A study of the influence of tropospheric subsidence on spring and summer surface ozone concentrations at the JRC Ispra station in northern Italy
- 1Academy of Athens, Research Center for Atmospheric Physics and Climatology, Athens, Greece
- 2European Commission, Joint Research Centre (JRC), Directorate for Energy, Transport and Climate, Air and Climate Unit, 21027 Ispra (VA), Italy
- 3European Commission, Joint Research Centre (JRC), Directorate for Nuclear Safety and Security, 21027 Ispra (VA), Italy
- 4Department of Environmental Science, iCLIMATE, Aarhus University, Frederiksborgvej 399, 4000 Roskilde, Denmark
- 5Laboratoire Interuniversitaire des Systèmes Atmosphériques (LISA), UMR 7583, CNRS, Université Paris-Est-Créteil, Université de Paris, Institut Pierre Simon Laplace, Créteil, France
Correspondence: Pavlos Kalabokas (email@example.com)
The influence of tropospheric ozone on the surface ozone concentrations is investigated at the monitoring station of JRC Ispra, based on 10 years of measurements (2006–2015) of surface ozone data. In situ hourly measurements of ozone and other air pollutants, meteorological parameters, and weekly averaged 7Be (as an indicator of upper-tropospheric–stratospheric influence) and 210Pb measurements (as an indicator of boundary layer influence) have been used for the analysis. In addition, IASI + GOME-2 and IASI ozone satellite data have also been used. It is observed that frequently 7Be and ozone weekly peaks coincide, which might be explained by the impact of deep atmospheric subsidence on surface ozone, particularly during late spring and early summer. Based on this observation, a detailed analysis of selected 7Be and ozone episodes occurring during that period of the year has been performed in order to further elucidate the mechanisms of tropospheric influence on the surface pollutant concentrations. For the analysis, composite NOAA/ESRL reanalysis synoptic meteorological charts in the troposphere have been used as well as IASI satellite ozone measurements and NOAA HYSPLIT back trajectories. The JRC station hourly measurements during subsidence episodes show very low values of local pollution parameters (e.g., NOx, 222Rn, nephelometer data, PM10), close to zero. Conversely, during these periods ozone levels usually reach values around 45–60 ppb during the afternoon hours but also show significantly higher values than the average during the night and morning hours, which is a sign of direct tropospheric influence on the surface ozone concentrations.
It has been reported that tropospheric ozone levels as well as surface ozone concentrations have increased significantly during the last couple of centuries (Volz and Kley, 1988; Forster et al., 2007; Monks et al., 2015; Gaudel et al., 2018). Ozone is an important greenhouse gas and can cause adverse effects on human health and also have negative impacts on vegetation and materials (Ito et al., 2005; Van Dingenen et al., 2009; Hollaway et al., 2012). Tropospheric ozone is mainly produced in the troposphere through photochemical reactions of precursor pollutants but it does also originate from stratospheric intrusions (Volz and Kley, 1988; Staehelin et al., 1994). On average, the tropospheric ozone originating from the stratosphere is about 10 % on a global scale (Monks et al., 2015). The surface ozone concentrations depend on photochemistry and transport within the boundary layer as well as tropospheric entrainment, which might also be associated with deep tropospheric subsidence, especially over the Mediterranean during summer where, in general, high ozone levels are observed (Kalabokas et al., 2000; Kouvarakis et al., 2000; Lelieveld et al., 2002, 2009; Zerefos et al., 2002, 2007, 2008, 2013, 2015; Gerasopoulos et al., 2005; Velchev et al., 2011; Richards et al., 2013; Cooper et al., 2014; Safieddine et al., 2014).
The influence of intercontinental ozone transport on surface ozone concentrations is considered a critical issue regarding ozone pollution control (UNESCE, 2010) and this issue has been extensively studied, especially in the USA where many studies have shown that tropospheric transport and entrainment of ozone from the free troposphere to the boundary layer has an important impact on surface ozone-mixing ratios (Cooper et al., 2011, 2012; Parrish et al., 2013, 2014; Langford et al., 2015). Also, anticyclonic synoptic conditions are normally linked to tropospheric subsidence, which is considered to be an important source of high ozone concentrations over the eastern Mediterranean. During the summer period, the Mediterranean area is under the influence of the descending branch of the Hadley circulation (Lelieveld, 2009) in combination with the impact of the Indian monsoon, inducing a Rossby wave that through the interaction with the midlatitude westerlies produces adiabatic descent in the area (Rodwell and Hoskins, 1996, 2001; Tyrlis et al., 2013). In the eastern Mediterranean strong deep subsidence throughout the troposphere to the boundary layer, which seems to be a quite frequent phenomenon, has been documented based on the analysis of MOZAIC vertical ozone profiles as well as surface ozone and satellite measurements (Kalabokas et al., 2007, 2008, 2013, 2015; Eremenko et al., 2008; Foret et al., 2009; Liu et al., 2009; Doche et al., 2014; Gaudel et al., 2018). In addition, large-scale atmospheric modeling simulations (Li et al., 2001; Richards et al., 2013; Zanis et al., 2014; Safieddine et al., 2014; Tyrlis et al., 2014; Akritidis et al., 2016; Cristofanelli et al., 2018) show the importance of the vertical ozone transport over the Mediterranean basin, especially in its eastern side. Also, sea-breeze circulation appears to have a particularly strong influence on ozone formation in the western Mediterranean, because it favors accumulation of ozone in recirculated polluted air masses (Millan et al., 1997, 2000; Castell et al., 2008). The atmospheric processes controlling ozone levels over the western and central Mediterranean need further studying, especially for what concerns the springtime months. It has been reported that surface background ozone levels in the western and central Mediterranean show a maximum in spring (April–May), while at the eastern Mediterranean stations a later ozone maximum appears in July–August (Kalabokas et al., 2008; Zanis et al., 2014). Also, it has been recently reported that high springtime ozone concentrations are detected over a large geographical area for several days under specific synoptic conditions, which could be explained by the impacts of tropospheric subsidence (Kalabokas et al., 2017). Apart from tropospheric subsidence influencing near-surface ozone concentrations, it has to also be mentioned that there are climatological and case studies of stratospheric intrusions affecting near-surface ozone concentrations for the Mediterranean region (Kentarchos et al., 1998; Cristofanelli et al., 2006; Gerasopoulos et al., 2006; Akritidis et al., 2012).
Atmospheric radionuclides are useful for studies of tropospheric subsidence and transport, in particular terrigenous 210Pb and cosmogenic 7Be, which are natural radionuclides that are helpful in understanding the roles of transport and/or scavenging in controlling the behavior of radiatively active trace gases and aerosol (WMO-GAW, 2004; Feichter et al., 1991; Balkanski et al., 1993; Koch et al., 1996; Graustein and Turekian, 1996; Arimoto et al., 1999; Gerasopoulos et al., 2001; Zanis et al., 2003; Liu et al., 2004; Leppanen et al., 2010; Pham et al., 2011; Garcia et al., 2012; Jiwen et al., 2013; Cuevas et al., 2013; Ioannidou et al., 2014; Brattich et al., 2017). Due to their different origins, the investigation of 210Pb and 7Be activities can be simultaneously useful for studies of atmospheric transport of pollutants, especially in the particle phase (Koch et al., 1996). 210Pb has a half-life of about 22 years. It originates from the decomposition of 222Rn, which has a half-life of 3.8 d and it is a decomposition product of 226Ra originating from the ground (Baskaran, 2011). 7Be has a cosmogenic origin and it is formed mostly by the decomposition of the atoms of carbon, nitrogen and oxygen present in the atmosphere by incident gamma radiation. It has a half-life of 53.3 d (Masarik and Beer, 1999). Its production rate increases with altitude and saturates at about 15 km height (Usokin and Kovaltsov, 2008). Most of 7Be is produced in the stratosphere and about one-third in the troposphere, especially in its upper part (O'Brien, 1979). After their formation, 7Be atoms are mostly attached to atmospheric particles and so their atmospheric concentrations are greatly influenced by transport and deposition processes of particles (Jaenicke, 1988; Feely et al., 1989; Papastefanou and Ioannidou, 1995; Koch et al., 1996; Bourcier et al., 2011; Duenas et al., 2011; Lozano et al., 2012; Steinmann et al., 2013; Hernández-Ceballos et al., 2016).
On average, the 7Be concentrations in the upper troposphere are about 25 % of the lower stratospheric concentrations (about 160 mBq m−3) at northern midlatitudes while 7Be concentrations close to the ground are generally below 5 mBq m−3 (Reiter et al., 1983; Dutkiewicz and Husain, 1985; Brost et al., 1991; Gaggeler, 1995). Thus, air masses originating from the upper troposphere or stratosphere usually contain high 7Be concentrations, and the intrusions of stratospheric air mass into the troposphere are the main processes transferring 7Be to the earth's surface through dry or wet deposition. Therefore, 7Be serves as a tracer for lower-stratospheric and upper-tropospheric air masses arriving to the ground (Lee et al., 2007; Papastefanou et al., 2012). Due to the exchange and removal processes in the atmosphere, the 7Be concentration in air at ground level varies strongly with the season while 7Be production rates in the atmosphere remain relatively constant (Durana et al., 1996; Masarik and Beer, 1999). In general, 7Be surface concentrations show a maximum in late summer (Reiter et al., 1983; Feely et al., 1989; Bourcier et al., 2011; Hernández-Ceballos et al., 2016).
The investigation of the atmospheric processes controlling the frequently observed springtime ozone maximum over parts of the European continent including the western Mediterranean is an interesting research issue as photochemical ozone production and tropospheric transport, including stratospheric influence, might be involved (Beekmann et al., 1994; Monks, 2000). It has been previously reported that high surface ozone concentrations, lasting several days, have been observed over large geographical areas at the same time (Kalabokas et al., 2017). It has also been shown that the observed regional springtime ozone episodes are usually associated with specific synoptic meteorological patterns, which have great similarities to those observed during the summertime ozone episodes over the eastern Mediterranean and are linked to large-scale subsidence (Kalabokas et al., 2013, 2015; Doche et al., 2014).
In the previous study (Kalabokas et al., 2017) some tropospheric mechanisms related to regional ozone episodes especially linked with large-scale subsidence were examined. In this paper a more detailed analysis of the suggested mechanisms was performed, based on the measurements of 7Be, 210Pb and a large variety of meteorological and air pollution parameters collected at the JRC Ispra station, which is considered to be one of the most well-equipped measuring sites in Europe. The present study focuses on the influence of tropospheric subsidence on surface ozone concentrations, especially during spring and summer months over the western Mediterranean area. It is based on the analysis of 10 years of ozone and other air pollution measurement data (2006–2015) as well as measurements of natural radionuclide tracers at surface level, which can be used as tracers of transport and photochemical and removal processes. These data are collected at the JRC Ispra site, located in the pre-Alpine area in northern Italy but also located relatively close to the western Mediterranean. In addition, we used meteorological maps, back trajectories and IASI satellite ozone data for a better understanding of the relative importance of the contributions of the different sources of ozone, especially the role of the vertical transport in the troposphere. To our knowledge, a similar analysis of such multiparameter long-term measurements has not yet been performed so far for this area.
2.1 Site description
The JRC Ispra station (45.807∘ N, 8.631∘ E, 223 m a.s.l.) is located in a valley in the pre-Alpine area of northern Italy. A general meteorological characteristic of the area is that low winds usually prevail with occasional northerly Foehn events (Mira-Salama et al., 2008). More details about the site can be found in Putaud et al., 2017.
2.2 Instrumentations and measurements at JRC Ispra site
The information on the instrumentation used for this investigation is presented in Table 1.
Regarding the meteorological measurements, a WXT510 weather transmitter from Vaisala simultaneously recorded six meteorological parameters, temperature, pressure, relative humidity, precipitation, wind speed and wind direction, from the top of an about 10 m high mast. Humidity (ppmV) was calculated from relative humidity (RH), temperature and atmospheric pressure, which was useful for the data analysis as an air mass reaching the surface by transport from higher altitudes will typically be relatively dry and entrainment of air from the free troposphere is thus normally associated with a drop in humidity mixing ratio as well as specific humidity.
2.3 Meteorological maps and back trajectories
Composite NOAA/ESRL reanalysis meteorological charts of various meteorological parameters for selected ozone episodes and at the atmospheric pressure levels of 850, 700 and 500 hPa have been produced with a horizontal resolution of (Kalnay et al., 1996). Due to space limitations, mostly the 700 hPa charts, representative for the free troposphere, are presented. In addition, 6 d NOAA/HYSPLIT back trajectories for selected high-ozone days for air masses arriving at the JRC Ispra site at various end points have been plotted, using the GDAS meteorological data (Draxler and Rolph, 2015).
2.4 IASI and IASI + GOME-2 satellite ozone measurements
Progress in satellite observations of tropospheric ozone has been made during the last decade (e.g., Fishman et al., 2003; Liu et al., 2005; Coheur et al., 2005; Worden et al., 2007; Eremenko et al., 2008, Cuesta et al., 2013). This progress combined with its spatial coverage and horizontal resolution make it possible to use such observations to complement in situ observations and to support the analysis of ground measurements as well as modeling simulations. In this study, we use ozone satellite observations derived from the IASI infrared instruments and from the multispectral synergism of IASI and GOME-2 in the ultraviolet range, for enhancing sensitivity to ozone closer to the surface. The first IASI instrument (Clerbaux et al., 2009) was launched on board the MetOp-A platform on 19 October 2006. It is a Fourier transform spectrometer operating at nadir in the thermal infrared between 645 and 2760 cm−1 with an apodized spectral resolution of 0.5 cm−1. IASI monitors atmospheric composition twice a day at any (cloud-free) location at high resolution with its swath width of 2200 km and its field of view composed of a 2 pixel × 2 pixel matrix with a diameter at nadir of 12 km each (e.g., Boynard et al., 2009; George et al., 2009; Clarisse et al., 2011; Coman et al., 2012). As in Doche et al. (2014), IASI ozone concentrations retrieved at 3 and 10 km height are used for our analysis as being representative of the lower and upper troposphere, respectively. The maximum of sensitivity of IASI retrievals ranges between 3 and 5 km in the lower troposphere and 9 and 12 km in the upper troposphere. Several studies show that the ozone concentrations retrieved from IASI in the lower and upper troposphere are mainly uncorrelated (Dufour et al., 2010, 2012, 2015). We use the vertical profiles retrieved from IASI to calculate the longitudinal transect for different latitudes. Vertical profiles within 1∘ in latitude and 0.5∘ in longitude are averaged in the transect calculation.
The satellite multispectral approach used here is called IASI+GOME-2 (Cuesta et al., 2013). It is based on the joint and simultaneous use of both GOME-2 and IASI measurements for deriving a unique ozone profile for each pair of spectra. It is designed for observing the lowermost tropospheric ozone located below 3 km of altitude (with typically a peak of maximum sensitivity down to 2 km of altitude), which is not directly observed with single-band retrievals. Like IASI, GOME-2 is only on board the MetOp satellite series and offers global coverage every day (for MetOp-A around 09:30 local time) with a swath width similar to that of IASI and a ground resolution moderately coarser than that of IASI (pixels of 80 km × 40 km for GOME-2). As described in detail by Cuesta et al. (2013), co-located IR and UV spectra are jointly fitted to retrieve a single vertical profile of ozone for each pixel at the IASI horizontal resolution. The UV measurements from the closest GOME-2 pixel (without averaging) are used for each IASI pixel. As for IASI-only retrievals, a priori ozone profiles representative of tropical, midlatitude and polar conditions are calculated by averaging the climatological ozone profiles from McPeters et al. (2007) over the 20–30, 30–60 and 60–90∘ N latitude bands. The selection of the a priori profiles used during the retrieval is based on the tropopause heights (determined by the temperature vertical profile for each IASI pixel) above 14 km, between 14 and 9 km, and below 9 km, respectively. IASI + GOME-2 retrievals are routinely produced at the global scale by the French data center AERIS and they are publicly available (https://iasi.aeris-data.fr/O3_IAGO2/, last access: 15 May 2019).
3.1 Seasonal variation in O3 concentrations, 7Be concentrations and the 7Be ∕ 210Pb ratio
For the investigation of entrainment episodes and based on information presented in the introduction, plots of weekly averages of ozone vs. 7Be concentrations and that of ozone vs. 7Be∕210Pb ratios were made for all years during the examined period (2006–2015), and the year 2011 is shown as an example (Fig. 1a, b). As observed, 7Be and O3 peaks coincide in several cases, which might be explained by an impact of deep atmospheric subsidence (air masses moving down from the stratosphere–upper troposphere) on surface ozone. Particularly during springtime, the high ozone levels during such events may be influenced by ozone-rich air being transported down to the boundary layer from the stratosphere–upper troposphere.
As seen in Fig. 1a–b, in May 2011 and in a period around the end of June 2011 and beginning of July 2011, there were episodes of downward transport of ozone to the surface from the above tropospheric layers. The relatively higher 7Be∕210Pb ratios at the end of the spring to the beginning of the summer seasons (mid-April to mid-July) indicate that stratospheric or upper-tropospheric influence should be most important during this period.
In addition, in Fig. 1c–d the 7Be activity and the 7Be∕210Pb ratio are presented together with specific humidity. As observed, very often the local 7Be∕210Pb maxima coincide with local minima of specific humidity, which supports the assumption that this isotope ratio is an indicator of the relative importance of entrainment of subsiding dry air originating from the upper atmospheric layer into the boundary layer and the ground surface. The 7Be activity does not show a similar correlation with specific humidity. If we look at the yearly variation in the isotope ratio, it has a maximum in the early summer while specific humidity has a maximum later in the summer, which may be explained by the fact that warm air can contain more water vapor.
The 7Be∕210Pb peaks in some cases coincide with ozone peaks, but local 7Be activity peaks are found to more frequently coincide with local ozone maxima. Thus the radioisotope data are consistent with the hypothesis that maximum ozone values are frequently reached in situations where there is a combined impact of entrainment of ozone-rich air brought down by subsidence (high 7Be activities) and stagnant atmospheric conditions (high 210Pb activities), favoring ozone formation in the boundary layer. In such conditions, 7Be activities will be high, but not the 7Be∕210Pb ratio. This is illustrated in Fig. 1 for the year 2011, but a similar picture is seen during other years, where observations are available (see Fig. S1–S4 in the Supplement).
As reported in the literature, stratospheric ozone intrusions in the Mediterranean occur most frequently from March to July (Beekmann et al., 1994; Monks et al., 2000). An ozone increase is generally observed during spring months, associated with the increase in solar radiation and photochemistry (Monks et al., 2000) but also with tropospheric downward transport (Kalabokas et al., 2017), and thus some caution would be needed in the data analysis as the increase in O3, 7Be and 7Be∕210Pb at the same time is not necessarily related to the impact of stratospheric intrusions. However, the occurrence of 7Be∕210Pb peaks above the baseline level can be interpreted as evidence of deep atmospheric subsidence followed by entrainment into the boundary layer. The episodes in May and June 2011 with high ozone and 7Be∕210Pb values (Fig. 1) appears to be due to such deep tropospheric subsidence as indicated by synoptic meteorological maps, back trajectories and IASI satellite data. Such specific episodes will be examined in detail later in the following section.
Table 2 shows the average monthly values for spring, summer and autumn (March to October) of 7Be, 7Be∕210Pb and O3 (12–18 afternoon mean) for all of the years 2006–2015 when measurements were available. The 7Be concentrations show maximum monthly values in June–July, the same as ozone, while the 7Be∕210Pb ratio has its peak values in the April–June period, which would indicate enhanced deep tropospheric subsidence during this period of the year.
3.2 Investigation of the main synoptic characteristics during the May–July ozone episodes
As the May–July period seems to be the most important one regarding the influence of subsidence on ozone concentrations, as a next step selected weekly high 7Be and ozone episodes during the May–July period will be examined. More than 10 weekly 7Be and ozone episodes were identified in the whole time series and the three most characteristic of them, for what concerns signs of tropospheric subsidence as observed in the meteorological and air pollution measurements (high 7Be and O3 concentrations combined with positive omega and dry air masses), will be presented in the following paragraphs. The selected episodes were 3–10 May 2011, 23–29 May 2012 and 28 June–4 July 2011. The episodes discussed here are not Foehn events.
3.2.1 May 2011 ozone episode
In Fig. 2 the composite NOAA/ESRL weather maps of geopotential height, wind speed, omega vertical velocity and specific humidity for the episode of 3–10 May 2011 (as well as the corresponding 3–10 May climatology charts) at JRC Ispra are shown. A strong low-pressure system is observed over the Atlantic and a weaker one over eastern Europe and the Black Sea while anticyclonic conditions prevail over western and central Europe in a vast region extending from Scandinavia to the Mediterranean. In this region strong subsidence is observed as deduced from the charts of omega vertical velocity and specific humidity, indicating large-scale downward movement of dry air masses. Similar subsidence conditions have already been observed during regional spring ozone episodes over the western Mediterranean, especially related to the interface of an anticyclone and a low-pressure system located further east (Kalabokas et al., 2017).
3.2.2 May 2012 ozone episode
The above feature is also clearly seen in the following selected episode of 23–29 May 2012 (Fig. 3), with a much stronger anticyclone established over the North Sea (weekly averages measured at Ispra: 7Be: 7117 µBq m−3; 7Be∕210Pb ratio: 9.6; ozone: 54.9 ppb). The corresponding IASI and IASI + GOME-2 satellite images as well as IASI vertical sections at various latitudes from 60 to 45∘ N for ozone concentration at 3 km and 10 km are shown in Figs. 4–6. The IASI + GOME-2 maps show enhanced ozone concentrations at 3 km over Germany, France and Italy, which seem disconnected from the values at 10 km. In a general way, IASI-GOME-2 ozone concentrations at 3 km seem more independent of those at 10 km than are those derived from IASI at the same altitudes, which is expected because the number of degrees of freedom is larger. It appears that the geographical distribution of tropospheric ozone as well as the movement of the high-ozone reservoirs at both altitude levels generally follow the synoptic weather patterns (Figs. 3, 4). An extended high-ozone area appears to the east of the anticyclone at both tropospheric levels apparently originating from the north and is an extension of the northern polar high-ozone reservoir. It has to be added that back trajectories show air masses arriving at the Ispra site from the N-NE direction and from higher altitudes, especially on 25–27 May (not shown). This behavior is usually encountered in the analysis of many spring ozone episodes over the area as the 6 d back trajectories usually originate from the region of high tropospheric ozone subsidence over central and eastern Europe, thus inducing high ozone background levels of tropospheric origin at the boundary layer and at the surface to which the photochemical ozone buildup might eventually be added.
3.2.3 June–July 2011 ozone episode
The next episode of 28 June–4 July 2011 seems to be quite representative of early summer ozone episodes over the area and will be examined in more detail by taking into account many relevant atmospheric measurements recorded at the JRC Ispra station. During this episodic event, very high 7Be concentrations as well as 7Be∕210Pb ratio values have been recorded, which were actually the highest weekly averages for 2011 (Fig. 1a, b). Regarding the weather conditions, it has been mostly sunny throughout the week with some rain on the second day and light northwesterly winds.
The synoptic conditions (Figs. 7–8, S5) show the existence of an extended deep low-pressure system over the Atlantic in the free troposphere (at 500–700 hPa) and also another one over central Europe in the boundary layer (at 700–1000 hPa), while high atmospheric pressure prevails over most of the European continent, including Scandinavia. Following the examination of the meteorological charts, it has been observed that massive subsidence occurs over a wide area over the Atlantic and western Europe towards the Mediterranean, including the Alpine region, peaking on 1–3 July. Indeed, specific humidity charts at various pressure levels (Fig. S5) show an extended area of dry air masses over the Atlantic (northern Spain and western France) at lower latitudes, moving towards the European continent and the Mediterranean following the synoptic flow (Fig. 7). The omega vertical velocity charts show that the descending motion is stronger at higher altitudes but at the same time there is an accumulation of dry air masses over the Atlantic (indicating subsidence), which are displaced according to the above-described synoptic pattern. In addition, the tropospheric ozone distribution as measured by the IASI and IASI + GOME-2 satellites at 3 and 10 km follows the synoptic patterns (Figs. 9–11). As observed on 30 June and 1 July, there is a large zone of enhanced ozone at 10 km, but also at 3 km, descending from the North Sea to the Alps, and which corresponds to a through east of the ridge. On 2 and 3 July, the trough developed to a cutoff low located over SE Poland and so did high ozone values at 10 km.
The above-described characteristics related to subsidence are much more pronounced if only 1–2 July is considered, especially the large-scale descending tendency of tropospheric air masses at all pressure levels over central and northern Europe, which is subsequently associated with extended tropospheric dryness over these areas (Figs. S6–S8).
In addition, according to the back-trajectory plots the subsiding air masses arrive at the JRC Ispra site from the Atlantic coast and France (Fig. 16). Almost all back trajectories arrive from the north, where the subsidence area is located (Figs. 9–10, S5) and where a large area of tropospheric ozone appears over western Europe, apparently originating from the high-ozone reservoir located over polar regions as shown in the corresponding IASI and IASI + GOME-2 satellite images as well as IASI vertical sections (Figs. 9–11).
The hourly air pollution measurements at the JRC station during the 28 June–4 July 2011 period first show a period (28 and 29 June) with high ozone (daily maximum more than 80 ppb) and PM10 (daily maximum more than 80 µg m−3), related to high temperatures (Tmax 30 ∘C and low wind speed (<1 m s−1). Aerosol is of mainly anthropogenic origin as indicated by different nephelometer responses to red, green and blue light. High ozone values during this period are probably due mainly to photochemical buildup from anthropogenic emissions in the Po valley. During the following period with a maximum of subsidence (1–2 July), ozone concentrations vary around 55–60 ppb with the diurnal concentration range significantly decreased in comparison to the previous days while at the same time the NOx concentrations (Fig. 13a) as well as the humidity, 222Rn, nephelometer and PM10 concentrations (Fig. 13b–d) show minimum values. Please note that the weekly resolution of 7Be measurements does not allow for ascertaining an expected maximum during these 2 d. During the days following the strongest subsidence period (3–4 July) the nocturnal ozone values are significantly reduced as the tropospheric entrainment has diminished while the ozone destruction by NO chemical titration and dry deposition on the ground reduces the concentrations substantially within the generally shallow nocturnal layer. On the other hand, the midday ozone concentrations are slightly increased, probably due to in situ photochemical ozone production, which is added to the increased tropospheric ozone background, due to the regional tropospheric subsidence episode occurring during the previous days. Thus, this period shows an interesting suite of days with strong photochemical ozone production and advection of tropospheric ozone to the ground.
In summarizing the above, it has to be mentioned at first that maximum ozone values in the area of the study are expected to be connected primarily with boundary layer ozone photochemistry. The presented analysis shows that regional tropospheric subsidence occurring frequently in the area during May–July might enable easier exceedances of ozone air quality standards, as photochemical ozone buildup is initiated in a clean boundary layer air mass containing already high ozone levels (i.e., 50 ppb), which is common after a regional tropospheric subsidence episode in the area. This phenomenon may explain the spring ozone maximum observed over many stations over the western and central parts of the European continent including the western Mediterranean. In relation to the above, it has been mentioned in the introduction that a similar phenomenon is observed in the eastern Mediterranean, reaching a maximum later in summer though (July–August).
The present study focuses on the influence of tropospheric subsidence on surface ozone concentrations, especially during spring and summer months over the western Mediterranean area. It is a much more detailed extension of a previous study (Kalabokas et al., 2017) where some tropospheric mechanisms related with regional ozone episodes in particular linked with large-scale subsidence were examined. This study is focused on a more detailed analysis of the suggested mechanisms, based on the measurements of 7Be, 210Pb and a very large variety of meteorological and air pollution parameters collected at the JRC Ispra station, which is considered to be one of the most well-equipped measuring sites in Europe. High boundary layer concentrations of 7Be are used as an indicator of the influence of free tropospheric air, in which 7Be activity is high due to a cosmogenic source. 210Pb activity is an indicator of accumulation of surface emissions and their reaction products and it reaches its highest levels during periods with stagnant air conditions. Radioisotope and humidity data from the Ispra station show that local peaks in 7Be∕210Pb frequently coincide with local minima in specific humidity, consistent with the hypothesis that these peaks are found in situations with a strong impact of free tropospheric influence on the boundary layer. Comparison with ozone measurements shows that these peaks on some occasions coincide with ozone peaks but more frequently ozone peaks coincide with peaks in 7Be activity. This observation was interpreted as a result of the fact that the highest ozone concentrations are frequently found in situations with a combined impact of entrainment of ozone-rich free tropospheric air and local formation in the boundary layer. The conclusions derived from the analysis of specific episodes were in accordance with this interpretation: the main characteristics of the frequently occurring spring episodes where both 7Be and ozone reach maxima at the Ispra station were found to be the following.
Anticyclonic stagnant conditions occur over parts of the European continent and the western Mediterranean.
Strong winds occur at the periphery of the anticyclone associated with a deep low-pressure system located to the north and a weaker one located to the east. A common feature is that Ispra is located at the eastern edge of a ridge system at the 700 hPa level and at the same time a trough is located eastwards.
Very extended areas of positive vertical velocity and omega (downward movement) are observed over eastern, central and western Europe, depending on the locations and the relative strength of the high- and low-pressure systems, at all pressure levels and associated with dry conditions (low specific humidity), indicating subsidence.
At the same time, the IASI satellite images show important ozone reservoirs in the upper and lower troposphere, which are generally delimitated by the meteorological systems and follow their movement, while large areas of enhanced tropospheric ozone appear over the region of subsidence, usually originating from the tropospheric ozone reservoirs associated with the low-pressure systems. These results consolidate the findings of the first phase of this study on spring ozone episodes in the western Mediterranean (Kalabokas et al., 2017) and extend them over a full year and a longer time period. The characteristics described above are also encountered during some summer episodes (in June–July) but the conditions generally observed in summer episodes are more related to local photochemical ozone production in the boundary layer while tropospheric subsidence is weaker and more concentrated over the eastern Mediterranean.
The most important new findings of this paper are as follows.
The examination of the Ispra station hourly measurements during subsidence episodes shows that the local pollution parameters (e.g., NOx, 222Rn, nephelometer, PM10) tend to have low values (compared to those observed during periods of anthropogenic pollution), while the ozone levels usually reach values around 45–60 ppb during the afternoon hours but show significantly higher values than the average during the night and morning hours. This is a clear sign of tropospheric entrainment to the boundary layer.
During high 7Be and high ozone episodes, the highest ozone values exceeding the standards usually occur within the following 2–3 d after the maximum of regional tropospheric subsidence. The increase in ozone concentrations usually occurs under the influence of favorable meteorological conditions for photochemical ozone production in the boundary layer, which is added to the increased regional background due to tropospheric subsidence and thus occasionally leading to exceedances in ozone air quality standards.
The results of this study might be useful for helping the required improvements in the veracity of global ozone air quality models for which biases have been made evident by several recent studies (Cooper et al., 2014; Parrish et al., 2014; Gaudel et al., 2018; Young et al., 2018). Indeed, these models need to accurately represent complex vertical transport processes affecting the surface ozone budget.
The following data sources were used: Table 2: The JRC-station data used in this study are available from the authors upon request (firstname.lastname@example.org, email@example.com) Figures 1 and 13: JRC-station data. Figures 2, 3, 7 and 8: NOAA/ESRL charts, https://www.esrl.noaa.gov/psd/data/composites/day/ (last access: 5 May 2019, NOAA/ESRL, 2019). Figures 4, 5, 9 and 10: IASI satellite data. The IASI satellite data used in this study are available from the authors upon request (firstname.lastname@example.org). Figures 6 and 11: Satellite observations of lowermost tropospheric ozone from the IASI + GOME2 multispectral approach can be provided upon request to Juan Cuesta from the LISA laboratory (email@example.com). From 2017, global IASI + GOME2 ozone retrievals are freely available at the AERIS data center at https://iasi.aeris-data.fr/o3_iago2/ (last access: 3 February 2020, Boonne and Cuesta, 2020). Figure 12: NOAA/Hysplit back-trajectories, http://ready.arl.noaa.gov/hypub-bin/trajtype.pl?runtype=archive (last access: 5 May 2019, NOAA, 2019).
The supplement related to this article is available online at: https://doi.org/10.5194/acp-20-1861-2020-supplement.
PK, NRJ and JH prepared the manuscript with contributions from all co-authors to the manuscript/data evaluation. MR provided 7Be and 210Pb data. NRJ and JH provided ozone and NOx data. PK provided synoptic meteorological maps and back trajectories. GF, GD, ME and MB provided the IASI satellite ozone measurements.
The authors declare that they have no conflict of interest.
The authors would like to acknowledge the following people: Sebastiao Dos Santos and Jean-Philippe Putaud for meteorological data and aerosol physics data, Giovanni Manca for 222Rn data, and Friedrich Lagler and Jean-Philippe Putaud for the help with the ozone and NOx data. The authors also acknowledge that a small part of the material in the present paper has been previously presented in Jensen et al. (2017) (Fig. 1). Acknowledgement is also made for the composite weather maps, which were provided by the NOAA/ESRL Physical Sciences Division, Boulder, Colorado, from their website at http://www.cdc.noaa.gov/ (last access: 15 May 2019). The authors also acknowledge the NOAA Air Resources Laboratory (ARL) for the provision of the HYSPLIT transport and dispersion model and/or READY website (http://www.ready.noaa.gov, last access: 15 May 2019) used in this publication. LISA acknowledges CNES (Centre National des Etudes Spatiales)/TOSCA (Terre Océan Surface Continentale Atmosphère) and PNTS (Programme National de Télédétection Spatiale) for endorsing the development and production of ozone observations from IASI + GOME-2 and IASI.
This paper was edited by Evangelos Gerasopoulos and reviewed by two anonymous referees.
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