3.1. The UHI Intensity in Moscow
There are at least two approaches to estimating the UHI intensity. The average air temperature in rural zone may be compared either with the temperature in the city centre (the station with the highest density of urban development, usually located close to the centre, although it may be located anywhere in the city), or with the average T at all urban stations. The former approach allows calculating the maximal UHI intensity over space (ΔT
MAX), whereas the latter one allows calculating the average UHI intensity over space (ΔT
AV) according to Lokoshchenko [
8]:
where
TC is the air temperature at the weather station in the centre of the city,
TU is the air temperature at other urban weather stations,
TR is the air temperature at the rural weather stations,
n is the number of stations located on the outskirts of the city, and
m is the number of stations located in the rural zone. It is better to use data from manned stations as more reliable; in our case,
n = 4 and
m = 13. The ΔT
MAX value is larger and, hence, reflects the UHI more clearly. On the other hand, ΔT
AV is more reliable as an average of all urban stations. This parameter is often used in studying the so-called “surface urban heat islands” (SUHI) using radiometric measurements of the surface temperature T
S from satellites. Usually, the SUHI intensity is calculated as the difference between the average values of the T
S in all cells inside the city and in all cells outside it in some comparison zone; for Moscow see, for example, Lokoshchenko and Enukova [
23].
Both parameters are closely connected to each other. In
Figure 1, all data about ΔT
MAX and ΔT
AV in Moscow for every 3 h during three years with a total data sampling of 8768 paired values are compared. As is seen from
Figure 1, firstly, the statistical relation is close to linear, and secondly, it is very close: the correlation coefficient R is 0.91. It should be noted that the comparison of the mean daily values of ΔT
MAX and ΔT
AV for the same period from 2018 to 2020 with a total sampling of 1096 demonstrated almost the same result: 0.90 in Lokoshchenko and Alekseeva [
7]. A small scatter of data is a result of changes in the thermal heterogeneity of Moscow area, i.e., changes in the differences between the data from the central station Balchug and the other four urban stations.
The map of isotherms calculated on average for the period 2018–2020 is presented in
Figure 2a. It was compiled on the basis of 59 stations, including 8 weather stations in Moscow (5 manned weather stations and 3 automatic weather stations), 38 stations in rural zone of Moscow region (14 manned weather stations; 3 manned special stations at airports; 1 manned station in the nature reserve and 20 automatic weather stations) and an additional 13 manned weather stations in the neighboring areas of Moscow region. The black circles represent all manned weather stations with the most reliable data due to daily manned control. In contrast, automatic weather stations are shown as white circles; their data are complementary and less reliable. The isotherms in
Figure 2a were drawn with a step of 0.5 °C by interpolation of values rounded to hundredths of °C; the same values on the map are rounded to tenths of °C.
As can be seen, the spatial field of the mean annual air temperature over Moscow region and neighboring areas is smoothed due to the thermal homogeneity of the relief (flat terrain and the absence of seacoasts). Except for Moscow city, only two isotherms (6.0 and 6.5 °C) are clearly present in rural zone in
Figure 2a. One more isotherm (7.0 °C) appears only on the southern edge of the map according to the data from only one station (Tula). It should be noted that the shape of the isotherms (e.g., the ridge of the 6.5 °C isotherm extending to the northwest) may be not a real and time-stable climatic feature. The configuration of the isotherms depends both on the averaging period and on the number of weather stations whose data are available. For example, the spatial distribution of the mean annual T for earlier averaging periods (from 1951 to 1965 in Lokoshchenko and Isaev [
24] and from 1957 to 1988 in Rubinshtein and Ginzburg [
6]) was different. It should also be noted that the mean annual T sharply increased in recent decades due to the rapid climate warming: as can be seen, at present, the air temperature in rural areas of Moscow region ranges from 6 to 7 °C, while in the middle of the 20th century it was approximately 4 °C [
24]. Geographical zonality is manifested in the general increase in T from the northeast to the southwest, but a large city (Moscow) disrupts it, creating a strong positive thermal anomaly. In the city centre T grew faster than in rural areas: from 5.6 °C on average for 1951–1965, up to 8.6 °C on average for 2018–2020. This was the result of the UHI accelerating in the recent past.
The UHI in Moscow is shown in
Figure 2a by four closed isotherms from 7.0 to 8.5 °C. At the central Balchug (B) station, T is 8.6 °C, whereas at other urban manned stations, including the Meteorological observatory of Moscow State University, it ranges from 7.2 to 7.5 °C. Nemchinovka station, located close to the city margin (N), demonstrated a value in the same range, around 7.3 °C, while at other 37 rural stations, T during three years is, on average, 6.7 °C (from 6.0 to 7.3 °C). Thus, the maximal and average UHI intensities in Moscow for this period are 1.9 and 0.9 °C, respectively. Both estimates almost coincide with the average values for the period 2010–2014: 2.0 and 1.0 °C, respectively [
8]. Therefore, Moscow UHI remains stable without any obvious changes in recent years. This could probably be the result of several reasons: the total stagnation of the Russian economy in the last decade, the deindustrialization of the city, its expansion in 2012 and, in addition, sharp drop in human activity in 2020 due to the COVID-19 pandemic. Firstly, as we know, the growth of gross domestic product in Russia has slowed down sharply since 2013. Secondly, over the past decade, many large industrial enterprises that created strong urban heat sources have been moved outside the city. In addition, in 2012, the so-called “New Moscow” was declared a new territory south of “Old Moscow”. Its gradual settlement led to a slowdown in growth, followed by a stabilization of population density in the traditional area of the city. Another additional reason was the strict quarantine measures during the COVID-19 pandemic, which led to the weakening of the UHI in Moscow in 2020 [
7]. It should also be noted that the SUHI intensity in the field of T
S in Moscow on average for the period of 2008–2015 is 2.6 °C [
23].
Let us also discuss an example of the extremely strong UHI that took place on 23 February 2018. As noted earlier by the authors [
7], Moscow on that day was located in a low-gradient baric field close to the axis of an extended ridge. As a result, clear sky and calm were observed at most urban and rural weather stations at night (only a few stations in Moscow region recorded a slight cloudiness of 3/0, which means 30% coverage of the upper Ac clouds). On average, of eight readings for that day, ΔT
MAX and ΔT
AV were 7.4 and 4.4 °C, respectively. Late at night (at 3 a.m.), ΔT
MAX and ΔT
AV were even higher: 11.5 and 6.3 °C, respectively, because T was −10.8 °C at the central urban Balchug station; −16.0 °C on average at all five manned city stations; −22.3 °C on average for 13 manned rural stations.
It should be noted that the minimal T at that time was recorded at the Cherusti station in the east of Moscow region, −27.9 °C, so the maximal difference between the two stations in the region (Balchug and Cherusti) was 17.1 °C both at 3 a.m. local time and three hours later. Moreover, in the past, a similar extremely high difference in T between two stations in Moscow region was smaller: 13.6 °C on 26 March 2001, according to Lokoshchenko and Isaev [
24]. Sometimes, these differences are taken as examples of an extremely strong UHI. However, they may be unreliable, because one rural station may reflect the influence of other factors: geographical zonality depending on the distance between stations, relief features (location of the station in a valley or basin), the passage of an atmospheric front between stations, etc. We note, in this regard, that Cherusti is the coldest weather station in the region: on average of three years, T there is the lowest among others: 5.0 °C. Thus, a correct estimation of the UHI intensity should be based on the real background T as a result of averaging over many rural stations.
The map of T at 6 a.m. on 23 February 2018 is presented in
Figure 2b. At the next reading after 3 a.m., the ΔT
MAX was slightly lower (11.2 °C), while ΔT
AV, on the contrary, became higher than it was 3 h before: 6.7 °C. As can be seen, the T field is more heterogeneous than in
Figure 2a due to one-time non-averaged data and, in addition, the specifics of the station location. Unlike
Figure 2a, the isotherms in
Figure 2b were drawn with a step of 2.0 °C. At Balchug station, T at 6 a.m. was −12.4 °C, while at other urban manned stations, it ranged from −15.9 to −21.0 °C. Thus, as seen in
Figure 2b, the nocturnal UHI in Moscow in strong anticyclone conditions was presented by four closed isotherms inside the city (from −14 to −20 °C) and two semi-closed isotherms around it (−22 and −24 °C). Some additional features of the T spatial field, such as a minimum on the east (T was −29.5 °C at the Cherusti station) and a secondary maximum in the north, are probably associated with the influence of relief and other local factors.
A similar detailed mapping of isotherms showing either the average (over time) or maximal (over time) UHI intensity is presented for San Francisco, USA and for Karlsruhe, Germany in Kratzer [
1]; for London, the UK, and other cities in Landsberg [
2]; for Leicester, the UK, and other cities in Oke et al. [
3]; for Vienna, Austria, in Böhm and Gabl [
17], etc.
3.2. Statistical Analysis of the Influence of Meteorological Parameters on the UHI in Moscow
Let us discuss the influence of various meteorological parameters on the UHI intensity.
Table 1 summarizes and evaluates both linear and non-linear relationships for both ΔT
MAX and ΔT
AV with various meteorological parameters. Eleven parameters were taken into account: total and low cloudiness; four wind parameters (mean daily wind speed, maximal value of wind speed according to eight readings during the day, maximal daily wind gust at a height of 15 m according to M-63 data and mean daily wind speed in the 40–200 m air layer according to MODOS sodar data); daily amplitudes of air and surface temperatures; the highest air pressure, the lowest relative humidity and precipitation amount during the day. Evidently, only cloudiness, wind parameters and possibly precipitation may directly affect the UHI intensity. The T and T
S amplitudes indirectly indicate anticyclonic conditions; relative humidity indirectly reflects changes in T. As we know a priori, the highest air pressure is not a real indicator of anticyclonic conditions; nevertheless, it was also analyzed. Two examples of the closest relations are presented in
Figure 3.
In addition to the classical Pearson correlation coefficient R indicating a linear relation, it was also necessary to check for possible non-linear relations. For this, the confidence index R2 of their description by the 4th degree power functions was used. The square root of this index was conventionally taken as the correlation ratio η. In fact, such a high order of the function allows us to take its confidence index as a value very close to η2 (the confidence indexes for the 4th, 5th and 6th degrees power functions are almost the same for all parameters). The closer to a linear relation, the closer R2 and η2 are to each other. For all parameters, it was determined that (η2–R2) is <0.1, except for only one comparison between ΔTAV and T daily amplitude, where the obtained value is 0.12. For all other parameters, the maximal value of (η2–R2) is only 0.06 for ΔTAV and 0.07 for ΔTMAX. Thus, except for just one relation, the non-linearity is negligibly small, so that R is a real indicator of the closeness of the relation.
As can be seen, low cloudiness represents the closest relation with the UHI intensity. The UHI intensity is more closely related to low cloudiness than to total cloudiness. This is not surprising, since the effect of thin and rarefied upper-level clouds (Ci and others) on the surface radiation balance is comparatively weak. As shown in [
7], the relationship between the UHI intensity and cloudiness is especially strong at night, when the role of low cloudiness in the radiation and heat balances of the surface is much higher than in the daytime. On the contrary, a separate comparison of ΔT
MAX and ΔT
AV with low cloudiness only for 3 p.m. leads to insignificant (<0.1) values of R, which is also not surprising, since the contribution of counter radiation to the daytime radiation balance is small.
Only slightly smaller values of R and η values were obtained for the relations with the daily amplitude of the surface temperature T
S, the daily amplitude of the air temperature T, total cloudiness and the lowest relative humidity during the day. The relations of the UHI intensity with various wind speed parameters are weaker, especially for wind speeds at high altitudes, while the relationships of the UHI intensity with the highest air pressure and precipitation are weak. A similar result on the weakening of the relationship between the UHI intensity and V with increasing altitude when comparing data at a height of 90 and 252 m was obtained in Vienna, Austria, in Böhm and Gabl [
17]. Thus, the wind speed affects the UHI intensity in Moscow less than cloudiness, in contrast to the conditions of Ibadan, Nigeria according to Anibaba et al. [
16].
To test the significance of statistical relationships, the well-known Student’s t-criterion is often used:
where
R is Pearson correlation coefficient;
σR is the
R error;
n is the sample size. As we know, the relation may be considered significant if t > 3. As can be seen from
Table 2, according to Student’s criterion, even the weakest relations are significant with an extremely high probability (much higher than 0.999). It should be noted that the
t criterion is parametric and can be used if the distribution follows the Normal law. As shown by the authors in [
7], the distributions of the UHI intensity are close to the Normal law in summer, while in winter they have a significant positive asymmetry. However, for large (
n > 100) samples and
R values far from 0 and 1, its application is possible even without a special estimation of the type of distribution according to Isaev [
25]. Thus, given the large sample size even for sodar data about wind, we use the t-criterion correctly. However, for greater confidence in the conclusions, we also consider another non-parametric Fisher’s z-criterion:
As can be seen from
Table 2, all absolute values of
tz are only a bit lower than absolute values of t. All correlation coefficients according to the z-criterion (4) are also reliable with an extremely high probability at a significance level
α→0 close to zero. Thus, any of the considered meteorological parameters significantly affect the UHI intensity.
In addition to the usual Pearson correlation coefficients, a multiple correlation coefficient
RX·YZ was also calculated between the maximal UHI intensity (X) and the two parameters which affect it more strongly than all other ones: low cloudiness (Y) and the mean daily wind speed at 15 m (Z). As we know, this coefficient indicates the simultaneous dependence of X on both parameters Y and Z, i.e., the closeness of a linear correlation between the maximal UHI intensity and the combined effect of both low cloudiness and mean daily wind speed. On average, over three years, it was determined to be 0.76. It should be noted that a separate calculation of the same
RX·YZ only for the data of 2018 leads to its even higher value: 0.82. It is notable that similar multiple correlation coefficient between the UHI intensity, wind speed and cloudiness in Vienna was much lower: only from 0.40 to 0.47 according to Böhm and Gabl [
17]. It may be that they used the data on total cloudiness and, therefore, the relation was weaker.
As is known, the significance of the multiple correlation coefficient is estimated by the Fisher distribution
F with 2 and (n − 3) degrees of freedom and under the null hypothesis that this coefficient is equal to zero in accordance with
In our case, the values of the formula are 729 for a three-year period and 372 for 2018, while the critical values of the Fisher statistics, even for a significance level of α = 1%, are 4.63 and 4.67, respectively. Thus, the significance of the RX·YZ values is evident for α→0.
3.3. Empirical Functions of Meteorological Parameters
Let us discuss the UHI intensity functions of the main meteorological parameters (air temperature T, wind speed V, total and low cloudiness). Such empirical statistical dependencies, calculated on large data samples, allow a better understanding of the influence of various parameters on the generation and dynamics of the UHI. As above, we used the same UHI intensity data and measurement results at the MSU Meteorological observatory for three years (from 2018 to 2020). All values of the UHI intensity, T, V and cloud amounts were averaged for each day. Thus, we do not consider any changes in the daily course, since they can create some noise in the results due to the inertia of the UHI response to short-term changes in meteorological parameters. Evidently, the use of daily averaged values provides more reliable functions, but, on the other hand, leads to shorter ranges of all parameters. Here, we used the maximal UHI intensity, i.e., ΔTMAX values (the difference between the Balchug station and the average of 13 out of 14 rural stations in Moscow region, except for Nemchinovka).
As seen in
Figure 4a, the function of the UHI intensity of T based on 1096 daily averaged values is non-monotonous is the demonstration of a minimum of the UHI intensity in the middle of the T range: from −4 to 0 °C. Relatively low values are observed in a wider range of T: from −9 to +10 °C. Both at higher and lower T values, the UHI intensity grows so much that there are two of its maxima at the edges of the function: at −15…−17 °C and at 21–26 °C.
Evidently, extremely low and extremely high T values when the UHI is the strongest are associated with anticyclonic conditions in winter and in summer. Neighboring ranges (−9…0 °C and 11–15 °C) on average indicate a much weaker UHI and represent either cyclonic or mixed conditions in winter and summer, respectively. Intermediate values of T from −4 to +10 °C in the middle of the total range are usually observed in the transitional seasons (spring and autumn), when the thermal difference between cyclonic and anticyclonic conditions is not so clear.
As can be seen, severe frosts increase the heat island faster than extreme heat. A stronger UHI in the conditions of extremely low T in winter than in hot weather in summer may seem unexpected, since, as we know, the UHI intensity annual course on average has a maximum in summer according to Lokoshchenko and Alekseeva [
7]. However, this is not surprising, because a cold wave in European Russia in recent decades has been a much rarer phenomenon than a heat wave. Data sampling for the lowest T values is insufficient: there were 33 days with mean daily T from −14 to −10 °C, but only 3 days with T from −17 to −15 °C.
On the contrary, the sample of data on warm and hot weather in Moscow for 3 years is much larger: 214 days at 16–20 °C and 97 days at 21–26 °C. Indeed, as in Lokoshchenko and Alekseeva [
7], during a short period of severe frosts under anticyclone conditions in February 2018, the UHI intensity was above average in summer. It should also be noted that differences in the UHI intensity between near-zero and extremely low T, as well as between near-zero and extremely high T, are statistically significant at a 5% significance level.
A similar analysis was carried out for the UHI intensity function of the wind speed V (
Figure 4b). This function was calculated twice, both according to the data of the M-63 vane at a height of 15 m above the ground, and according to the MODOS sodar data on V in the air layer from 40 to 200 m. Station data on V were used for all three years (1096 daily averaged values), while sodar data were only used for two years (2018 and 2019) and their sample contains 729 daily values, since one day (22 September 2018) was lost to acoustic remote sensing: the sodar was not working.
All station data on wind speed according to M-63 measurements were averaged over eight values every 3 h during the day. The V range of these daily averaged data is short, since the wind speed in the surface air layer is limited. The highest value was 4.6 m/s and was observed three times when Moscow was located on the periphery of deep cyclones under conditions of a high horizontal baric gradient: 19 December 2019; 13 March; and 22 April 2020. The lowest V close to calm was 0.2 m/s and was observed twice for two days in a row: on 8 and 9 September 2018, under conditions of a low-gradient baric field on the periphery of an extensive anticyclone.
Therefore, all values according to M-63 data were divided into five gradations. Sample data comprised 12 days for 0–1 m/s; 297 days for 1–2 m/s; 595 days for 2–3 m/s; 172 days for 3–4 m/s and 20 days for the highest values of 4–5 m/s. As is seen, the UHI intensity function of V according to the M-63 data is simple and monotonously decreasing. It is notable that this function is strong: starting from the second gradation of 1–2 m/s, the average UHI intensity in each next gradation is significantly lower than that in the previous one with the 0.95 confidence probability. It should also be noted that this function is non-linear and tends to slow down as V increases. Thus, it is qualitatively close to a hyperbola (inverse proportionality function) y = k/x for x > 0.
Another calculation was conducted using daily averaged sodar wind speed data in the air layer 40–200 m above the ground. As can be seen, in general, this function also demonstrates a gradual decrease in the UHI intensity with wind increase, but weaker than the previous function based on the M-63 data. This is not surprising, since the higher the air layer above the ground, the weaker the effect of the high-altitude wind on T near the ground. Differences between average values of the UHI intensity are statistically significant only when comparing conditions of light (V ≤ 6 m/s) and very strong winds (V ≥ 9 m/s). Unlike the function of the M-63 data, the differences between adjacent gradations of sodar data are, as a rule, insignificant. In the range of intersection of both functions from 2 to 4 m/s, the UHI intensity is much higher according to the sodar data than according to the M-63 data due to the total increase in the wind with a height. The sampling size of the MODOS data is quite sufficient for statistical analysis (≥24 cases) at all gradations, except for the three highest gradations (from 11 to 13 m/s). Nevertheless, we can assume that the stabilization of the UHI intensity under strong winds for V >10 m/s at these gradations is a real effect, as is the deceleration of the fall of the previous function according to the M-63 data for V values from 3 to 4 m/s (this range is insufficient for the asymptotic low limit detection). A similar function with a deceleration of the UHI intensity fall for V > 4.5 m/s was obtained in Shanghai by Qunfang Huang et al. [
14], for V > 3.5 m/s, in the cities of the Pearl River Delta by Baomin Wang et al. [
15].
Indeed, if the range of wind speed is not too short, then at a certain threshold value of V its influence on the UHI reduces to nothing. This critical value of V according to station (close to the ground) data preventing the development of the UHI was obtained as 7 m/s in Ibadan, Nigeria by Anibaba et al. [
16]; 6 m/s in Salamanca, Spain by Alonso et al. [
18]; 5 m/s in both Szeged, Hungary by Unger [
12], and Melbourne, Australia by Morris et al. [
13]. Evidently, taking into account the general increase in wind with a height in the atmospheric boundary layer, the 10 m/s threshold of wind influence in the 40–200 m air layer corresponds to a lower threshold at the station level (usually 10–15 m), which seems to be close to these estimations.
Empirical functions of the UHI intensity on cloudiness (both total and low) are presented in
Figure 4c. As can be seen, in general, both functions decrease with increasing cloudiness, so the most favorable condition for the UHI is a clear sky. Differences between the UHI intensity for ≥90% and <90% of total cloudiness and for ≥70% and <70% of low cloudiness are statistically significant with a 0.95 confidence probability. Another conclusion is that the difference between the effect of total and low cloudiness on the UHI is stronger the higher the cloudiness: it is insignificant at cloud cover <50% and significant at >50%. Similar UHI intensity functions of cloudiness were obtained in Unger [
12] for Szeged, in Qunfang Huang et al. [
14] for Shanghai, in Morris et al. [
13] for Melbourne.