{'fraction_non_alphanumeric': 0.03536304666248169, 'fraction_numerical': 0.034735300272023435, 'mean_word_length': 4.6696322657176745, 'pattern_counts': {'":': 0, '<': 0, '<?xml version=': 0, '>': 0, 'https://': 0, 'lorem ipsum': 0, 'www.': 3, 'xml': 0}, 'pii_count': 0, 'substrings_counts': 0, 'word_list_counts': {'cursed_substrings.json': 0, 'profanity_word_list.json': 0, 'sexual_word_list.json': 0, 'zh_pornsignals.json': 0}}
Monitoring of the 2011 spring low ozone events in the Arctic region

Data from FY-3B SBUS and NOAA SBUV/2 were used to monitor ozone levels in the Arctic region from March 1 to April 5, 2011. Results revealed a significant ozone depletion in the area, with total ozone levels between 200–250 DU. The ozone levels recorded were 100–200 DU below normal, and in some parts the levels were as low as 200 DU, indicating a mini ozone-hole. During the sampling period, the ozone depletion area underwent identifiable expansion and detraction, a rotation around the North Pole from the west to the east, and a longitudinal movement from the Pole, spreading to the mid latitudes. The effects of these rare low ozone events were not only felt in the Arctic, but also extended to densely populated areas between Europe and the middle of Russia. In this region, rapidly increasing levels of ultraviolet radiation were detected at the Earth’s surface. Given the significant risk that this poses to both the environment and people’s health, this occurrence has significant global implications.

The depletion of ozone in our atmosphere, especially in the stratosphere, and the resultant effect that this has on the environment, has been a topic of much concern for both atmospheric science and climate change research [1][2][3][4][5]. The discovery of the ozone hole above the South Pole in 1985 provided the first clear evidence that human impacts affect the atmosphere, and was a major catalyst for new research regarding ozone depletion [6]. However, the ozone depletion phenomenon is not unique to the South Polar region, and has occurred at different times and in different places throughout the northern hemisphere [2]. Since 1995, Chinese scientists have continued to monitor the existence of mini-ozone holes over the Tibetan Plateau during the Summer and Winter periods, and have conducted systematic research into the resultant effects of these findings, including seasonal changes and changes in the scope of ozone distributions [7][8][9][10]. Furthermore, European scientists also have made discoveries of ozone depletions, as these phenomena occurred throughout Europe [11][12][13][14][15][16].
The Chinese new generation polar orbit satellite, FY-3, carrying the SBUS (Solar Backscatter Ultraviolet Sounder), is China's first global ozone-monitoring instrument. The design and channels of the device are similar to those of the American NOAA SBUV/2 (Solar Backscatter Ultraviolet). Both instruments have the capability of monitoring global total ozone, as well as vertical ozone profiles [17,18]. In November 2010, the FY-3B SBUS was launched and began its in-orbit test. The precision of the vertical profile data obtained with the FY-3B SBUS marked significant improvements over its predecessor, and is on par with those of NOAA SBUV/2. The FY-3B SBUS is now regularly used for the ozone monitoring program in China. Prior to the introduction of the FY-3B, the FY-3A carrying the TOU (Total Ozone Unit) also delivered reliable and precise ozone measurement data [19,20]. The main difference between the SBUS and TOU lies in the design of channels and observation methods. The SBUS has 12 channels aimed at the surface of the Earth with fixed nadir observation, which provides vertical ozone profile data from the surface to the top of the atmosphere with a spatial resolution of approximately 200 km [17,18]. The TOU, on the other hand, uses 6 channels and a scanning method of observation to obtain global total ozone data with a spatial resolution of 50 km [19,20]. With both the SBUS and TOU on board, the FY-3 is able to take full advantage of two different technical monitoring methods which deliver complete and accurate data relating to both total ozone and vertical distribution levels.
In the spring of 2011, the northern polar region experienced the most significant depletion in ozone levels in recorded history. This occurrence was reported by the WMO (World Meteorological Organization, http://www.wmo.int/ pages/mediacentre/press_releases/pr_912_en.html) and Science (http://www.sciencedaily.com/releases/2011/04110405-102202. html). In this paper, we present the ozone depletion monitoring results using data from the FY-3B SBUS and NOAA SBUV/2s in the Arctic region between March-April, 2011.
The two ozone stereographic polar projection maps in Figure 1 provide a comparison of data obtained from (a) the FY-3B SBUS and NOAA-16, 17, 18 and 19 SBUV/2, with data obtained from (b) the FY-3A TOU over the Arctic region. Figure 2 shows the total ozone distribution map using data from the WOUDC (World Ozone Ultraviolet Radiation Data Centre) over the Arctic region on March 14, 2011. (http://www.theozonehole.com/arctic2001loss.htm). To allow for comparisons, we have revolved the original map to correspond with the longitudinal position in Figure 1.
Comparing Figures 1 and 2, we can see a clear con  sistency between the data obtained from the satellite monitoring and figures obtained from ground observations made by WOUDC. Thus, the similarities between these two sets of figures provides evidence of the reliability and accuracy of the data obtained from the FY-3B SBUS and NOAA SBUV/2. Figures 1 and 2 both reveal that a sharp reduction in ozone levels revolving around the Arctic Circle occurred on March 14, 2011, in the area north of the 72° latitude. In this region, total ozone levels were between 200-250 DU, with sections as low as 200 DU, indicating a mini-ozone hole. Since satellite monitoring of ozone levels began in the 1970s, both vertical ozone profile data and total ozone data revealed that the area around the North Pole normally experiences ozone levels between 300 and 400 DU [21][22][23]. Thus, it can be said that this phenomenon is the first recorded instance of ozone reduction in the Arctic region. From Figure 3, we can further ascertain that the vertical ozone profile data obtained on March 14 show changes in ozone levels mainly in levels 5-10, with a height of around 100-10 hPa. These values correspond to changes from the upper troposphere to the stratosphere. Analyses also revealed that during the period of ozone reduction, ozone levels from the upper troposphere to the stratosphere were approximately 100 DU lower than normal, or 193 DU lower than average high levels. This change represents a change in ozone levels between 77% and 83%. The data also revealed that the bulk of the changes to ozone levels during this phenomenon occurred mainly between the upper troposphere Using data from the FY-3B SBUS and NOAA SBUV/2 constant monitoring from March to April, 2011, we can see the general trend of the ozone depletion in the Arctic region. This instance of depletion in the Arctic region began on March 1, 2011, when ozone distribution levels began to fall (between March 1 and 3) at a relatively fixed area of 80°N, 90°E and 90°W. From March 4, the area of reduction began expanding and revolving around the Pole from west to east. On the 10th, the region of reduction began to spread, heading 90°W and 40°N, where it soon developed into a significantly large region of ozone depletion. From March 11-13, the area began expanding from the Pole to 40°N, and began revolving from west to east, reaching 30°-50°W on the 13th. On the 14th, the area began retracting to the Pole, but extended along 70°N, towards the area around 30°-50°W. On the 15th, the affected area was focused by the Pole, before developing and stretching along a longitudinal path, and following the Pole's slow rotation from west to east. On the 22nd, the area of ozone reduction appeared at 54°N and 120°E, and headed north where it crossed the North Pole and reached 60°N and 60°W in a narrow strip-like manner, with the width extending to the 20° longitude line.
From the 23-25th, the "arm" of the hole appeared spinning anti-clockwise from west to east, and gradually began to break up into parts. From the 25th, the region began extending from the Pole along a longitudinal path until it covered an area with bearings of approximately 45°N, 10°W to 25°W. From March 26 to April 4, the main section of the depletion area covered a region with bearings of approximately 50°N, 10°W to 75°E and, with the Pole at the centre, slowly began rotating from west to east. From March 26, the size of the area began expanding, and reached its largest size on the 28th, before slowly shrinking in area to its smallest size on April 5. The depletion area then gradually began to leave the Polar region, and small sections could be seen moving towards the equator, signaling the end of this occurrence of ozone reduction. Figure 4 outlines the size of the area of ozone reduction at its peak during March 28-31, as the region extended to Europe and the middle of Russia. Figure 4(a)-(d) shows the growth of the area during March 28, 29, 30 and 31, respectively.
As Figure 4 reveals, during the period of March 28-31 the area of ozone reduction extended from the Pole and covered a significant area, including western Europe and central Russia. Total ozone levels for the area were between 230-250 DU, with the sections falling below 220 DU reaching the level of a mini-ozone hole.
This occurrence of ozone depletion over the Arctic region lasted over a month, from March 1 to April 5, 2011. Furthermore, the scope and scale of the area, which covered almost all of Europe and the western parts of Asia, posed a threat to not only the health and safety of the people in this region, but also to the environment. The initial observation