1. Introduction
From the very beginning of the problem of light pollution, especially in the form of an artificial night sky glow, it was obvious that the main sources of this problem were cities, particularly street lighting [
1,
2]. The concept of a light glow was first introduced probably in 1935 [
3], and the concept of astronomical light pollution in 1973 [
4]. In the following years, the described phenomenon increasingly threatened astronomical studies [
5], including those carried out in Cracow (Poland) [
6]. Along with the development of urban infrastructures, in addition to street lighting, other light sources appeared, increasing the brightness of the sky glow. Light pollution is mainly due to the operation of wrongly designed street lighting, advertising, illumination of sports stadiums, construction, security, and façade lighting [
7,
8,
9,
10,
11]. To this day, there is no real effective policy that deals with this problem.
As a result of studies on the impact of urban lighting on the brightness of the night sky, several theoretical models were created to describe this problem [
12,
13,
14,
15,
16,
17,
18,
19,
20,
21].
The impact of cities on light pollution was also the subject of field studies, enabled by the introduction of cheap Sky Quality Meters (SQMs), which became a kind of measurement standard [
22,
23,
24,
25]. Similar measurements were also carried out in 2009 in Cracow and the surrounding area by the team of the Light Pollution Monitoring Laboratory (LPML) operating at the Cracow University of Technology, led by the author of this paper [
26,
27]. The obtained results showed compliance with the values predicted by the first World Atlas of the Artificial Night Sky Brightness [
28].
From 1972, it became possible to quantify the light emission from cities based on satellite images taken by the Defence Meteorological Satellite Program (DMSP) satellites [
29,
30]. In 2001, using the Treanor and Garstang models and determining the amount of light emitted by cities based on DMSP images, the aforementioned atlas was created (often called the Atlas of Light Pollution), commonly used to describe light pollution on Earth’s surface [
28]. However, since the purpose of the DMSP satellites was to forecast the weather, their cameras did not have sufficient resolution to show the fine structure of light sources.
In 2011, the National Oceanic and Atmospheric Administration (NOAA) launched the Suomi NPP satellite [
31]. This satellite has a visible infrared imaging radiometer suite camera (VIIRS) providing the best freely available night-time dataset with daily and global coverage. While in the case of DMSP satellites the smallest visible objects were 3 km in size, the VIIRS images show objects smaller than 1 km [
32]. The fundamental importance of VIIRS data, in particular Day–Night Band (DNB) images for mapping Earth’s surface night illumination, especially when compared to earlier DMSP data, was highlighted in 2013 [
33]. VIIRS data were also used to create the all-sky artificial sky glow model [
34] and the new World Atlas of the Artificial Night Sky Brightness [
35].
In 2008, the Luojia 1-01 CubeSat (6U) sized earth observation satellite, built by the Wuhan University (China), was launched into orbit. This is the first dedicated night-time light satellite providing images with a spatial resolution of 130 m, which is much better than that of DMSP/OLS and Suomi-NPP/VIIRS [
36]. This creates new perspectives for remote sensing of night lights [
37].
Additionally, to analyse the impact of individual types of urban lighting, high-resolution photos of some cities taken from the International Space Station (ISS) can be used [
38,
39]. Such a photograph was also taken for Cracow on 28 March 2017 (
Figure 1). In this photo, almost all types of illuminated streets can be distinguished, as well as separate parts of the city where metal-halide or high-pressure sodium lamps (HPS) have been replaced by LED lighting.
One of the first analyses of the contribution of particular types of urban lighting to the city’s total radiance was the 2009 estimation of the complete outdoor lighting of Flagstaff (Arizona) [
40]. It was found that the average fraction escaping directly upward from light fixtures was equal to 8.3%. Of the total uplight, 33% came from sports lighting when it is on; when sports lighting is off, commercial and industrial lighting accounted for 62%, with the remainder dominated by residential (14%) and roadway lighting (12%).
The potentially most complete data on light pollution sources could be obtained by switching them off sequentially and analysing the effect of these switching offs on the night sky glow. Thus far, city lighting outages have been short lived, related to lighting failures, and have occurred in a limited area, most often in a certain part of the city. However, these events were always an opportunity to research their effect on the brightness of artificial sky glow.
One of the first studies of this type was conducted on 28 September 2006 in Reykjavik, where all streetlights were shut off from 10:20 p.m. to 10:40 p.m. to prepare for the Reykjavik International Film Festival [
41]. It was found that street lighting was a significant contributor to sky-glow light pollution.
Another example can be a power failure in part of Cracow in the late evening of 25 August 2011 [
42]. During the failure, for more than two hours, a compact area of 2 km
2 with approx. 50,000 population was deprived of any power supply (both flats and street lighting). The sky brightness was then equal to 18.07 mag/arcsec
2 (6.44 mcd/m
2). When repairing the failure, only the closest vicinity of the measurement site, with an area of about 0.03 km
2, was deprived of light for about half an hour. The measured zenith surface brightness of the sky was then equal to 17.72 mag/arcsec
2 (8.90 mcd/m
2). After the failure was completely repaired, the zenith surface brightness of the virtually cloudless sky, measured near the centre of this region, was equal to 17.51 mag/arcsec
2 (10.79 mcd/m
2). Measurements performed during the phenomenon allowed for the analysis of the impact of local lighting on the artificial sky glow of the entire city. It was found that the complete switching off of lighting in an area constituting only 4% of the city’s area causes a 40% reduction in the zenith surface brightness of the night, cloudless sky.
In 2016, differential photometric measurements of the change in night sky brightness and illuminance were performed during an automated regular switch-off of ornamental light in the town of Balaguer and an organised switch-off of all public lights in the village of Àger, both near Montsec Astronomical Park in Spain [
43]. It was found that during the clear night, the ornamental lights in Balaguer contribute over 20% of the sky glow at zenith at the observational site, while very small changes were found in the ground illuminance on a cloudy night near Àger. Similar research, but on a local scale, was conducted in an urban park (Tiergarten) in Berlin (Germany) during the WWF Earth Hour in 2018 [
44]. It was found that turning off nearby lighting (Potsdamer Platz) resulted in a 15% decrease in scalar illuminance, 11% decrease in horizontal illuminance, and 8% decrease in zenith luminance.
To find out what fraction of outdoor light emissions and associated energy use are due to streetlights or various types of private light sources, an experiment was carried out in 2019 in Tucson (Arizona). The streetlight output had been intentionally altered over 10 days, and the change in emissions observed by satellite was examined. It was found that streetlights operated by the city are responsible for only 13% of the total radiance measured from Tucson from space after midnight [
45]. If the city did not dim its streetlights after midnight, the contribution would be 18%. When streetlights operated by other actors are included, the best estimates rise to 16% and 21%, respectively.
Another analysis of this experiment showed that the zenith sky brightness during the tests decreased by 5.40% near the city centre and 3.6% at an adjacent suburban location on nights when the output of the street lighting system was dimmed from 90% of its full power draw to 30% after local midnight [
46]. The model of light sources, consisting of 26% known street lights and 74% of other sources results suggests that street lights account for about 14% of light emissions resulting in sky glow seen over the city. However, the direct measurements implied that street lighting contributed only 2–3% of light seen at the zenith over Tucson. The difference between the modelled and experimentally determined values was explained by an underestimation of the total city light emission, not accounting for the transient sources of light whose emission patterns are near horizontal, such as interior lighting escaping through uncovered building windows, automotive lighting, and illuminated signs. The improvement of sky brightness may also be related to air pollution in the studied areas [
47,
48].
The spreading of a COVID-19 pandemic in 2020 influenced the increase in the burden on health care, decreased human mobility, and the related decline in tourism and caused various kinds of unexpected effects in the natural environment as well [
49]. As a result of migration restrictions and industrial activity limitations, overall carbon emissions have dropped [
50]. An improvement in air quality and a decrease in water pollution in many cities around the globe were also noticed [
51]. The impact of the pandemic was even visible in aspects such as the reduction of seismic noise associated with anthropogenic earth surface vibrations from trains, aeroplanes, industrial processes, etc. [
52].
Of course, the pandemic lockdown also prompted many light pollution researchers to investigate the changes it caused in the brightness of a sky glow. The effects of the lockdown on urban light emissions were described for Granada (Spain), including both ground and satellite data [
47]. The research, conducted from 14 March until 31 May 2020, showed a clear decrease in light pollution due to both a decrease in light emissions from the city and a decrease in anthropogenic aerosol content in the atmosphere which resulted in less light being scattered. A clear correlation between the abundance of PM10 particles and sky brightness was observed, such that the more polluted the atmosphere, the brighter the urban night sky. The ground-based data showed little change in the second half of the night, compared to the first, and also the satellite imagery does not show marked differences during the lockdown in terms of total light output. Given that outdoor activities decreased by up to 90% during a lockdown, these results indicate that the light output of the city seems to be dominated by permanent lighting that does not adapt to the real use of the outdoor areas by the citizens.
A photometric mapping of the artificial sky glow of a large city and its surroundings was also performed on the example of Berlin, both in the case of a cloudless and completely overcast sky [
48]. It was found that the brightness of the artificial sky glow at zenith decreased by 20% at the city centre and by more than 50% at a 58 km distance from this area during the lockdown. At the same time, the overall light emission trend in the region, as observed by satellite data, was increasing. It has been suggested that the main cause for the reduction of artificial sky glow originates from improved air quality due to less air and road traffic, which is supported by statistical data and satellite image analysis. A similar analysis is currently being carried out for Cracow by the author of this paper, to be published in the future.
In April 2020 and the following months, the authorities of Cracow, as well as several neighbouring communes, resolved to completely or partially turn off street lighting at night, starting from midnight (or from 1:00 CEST) to dawn (usually to 4:00 CEST). This created a unique opportunity to study the contribution of street lighting to both the emission of light energy from the entire city (especially since VIIRS/DNB images of the research area are taken just after 1:00 CEST, i.e., after turning off street lighting in all researched communes), as well as to measure changes in the surface brightness of the night sky. A network of automatic and manual LPML measuring stations was used for these measurements. The analysis of both these data sets is the subject of this paper.
4. Discussion
The number of illuminated roads in the commune, and particularly in the city, should depend on the number of inhabitants.
Figure 15 shows the mean monthly radiance determined in March (before the street lighting shutting off period) vs. the population of the researched communes. There is a clear proportionality between these values. It means, as expected, that the main factor responsible for the amount of light energy emitted into the space is related to the number of emitters, which in turn is related to the population of the area. This relationship is consistent with the models proposed by Walker [
14] and Berry [
16].
The presented research concerns the impact of switching off street lighting on the radiance. Therefore, the relationship between the radiance and the total length of illuminated roads in a given commune was checked. In this case, a clear proportionality of these values is also visible (
Figure 16). However, it should be kept in mind that this relationship is indirect since undoubtedly the total length of roads in a given area depends on the population. Nevertheless, the presented graph means that unquestionably turning off street lighting should reduce the radiance. It can be concluded that the average radiance per kilometre of road in the research areas is 11.1 nW/cm
2·sr/km.
Switching off street lighting in the analysed communes should impact their mean annual radiance. The column chart of the average annual radiance for Cracow in recent years (
Figure 5) shows that the street lighting switching off in 2020 decreased this value, compared to the three previous years (in 2017, street lighting was modernised and extended in Cracow). To exclude the impact of other random factors that could cause such an effect, the monthly mean values of radiance for Cracow in the spring months of 2015–2020 were analysed (
Figure 6). In May 2020, the radiance of Cracow significantly decreased, compared to both the neighbouring months and the same month in the preceding years. This should, of course, be linked to the total shutdown of street lighting in the city for the entire month. In this way, it was shown that indeed switching off street lighting has a noticeable effect on the radiance. The obtained image of the differential radiance between March 2020 (when the lighting was not turned off) and May 2020 (
Figure 7) shows that the effect of reducing the radiance was mainly caused by turning off street lighting in the western part of Cracow, mainly in the area of the Old Town and its surroundings (the lighting of the ArcelorMittal Poland steel plant in the eastern part of the city was also turned off). The analysis of the daily radiance on selected days in the research period (
Table 4) shows that initially (when only part of the lighting was turned off), it decreased by approx. 19,400 nW /cm
2 · sr. At the beginning of May, on the days when the lighting of the greatest number of streets was turned off, the reduction in radiance compared to March was approx. 26,300 nW/cm
2 · sr, which means a reduction in the radiance of Cracow by half. This value is much higher than in the case of tests carried out with the street lighting switched off in Tucson (46). The reason is probably that Tucson has long had a very well-designed street light system that complies with protection against light pollution, while in Cracow, the modernisation of street lighting began only in 2017.
Analogous diagrams made for near-Cracow communes showed that the type of commune and the scale of switching off street lighting are of significant importance here. The effect of reducing the mean annual radiance in 2020, compared to previous years, is most clearly visible in the case of Alwernia (280 nW/cm
2 · sr), Chrzanów (780 nW/cm
2 · sr), Krzeszowice (580 nW/cm
2 · sr), and Wieliczka (290 nW/cm
2 · sr), i.e., communes in which a significant part of street lighting was turned off, or this turning-out lasted several months (
Appendix F:
Table A3). This effect is not visible in the case of Skawina and Zabierzów. The effect of switching off street lighting is particularly evident in diagrams showing the mean monthly radiance (
Figure 9). The period of radiance reduction in Chrzanów, Krzeszowice, Skawina, or Wieliczka is fully consistent with the period of street lighting switching off (
Appendix F:
Table A4). However, the rapid decrease in radiance in the case of Zabierzów is rather not related to switching off street lighting but to the annual temporary turning off the lighting of the aforementioned greenhouse in summer months. In the case of Dobczyce, only part of the street lighting in some rural areas was turned off, which caused only a slight change in the commune’s radiance.
Confirmations of the dates of switching off and switching on the street lighting are the daily radiances of individual communes (
Figure 11;
Appendix F:
Table A5).
The analysis of VIIRS/DNB images for the dates preceding the periods of switching off the street lighting and for the periods during which it took place allows, to some extent, to identify the main light sources (
Figure 3;
Appendix C:
Figure A1 and
Figure A2). The differential radiance images are also helpful in the identification. On their basis, it can be concluded that the radiance changes were indeed caused by switching off the lighting of the main roads in a given commune. However, turning off street lighting in towns and larger cities was of particular importance, which is especially well visible in the case of Alwernia, Chrzanów, and Wieliczka. In the case of Zabierzów, it was possible to find in the database the night during which the bright greenhouse, usually dominant in the image of this commune, was turned off—it is clear that it is indeed the main source of light in the commune. To identify the sources of radiance changes in urban–rural communes more confidently, it was determined separately for urban and rural areas (
Figure 11;
Appendix F:
Table A5,
Figure A4). In the case of poorly urbanised communes, such as Alwernia or Krzeszowice, radiance changes are caused only by turning off the street lighting in rural areas, which is evident especially for September 2020, when the lighting of rural roads was turned off for savings. In the case of urbanised communes, such as Chrzanów or Skawina, radiance changes are only caused by switching off the city lighting (in Chrzanów, the process of the gradual restoration of street lighting in August 2020 is visible). In the commune of Dobczyce, only part of the street lighting in rural areas was turned off. Wieliczka is the only commune where street lighting has been consistently turned off, both in the city and in rural areas. In the case of the rural commune of Zabierzów, the observed reduction in radiance is less due to switching off the street lighting and to a much greater extent switching off the lighting of the aforementioned greenhouse in July 2020. In the case of Cracow, which is a municipal commune, naturally, switching off the street lighting in the city is responsible for the entire radiance change. A detailed territorial distribution of radiance and the linking of its changes with specific objects in the city is the subject of a separate publication that is being prepared.
Information was obtained from the analysed communes about which roads’ lighting was turned off (
Appendix B:
Table A2). It is confirmed by the analysis of radiance images and their comparison with the road maps (
Figure 3;
Appendix C:
Figure A1 and
Figure A2). These data make it possible to plot the relationship between the differential radiance of communes (the difference of radiance between the month in which street lighting was switched on and that in which street lighting was switched off) and the length of roads in which lighting was switched off (
Figure 17).
In the case of rural and urban–rural communes, the proportionality of the differential radiance to the length of “darkened” streets is evident. In these surroundings, street lighting is the dominant factor emitting light into space. In the case of Cracow, where all public street lighting was turned off (both in more and less urbanised areas), this resulted in a relatively small decrease in radiance. Perhaps it is related to the fact that in Cracow it is not the dominant factor illuminating the night sky. Additional sources of light are numerous apartment communities with their own lighting, as well as light advertising, offices, and even some important road intersections. It is also possible that this effect is caused by a higher concentration of particulate matter, which is the source of light scattering.
In communes, where the S
a measuring points were active (Dobczyce (DOB); Cracow (KPO, KPO2, BOT); Wieliczka (WIE)), it is possible to plot a relationship between the decrease of S
a and the decrease of radiance (
Figure 18). Unfortunately, the small number of these measuring points makes it difficult to conduct a deeper analysis. However, it seems that the decrease in the surface zenith brightness of the sky (dS
a) depends mainly on the population of the commune not on the decrease in radiance. In the case of measuring points located in Cracow, dS
a is equal to 0.5–0.6 mag/arcsec
2 (37% decrease), while in the case of neighbouring small cities, it is equal to 0.2–0.3 mag/arcsec
2 (17% decrease). In the case of Cracow, this value is much higher than the zenith brightness decrease in the Tucson experiment [
46]. The reason is probably that street lighting in Cracow began to be modernised only in 2017, and this modernisation is still underway.
At several measuring points, located outside Cracow, a decrease of S
a can be related to the turning off the street lighting in this city.
Figure 19 shows the relationship between the S
a value measured at all active measuring points and the distance from the centre of Cracow, defined as the centre of the area with the greatest radiance change (i.e., the Old Town,
Figure 7). A clear relationship between these values is visible. Moreover, as can be observed, even at a distance of 20 km, the changes of street lighting in Cracow affect the zenith brightness at this measuring point. A similar decrease in zenith brightness with distance was also found for Berlin [
48], but in the case of Cracow, the range is much smaller. This should be associated with the much smaller population of Cracow (almost 800,000), compared to the population of Berlin (over 3,500,000).
A similar analysis, but with a smaller number of cases, can be carried out on the example of the Wieliczka commune. Additionally, in this case, switching off the street lighting in the city impacts the zenith surface brightness of the night sky at the measuring points located in the neighbouring communes, up to a distance of approx. 12 km (
Figure 20).
No change in the value of Sa, which could be associated with the shutdowns of street lighting in Cracow or the surrounding communes, was recorded at the measuring points in Kasinka Wielka (KAS, 40 km from Cracow) and at Suhora Mt. (SUH, 55 km from Cracow).
The above considerations apply to the case of the cloudless sky. However, at several measuring points, it was possible to analyse the impact of switching off street lighting in Cracow on the surface brightness of the overcast sky.
The most complete research of this type was carried out at the BOT measuring point located in the centre of Cracow. To determine the degree of cloudiness, and especially the genus of clouds, both the method of discrete derivatives [
72,
73] and the data of the meteorological station located at this point can be used. Throughout several nights, it was observed that in the presence of high-level clouds (and few middle-level clouds), when street lighting was turned off, the surface brightness curve typical for a cloudy sky “flattened”, assuming the appearance characteristic of a cloudless sky (
Figure 13). This is in line with previous observations [
73,
74], according to which the noticeable scattering of light on the high-level clouds occurs only in large cities with strong radiance. A similar effect was not observed in other cities where the brightness of the night sky was continuously measured (Wieliczka and Dobczyce). It is also not visible, even in Cracow, in the case of low-level clouds, e.g., of the Stratus genus (
Figure 14).
At the KPO and KPO2 measuring points, located within Cracow, where manual measurements of the sky surface brightness were carried out along with noting the genus of clouds and the degree of cloud cover, it was found that with the low-level clouds, the S
a value at the moment of switching off the street-lighting changes by 0.5–0.7 mag/arcsec
2, and this value does not depend on the genus or altitude of clouds. Analogous measurements carried out in Zabierzów (ZAB) and Jerzmanowice (JER) at the moment of switching off street lighting in Cracow showed that with low-level clouds of the genus of Stratus and Nimbostratus, the effect of changing S
a is very weak and amounts to only approx. 0.06 mag/arcsec
2, while in the case of Stratocumulus clouds, it approaches 1.00 mag/arcsec
2. This means that both the altitude of clouds and their genus may be important. Unfortunately, a small number of measurements does not allow for more detailed conclusions. However, it seems that these observations are consistent with those reported in the literature [
74,
75].
5. Conclusions
The analysis of VIIRS/DNB data showed that in each of the researched communes switching off street lighting significantly decreased the radiance. This effect is most clearly visible in urban or urban–rural communes with a high degree of urbanisation. For these communes, including Cracow as a commune, as a result of switching off all street lighting in cities, the radiance decreased by approx. 50% of values before the pandemic. In the case of rural communes (or communes with a dominant rural function), the corresponding decrease in radiance was approx. 35%. This means that in cities half of the light energy emitted into the sky comes from badly constructed street lighting. The other half comes from the lighting of private properties, parking lots, illuminated advertisements, etc. In communes with a predominant rural function, about one-third of the light energy is lost in this way—the remaining two-thirds come mainly from the lighting of individual farms and industrial plants. Unfortunately, the research covered only one rural commune (Zabierzów), where the dominant contribution to radiance comes from a single, bright object—a large greenhouse. Switching off its lighting reduced the commune’s radiance by approx. 45% of the value before the pandemic.
Turning off street lighting and the resulting reduction in the amount of energy emitted to the sky obviously reduce the brightness of the sky glow, both in the case of cloudless and cloudy skies. In the case of a cloudless sky, the difference between the decrease in the surface brightness of the sky glow over the large city (Cracow) (amounting to approx. 1.7 mcd/m
2, i.e., approx. 39%) and the same value determined for smaller cities, such as Dobczyce and Wieliczka (amounting to 0.4 and 0.2 mcd/m
2, i.e., 22% and 15%, respectively), is evident. It is interesting that turning off all street lighting in Cracow reduces the radiance by, in fact, such a small amount. This effect and the difference between the relative decrease of radiance from Cracow and the one from smaller cities should probably be associated with the various concentration of atmospheric light scattering centres, especially with the density of particulate matter (PM). The decisive impact of PM on the brightness of the cloudless sky has already been found earlier by the author of this paper (it should be kept in mind that Cracow is one of the most polluted cities in the world) [
27,
76]. The research by Jechow and Hölker [
48] also indicates the possibility of such correlation in the pandemic period in Berlin, but a similar effect in the Małopolskie Voivodeship will be the subject of a separate publication.
In the case of overcast nights in Cracow, a significant absolute difference was found between the decrease in the surface brightness of the night sky in the presence of low- and medium-level clouds (20.1 mcd/m2) and in the presence of high-level clouds (1.8 mcd/m2). However, the relative decrease in surface sky brightness slightly depends on the genus of clouds and amounts to approx. 43%, compared to the situation before switching off the street lighting. This value is similar to that found in the case of the cloudless sky (39%).
Therefore, it can be concluded that turning off all street lighting in a large city reduces the amount of light energy radiated into the sky by about 50%, while reducing the surface brightness of the night sky by about 40%, regardless of the state of the atmosphere.
In the case of smaller cities (Dobczyce and Wieliczka), the effect of reducing the surface brightness of the overcast night sky was not observed. It can only be stated that this change was smaller than the amplitude of changes in brightness associated with the variability of cloud cover. It gives the upper limit of reducing the sky brightness to 60%, which does not exclude a value analogous to that in Cracow.
The measurements of the impact of changes in the brightness of the light source, which is the city, on the zenith surface brightness of the sky at measuring points of different distances, allowed the verification of previous theses [
73,
76,
77]. It was found that these changes are still visible at a distance of 24 km from Cracow, which confirmed the previously established size of the city’s light island [
25].