, denoted by characters, clearly depend on the mass concentration of snow impurities for the cases of d = 0–2 cm and d = 0–10 cm (Fig. 5a). Curves illustrate the theoretically calculated maximum and minimum broadband albedos during the observation period for each of three different types of snow impurity models, using a radiative transfer model for the atmosphere–snow system (Reference Aoki, Aoki, Fukabori and UchiyamaAoki and others, 1999). In this model, each snow layer is assumed to be semi-infinite and homogeneous (the snow grain size and mass concentration of snow impurities have constant profiles in a snowpack). The maximum and minimum curves are determined from simulated albedos for all possible ranges of geometric conditions, sky conditions and the measured snow physical parameters during the observation period. A detailed method to determine the maximum and minimum albedo is described in section 4.3 and the appendix of Reference Aoki, Hachikubo and HoriAoki and others (2003). In the present study, the maximum albedo is expected for the smallest snow grain radius (0.02 mm), at the largest θ0 (66.6˚ on the winter solstice), under a clear sky (for the visible albedo) or cloudy sky (for the near-infrared albedo). The minimum albedo is expected for the largest snow grain radius (1.5 mm), at the smallest θ0 (34.5˚ on 12 April), under a clear sky. The smallest and largest values of snow grain size are the in situ measured minimum and maximum values during the two winters.

Fig. 5.

Visible albedo (a) and near-infrared albedo (b) as a function of the mass concentration of snow impurities during the period 2003–05. Characters denote the measured albedos vs mass concentration of snow impurities measured for the snow surface (filled circles) and the snow layer from surface to 10 cm (open circles). Thin and thick curves indicate the theoretically predicted maximum and minimum albedos during the observation period using three types of snow impurity models: MD only, MD+ST0.25 and MD+ST0.50. The snow grain size (r _e), sky conditions (clear/cloudy) and solar zenith angle (θ ₀) corresponding to the maximum and minimum albedos were determined within the measured ranges of these parameters during the observation period.

Since the optical properties of snow impurities are uncertain factors, we adapted the typical aerosol models in the same manner as Reference Motoyoshi, Aoki, Hori, Abe and MochizukiMotoyoshi and others (2005), in which three types of aerosol (snow impurity) mixings from mineral dust (MD) and soot (ST) were assumed: (1) MD-only model (MD only), (2) MD with ST of 0.25 ppmw model (MD+ST0.25), and (3) MD with ST of 0.5ppmw model (MD+ST0.50). For example, when mass concentration of snow impurities is 1ppmw, the MD+ST0.25 model consists of soot of 0.25ppmw and dust of 0.75ppmw. In these impurity models, light absorption is weakest for MD-only and strongest for MD+ST0.50. The optical properties for MD and ST were employed from the ‘transport mode’ of the mineral dust model and the soot model both compiled in the Optical Properties of Aerosols and Clouds (OPAC) database by Reference Hess, Koepke and SchultHess and others (1998).

In Figure 5, the range between the maximum and minimum albedo curves for each aerosol mixing type represents the possible variation of albedos. Although the range of the theoretically predicted visible albedo for the MD-only case takes values up to 0.99 for low concentrations of snow impurities (Fig. 5a), the measured visible albedos went up to 0.93, which was recorded for new snow during the accumulation season. Major data points are distributed within the ranges for MD+ST0.25 or MD+ST0.50. Even the highest albedos are lower than the maximum albedo curve of MD+ST0.50. These results suggest that the snow in Sapporo was contaminated not only with mineral dust but also with more absorptive soot.

On the other hand, the amount of information on snow impurities contained in the near-infrared albedo is not as great. As a result, the theoretically calculated near-infrared albedos do not differ remarkably among the three types of snow impurity models (Fig. 5b). Although the measured values of near-infrared albedos fall completely within the ranges of the theoretically predicted albedos, the measured values are distributed from the upper left to the lower right in the theoretically predicted ranges. This is because, in general, the measured snow impurity and snow grain size correlate to each other (Reference Aoki, Hachikubo and HoriAoki and others, 2003).

The relationships between broadband albedos and snow grain size for two different snow layers are illustrated in Figure 6. In the theoretical calculations, the maximum albedo is expected for low snow impurities (1 ppmw), at the largest θ0 (66.6˚), under a clear sky (for the visible albedo) or a cloudy sky (for the near-infrared albedo). The minimum albedo is expected for high snow impurities (200 ppmw), at the smallest θ0 (34.5˚), under a clear sky. The low and high values for the mass concentration of snow impurities are not the minimum and maximum values, but the lower and upper values of the distribution group of impurity concentrations measured from snow samples for d = 0–10 cm. The measured snow grain sizes plotted in Figure 6a and c are for the shallower snow layer (d = surface); Figure 6b and d are for the deeper layer (d = 0–10 cm). The data points for d = 0–10 cm (Fig. 6b and d) shift in the direction of large grain size compared with those for d = surface (Fig. 6a and c) because the measured snow grain sizes in the lower layer were larger than those for the surface as seen in Figure 3. For visible albedo (Fig. 6a and b), data points (measurements) outside the range of the theoretical curves for d = 0–10 cm are fewer than those for d = surface, while the situation is reversed for the case of near-infrared albedo (Fig. 6c and d). This is because light absorption by ice (snow grains) is weaker in the visible wavelengths than in the near-infrared wavelengths. The visible albedo contains information on snow grain size in deeper snow layers, while the near-infrared albedo contains only information on the shallower layers. This phenomenon is confirmed by remote sensing of snow grain size (Reference Tanikawa, Aoki and NishioTanikawa and others, 2002) and by theoretical study for vertical inhomogeneity of snow on spectral albedo (Reference Zhou, Li and StamnesZhou and others, 2003). In Figure 6c and d, some measured albedos where the measured snow grain size is 0.2–0.3mm are distributed at higher values than the theoretical predictions (cloudy case). Before snow disappears, the snow depth can be very thin and spectral albedo of the grassland beneath the snow cover could play some role in snow surface albedo.

Fig. 6.

Visible albedo (a, b) and near-infrared albedo (c, d) as a function of snow grain size during the period 2003–05. Characters denote measured albedos vs in situ measured snow grain sizes at the snow surface (a, c) and averaged over the snow layer from surface to 10 cm (b, d). Thin and thick curves indicate the theoretically predicted maximum and minimum albedos during the observation period using three types of snow impurity models: MD only, MD+ST0.25 and MD+ST0.50. The mass concentration of snow impurities, c, sky conditions (clear/cloudy) and solar zenith angle, θ ₀, corresponding to the maximum and minimum albedos are determined within the measured ranges of these parameters during the observation period.

However, the minimum snow depths before snow disappearance at which the measured albedos are plotted in Figure 6 were 39 cm in 2004 and 24cm in 2005. Thus, less effect of underlying surface would be expected. One possible reason is the assumption of an inappropriate cloud model (regarding cloud type and thickness) in the theoretical calculations.

Conclusions

Variations of the snow physical parameters and their effect on albedo were investigated from the data of radiation budget, meteorological components and frequent snow-pit work measured in Sapporo during two winters in 2003–05. Snow types observed in the accumulation season showed a significant contrast with those previously observed at Kitami, although the sites are located at a similar latitude and at a low altitude. Since the internal snow types would be affected by local climate conditions, the monitoring of snow types is important.

Measured snow grain sizes were on the order of 1.0 mm for granular snow and were one order of magnitude smaller for new snow and (lightly) compacted snow. The latter sizes are on the same order as, or larger than, those measured in Antarctica. Measured mass concentrations of snow impurities for snow layers of d = 0–2cm and d = 0–10cm were 2–8 and 0.7–8ppmw, respectively, during the accumulation season, and sometimes exceeded 100 ppmw during the melt season. Increases in both snow grain size and mass concentration of snow impurities contributed to a reduction in snow albedo.

The measured relationships between broadband albedos and the mass concentration of snow impurities agreed with the theoretically predicted relationship for the snow model assuming contamination not only with mineral dust but also with more absorptive soot. A similar comparison for the relationships between broadband albedos and snow grain size revealed that the visible albedo contains information on the snow grain size in deeper snow layers (d = 10 cm), and that the near-infrared albedo contains information on only the top snow layer. This is because light absorption by ice (snow grains) is weaker in the visible wavelengths than in the near-infrared wavelengths.