Journal topic
Atmos. Meas. Tech., 12, 5959–5977, 2019
https://doi.org/10.5194/amt-12-5959-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.
Atmos. Meas. Tech., 12, 5959–5977, 2019
https://doi.org/10.5194/amt-12-5959-2019
© Author(s) 2019. This work is distributed under
the Creative Commons Attribution 4.0 License.

Research article 18 Nov 2019

Research article | 18 Nov 2019

# Studies of the horizontal inhomogeneities in NO2 concentrations above a shipping lane using ground-based multi-axis differential optical absorption spectroscopy (MAX-DOAS) measurements and validation with airborne imaging DOAS measurements

Studies of the horizontal inhomogeneities in NO2 concentrations above a shipping lane using ground-based multi-axis differential optical absorption spectroscopy (MAX-DOAS) measurements and validation with airborne imaging DOAS measurements
André Seyler1, Andreas C. Meier1, Folkard Wittrock1, Lisa Kattner1,2, Barbara Mathieu-Üffing1,2,a, Enno Peters1,b, Andreas Richter1, Thomas Ruhtz3, Anja Schönhardt1, Stefan Schmolke2, and John P. Burrows1 André Seyler et al.
• 1Institute of Environmental Physics, University of Bremen, Bremen, Germany
• 2Federal Maritime and Hydrographic Agency (BSH), Hamburg, Germany
• 3Institute for Space Sciences, Freie Universität Berlin, Berlin, Germany
• anow at: State Agency for Agriculture, Environment and Rural Areas of the German Federal State Schleswig-Holstein (LLUR), Flintbek, Germany
• bnow at: Institute for the Protection of Maritime Infrastructures, German Aerospace Center (DLR), Bremerhaven, Germany

Correspondence: André Seyler (aseyler@iup.physik.uni-bremen.de)

Abstract
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This study describes a novel application of an “onion-peeling” approach to multi-axis differential optical absorption spectroscopy (MAX-DOAS) measurements of shipping emissions aiming at investigating the strong horizontal inhomogeneities in NO2 over a shipping lane. To monitor ship emissions on the main shipping route towards the port of Hamburg, a two-channel (UV and visible) MAX-DOAS instrument was deployed on the island Neuwerk in the German Bight, 6–7 km south of the main shipping lane. Utilizing the fact that the effective light path length in the atmosphere depends systematically on wavelength, simultaneous measurements and DOAS retrievals in the UV and visible spectral ranges are used to probe air masses at different horizontal distances to the instrument to estimate two-dimensional pollutant distributions. Two case studies have been selected to demonstrate the ability to derive the approximate plume positions in the observed area. A situation with northerly wind shows high NO2 concentrations close to the measurement site and low values in the north of the shipping lane. The opposite situation with southerly wind, unfavorable for the on-site in situ instrumentation, demonstrates the ability to detect enhanced NO2 concentrations several kilometers away from the instrument. Using a Gaussian plume model, in-plume NO2 volume mixing ratios can be derived from the MAX-DOAS measurements.

For validation, a comparison to airborne imaging DOAS measurements during the NOSE campaign in July 2013 is performed, showing good agreement between the approximate plume position derived from the onion-peeling MAX-DOAS and the airborne measurements as well as between the derived in-plume NO2 volume mixing ratios (VMRs).

1 Introduction
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Over the last decades, there has been a strong increase in ship traffic and shipping emissions of gas-phase pollutants but a reduction in their land sources in much of Europe. This has lead to an increasing contribution of shipping emissions to air pollution in coastal regions. Consequently, emission reduction measures have been enacted by the International Maritime Organization (IMO) in the International Convention for the Prevention of Pollution from Ships (MARPOL 73/78 Annex VI) globally as well as, more stringently, locally in so-called emission control areas (ECAs) like the North and Baltic seas (IMO2009). To reduce sulfur oxide (SOx) emissions, at the time of this study, the allowed sulfur content in shipping fuel is limited to 0.1 % in ECAs (since 2015, before it was 1.0 %) and to 3.5 % globally, which is planned to be reduced to 0.5 % by 2020. For NOx, the allowed emission rate depends on the rated rotational speed of the engine crankshaft (engine power and fuel efficiency) and is implemented in three tiers: Tier I (globally) for ships built between 2000 and 2010, Tier II (globally) for ships built from 2011 onwards, and Tier III (locally in ECAs) for ships built from 2016 onwards, with the last one not yet implemented in the North and Baltic seas, shifted to 2021 (IMO2017). In order to monitor the effectiveness of these measures as well as the overall impact of ship emissions on air quality, measurements of air pollution from ships are required.

Most measurements of air pollution are performed with in situ instrumentation, and this includes monitoring of the effect of ship emissions, which is usually performed with either land-based or shipborne in situ measurements. As shown in , multi-axis differential optical absorption spectroscopy (MAX-DOAS) measurements can provide both a complementary approach and an alternative to in situ trace gas measurements at sites, where the ships are several kilometers away from the instrument and interpretation of in situ measurements is challenging due to dilution and broadening of the plume during the travel time from the ships to the measurement site.

MAX-DOAS measurements pointing at the horizon probe a long horizontal light path and are thus very sensitive to absorbers located close to the ground. The strong wavelength dependence of Rayleigh scattering ($\propto {\mathit{\lambda }}^{-\mathrm{4}}$) leads to longer effective horizontal light paths for longer wavelengths. Simultaneous measurements and DOAS retrievals in the UV and visible spectral ranges can thus be used to probe different parts of the horizontal light path, an approach which is often called an “onion-peeling” method and has been applied to MAX-DOAS measurements before; used this method to retrieve two-dimensional NO2 fields from circular azimuth scans around the instrument in the framework of the MAD-CAT campaign (Multi-Axis DOAS Comparison campaign for Aerosols and Trace gases) in Mainz, Germany. The aim of the study was the investigation of horizontal gradients in a strongly polluted urban area, with the cities of Mainz, Wiesbaden, and Frankfurt as well as the Frankfurt airport close by, focusing on comparison to satellite measurements.

The present study focuses on measurements in a relatively clean coastal region where ships passing by the island are often the only dominant source of air pollution . The ships are mobile point sources of NOx emissions and the emitted exhaust gas plumes are transported, depending on wind conditions, leading to a strongly inhomogeneous NO2 field over the shipping lane.

probed a circular area with 14 azimuthal viewing directions distributed over a 360 view around the instrument. In the present study, a similar measurement pattern was applied using five different azimuth directions distributed over a 120 angle to cover the shipping lane close to the island (see Fig. 1b) with sufficient time resolution to monitor individual passing ships. The onion-peeling approach provides additional distance information for the measured NO2 columns.

Figure 1(a) Ship traffic density map calculated from all received AIS messages (2013–2016) showing the main shipping lane from the North Sea into the Elbe river close to the measurement site on a radar tower on the island Neuwerk (red dot). Wind measurements are available on Neuwerk as well as the neighboring island Scharhörn (green dots). (b) Effective horizontal light paths in UV (purple line) and visible spectral ranges (green line) for the five azimuthal viewing directions of the MAX-DOAS instrument (310, 335, 5, 35, 65, with respect to north), shown for typical light path lengths of 9 km (UV) and 13 km (vis), respectively. The difference between both paths, ΔL, is highlighted by the orange line.

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This study uses measurements in both the UV (∼350 nm) and blue spectral ranges (∼450 nm), while used additional measurements in the yellow spectral range (∼570 nm) to get an even longer effective horizontal light path and cover a larger region. This is not possible here as the instrument used has a smaller wavelength coverage.

As can be seen from Fig. 1a and b, the measurement site on the island Neuwerk is ideal for applying this measurement principle: the distance between site and shipping lane is of the order of 6 to 10 km, depending on the azimuthal viewing direction, which is in the range of typical UV horizontal effective light path lengths . Depending on the azimuthal direction, the additional probing distance gained by measurements in the visible spectral range covers the shipping lane or the region to the north of the ship track. As is shown in the following, this enables the NO2 distribution caused by the ship emission plumes over and around the ship track to be determined. In addition even the distance and course of the emitted plumes is observed.

This publication is a follow up to an earlier study entitled “Monitoring shipping emissions in the German Bight using MAX-DOAS measurements” , where long-term measurements were used to assess the impact of shipping emissions on the regional air quality, while the present study focuses on describing, demonstrating, and validating a new method for improved measurements of ship emissions and their localization.

The present study is part of the project MESMART (Measurements of Shipping Emissions in the Marine Troposphere), a cooperation between the University of Bremen (Institute of Environmental Physics, IUP) and the German Federal Maritime and Hydrographic Agency (Bundesamt für Seeschifffahrt und Hydrographie, BSH), supported by the Helmholtz Zentrum Geesthacht. For further information visit http://www.mesmart.de/ (last access: 7 October 2019).

2 Measurement site and instrumentation
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## 2.1 MAX-DOAS instrument

Multi-axis differential optical absorption spectroscopy (MAX-DOAS) is a well-established technique for measurements of trace gases that absorb in the UV and visible spectral ranges. This passive remote sensing method measures spectra of scattered sunlight in multiple viewing directions and is highly sensitive to absorbers in the atmospheric boundary layer. A two-channel MAX-DOAS instrument was deployed on the island Neuwerk from July 2013 to July 2016. It comprises a telescope unit with a field of view of 1 on a pan-tilt head, an optical fiber cable, and two spectrometers with charge-coupled device (CCD) cameras for UV (304.6–371.7 nm) and visible (398.8–536.7 nm) spectral ranges. This arrangement is optimized for the simultaneous retrieval of NO2 and O4 in both spectral domains. The total exposure time (or integration time) per measurement is 10 s for off-axis measurements and 20 s for zenith sky reference measurements. A new azimuthal measurement in one of the five different directions (see Sect. 2.2 and Fig. 1) starts about every 30 s. The measurement sequence is intermitted by a vertical scan in the main direction (335 azimuth) and a zenith sky measurement, both together taking in total around 90 s. The temporal resolution for one viewing direction, i.e., the time until the same azimuthal direction is probed again, is around 4 min.

A detailed description of the MAX-DOAS instrument and its components as well as the general measurement geometry for ship emission measurements is given in . Details of the DOAS fit settings used are summarized in Table 1.

Table 1DOAS fit settings for the retrieval of NO2 and O4 in UV and visible spectral ranges.

* Interpolation in time between the zenith measurements directly before and after the off-axis scan.

## 2.2 Measurement site

Neuwerk is a small island in the German Bight, northwest of the city of Cuxhaven at the mouth of the river Elbe, around 9 km off the coast. An overview of the area is shown in Fig. 1a. The main shipping lane into the river Elbe towards the port of Hamburg passes the island in the north at a distance of 6–7 km (see Fig. 1a). The MAX-DOAS instrument was installed on a radar tower at a height of 30 m above ground level (a.g.l.). Additional instrumentation on-site included in situ gas analyzers (NOx, SO2, O3, CO2) in a combined compact housing (Airpointer from MLU recordum, Austria), a Davis Vantage Pro2 semiprofessional weather station and an automatic identification system (AIS, ) receiver. The AIS signal broadcasts different information like identification, position, speed, course, and size of the ship. Broadcasting equipment is mandatory for all ships larger than 20 m. In the present study, the AIS information is used to attribute the measurements to individual ships. Wind direction and speed are available with a time resolution of 10 min from two stations (see Fig. 1a), one on Neuwerk and one on the neighboring island Scharhörn, operated by the Hamburg Port Authority (HPA).

To sample a larger region, the MAX-DOAS instrument was set up to have five different azimuthal viewing directions: 310, 335, 5, 35, and 65 with respect to north, each pointing towards different sections of the shipping lane (see Fig. 1b).

For further information on the measurement site and instrumentation see .

3 Methodology
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The quantity retrieved from DOAS measurements is the so-called slant column density (SCD), the integrated concentration of an absorber along the atmospheric light path. To measure the NO2 absorption inside the ship plumes emitted on the shipping lane, the instrument points in 0.5 elevation towards the horizon. Taking a close-in-time zenith sky measurement as a reference, in a first assumption only the absorption along the horizontal part of the effective light path is retrieved and the absorption higher up in the atmosphere cancels out. This yields the differential slant column density (DSCD).

For the comparison with in situ measurements the MAX-DOAS horizontal trace gas columns are converted to horizontal path-averaged volume mixing ratios (VMRs) by using the O4 scaling approach (see Sect. 3.1). The onion-peeling approach (see Sect. 3.2) is used to separate NO2 absorptions at different horizontal distances to derive separate NO2 VMRs and estimate the distance to the plumes.

## 3.1O4 scaling approach – methodology and limitations

The oxygen collision complex O4 absorbs in similar wavelength ranges as NO2 in the UV and visible ranges. Since the near-surface concentration of O4 is known, the effective horizontal path length can be calculated by dividing the DSCD of O4 by its number density ${n}_{{\mathrm{O}}_{\mathrm{4}}}$:

$\begin{array}{}\text{(1)}& L=\frac{{\text{SCD}}_{{\mathrm{O}}_{\mathrm{4}},\phantom{\rule{0.125em}{0ex}}\mathrm{horiz}}-{\text{SCD}}_{{\mathrm{O}}_{\mathrm{4}},\phantom{\rule{0.125em}{0ex}}\mathrm{zenith}}}{{n}_{{\mathrm{O}}_{\mathrm{4}}}}=\frac{{\text{DSCD}}_{{\mathrm{O}}_{\mathrm{4}}}}{{n}_{{\mathrm{O}}_{\mathrm{4}}}},\end{array}$

with ${n}_{{\mathrm{O}}_{\mathrm{4}}}={\left({n}_{{\mathrm{O}}_{\mathrm{2}}}\right)}^{\mathrm{2}}$, which can be calculated from the measured temperature and pressure. This can be done independently for both UV and visible measurements, giving average light path lengths of ${L}_{\mathrm{UV}}=\left(\mathrm{9.3}±\mathrm{2.3}\right)$ km and ${L}_{\mathrm{vis}}=\left(\mathrm{12.9}±\mathrm{4.5}\right)$ km (mean ± standard deviation) for the 3 years of measurements on Neuwerk, depending on the observational conditions. Under clear-sky conditions, typical light path lengths are 10 km in the UV and 15 km in the visible spectral range .

Knowing the horizontal light path length L, the NO2 DSCD can be divided by L to obtain the average concentration (number density) of NO2 along the horizontal light path. Dividing the NO2 concentration by the concentration of air, nair, which can be calculated via the ideal gas law from the measured temperature and pressure, yields the average volume mixing ratio (VMR) along L:

$\begin{array}{}\text{(2)}& {\mathrm{\text{VMR}}}_{{\mathrm{NO}}_{\mathrm{2}}}=\frac{{\text{SCD}}_{{\mathrm{NO}}_{\mathrm{2}},\phantom{\rule{0.125em}{0ex}}\mathrm{horiz}}-{\text{SCD}}_{{\mathrm{NO}}_{\mathrm{2}},\phantom{\rule{0.125em}{0ex}}\mathrm{zenith}}}{L\cdot {n}_{\mathrm{air}}}=\frac{{\text{DSCD}}_{{\mathrm{NO}}_{\mathrm{2}}}}{L\cdot {n}_{\mathrm{air}}}.\end{array}$

This O4 scaling approach has been successfully applied to MAX-DOAS measurements before, for example in urban polluted areas or at high mountain sites .

For a homogeneous, well-mixed NO2 field along the light path, this VMR must agree with in situ measurement from the same altitude. For the ship emission case, where emission plumes fill only a small fraction of the several-kilometer-long light path, the path-averaged MAX-DOAS VMR will not represent the VMR inside the plume and values will be smaller than in situ measurements inside the plume .

In addition, the different shapes of the atmospheric profiles of NO2 (emitted and formed close to the surface) and O4 (exponentially decreasing with altitude) introduce systematic errors as has been shown by and . To account for this, correction factors calculated by radiative transfer simulations are needed. These depend on well-known quantities such as solar zenith angle (SZA) and relative solar azimuth angle (RSAA) as well as on unknown quantities such as aerosol optical density (AOD), height of the NO2 box profile, and the extent and vertical position of the aerosol layer relative to the NO2 profile , which are not measured and cannot be easily approximated for the present study. In previous studies, it has been assumed that NO2 is well mixed within a layer from the surface up to a top layer height and absent above this altitude. This is not a valid assumption in the case of horizontally inhomogeneous NO2 fields such as those probed over the shipping lane. As in , scaling factors are therefore not considered here, presumably leading to a systematic overestimation of path lengths and thus underestimation of MAX-DOAS VMRs .

Clouds can decrease or increase the light path length (and O4 absorption) by multiple scattering, depending on the cloud's position and its optical properties, especially its optical thickness . As a result, a day with scattered or broken clouds will show much more variation in path lengths than a clear-sky day, even between consecutive measurements, by having clouds in off-axis or reference measurements, both, or neither, which makes interpretation of results more difficult. In the following, only clear-sky days or measurements under cloud free conditions are considered.

Figure 2Plume–light path geometry and the resulting path-averaged NO2 concentrations for three possible cases: when the plume is close to the instrument and completely covered by the UV path (a), when the plume is further away from the instrument than the UV scattering point and is only covered by the visible path (and ΔL(b), and when the plume is located around the UV scattering point (c).

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## 3.2 Onion-peeling MAX-DOAS approach

As mentioned above, the wavelength dependence of Rayleigh scattering results in a wavelength dependence of the light path lengths after the last scattering point. This can be utilized to probe different air masses in the atmosphere by measuring both in the UV and visible spectral ranges.

The aforementioned O4 scaling method gives two path-averaged volume mixing ratios for each measurement: one for the shorter UV range and one for the longer visible effective horizontal light path, which are shown in Figs. 1b and 2 as purple and green lines, respectively. One can calculate a third volume mixing ratio from the difference of the two DSCDs and path lengths:

$\begin{array}{}\text{(3)}& {\text{VMR}}_{\mathrm{@}\mathrm{\Delta }\phantom{\rule{0.125em}{0ex}}L}=\frac{{\text{DSCD}}_{\mathrm{vis}}-{\text{DSCD}}_{\mathrm{UV}}}{\left({L}_{\mathrm{vis}}-{L}_{\mathrm{UV}}\right)\cdot {n}_{\mathrm{air}}}=\frac{\mathrm{\Delta }\text{DSCD}}{\mathrm{\Delta }L\cdot {n}_{\mathrm{air}}}.\end{array}$

This yields the average volume mixing ratio VMR@Δ L along the path difference ΔL, which is shown as an orange line in Figs. 1b and 2.

As each ship is a moving point source for NO2 emissions, the NO2 field over a shipping lane is strongly inhomogeneous. This means that the NO2 is in general not distributed evenly along any of the effective horizontal light paths.

Depending on the position of the plume in relation to the UV and visible light path, the path-averaged mixing ratios can differ substantially. Figure 2 shows schematically the plume–light path geometry for three possible observation scenarios and illustrates the expected NO2 signal for the different horizontal light paths.

In case (a) the plume is close to the instrument and is completely covered by the shorter UV path LUV; i.e., it is closer to the instrument than the (mean) last scattering point in the UV. Although both paths cover the same amount of NO2, the retrieved path-averaged concentration is higher for the UV signal because of the higher relative contribution of the fraction of the light path which probes the NO2 plume. The path difference ΔL incorporates no NO2 from the emission plume, resulting in zero or background level NO2 measured along this path segment. It can be seen from Fig. 1b that this situation occurs for northerly wind directions. Section 4.2 shows example measurement results for such a case.

Case (b) shows the opposite situation, when the plume is further away from the instrument than the UV scattering point and only covered by the visible path Lvis. This results in an enhanced signal for the NO2 retrieved in the visible range and no signal in the UV range. The path-averaged concentration retrieved for ΔL is even higher because ΔL is only a segment of the visible path and therefore shorter than the complete visible path. On Neuwerk, such a situation can occur for southerly winds (compare Fig. 1b). Section 4.3 shows example measurement results for this kind of situation.

In case (c) the plume is close to the UV scattering point. All three light paths see enhanced NO2. The relative peak heights depend on the fraction of plume NO2 probed by the different light paths as well as the total light path lengths. On Neuwerk, situations like this will most likely occur for westerly and easterly winds.

As already discussed in , the measured column density as well as the path-averaged concentration do not only depend on the emitted amount of NO2 inside the plume, but also on the angle of intersection between plume and line of sight of the instrument. The smallest absorptions, and thus column amounts, will be retrieved if the plume runs orthogonally to the line of sight, and the highest values if the instrument measures along the plume. The latter can occur for certain combinations of wind direction and speed and ship movement direction and speed. But as the movement of the ship together with the measured wind can result in an apparent wind direction very different from the measured wind direction , a measurement along the measured wind direction (windward, i.e., pointing antiparallel to the wind vector) does not in general correspond to measurements along the plume.

The time span between plume emission and measurement is important for the measured NO2 values because of NO-to-NO2 titration in the plume ($\mathrm{NO}+{\mathrm{O}}_{\mathrm{3}}\to {\mathrm{NO}}_{\mathrm{2}}+{\mathrm{O}}_{\mathrm{2}}$), as a large fraction of nitrogen oxides (NOx) are emitted as NO , which does not absorb in the spectral range covered and cannot be measured with MAX-DOAS. Therefore, the NO2 content in the plume is expected to increase with distance from the ship until a steady state is reached. modeled the NO-to-NO2 conversion in plumes at short ranges depending on the O3 concentration. For O3 VMRs of 30 to 50 ppb (20 to 70 ppb), which are typically measured at our Neuwerk station in summer, they predicted the steady state to be reached after 3 to 4 min and in the steady state the fraction of NO2 of the overall NOx to be 65 %–70 %. For very fresh plumes shortly after emission, found that the NO2-to-NOx ratio in the plume does not depend on ambient ozone concentrations, as diffusion limits the availability of O3. Airborne imaging DOAS measurements during an overflight over a ship and its plume from the NOSE campaign on 21 August 2013 presented by show an increase in NO2 with flown distance from the ship overpass. After the airplane covered a distance of around 3 km the values stabilize and do not increase further. Applying the plume modeling approach discussed in Sect. 3.3, the plume age at this point where presumably the steady state was reached was estimated to be around 6.5 min, in which the respective plume air parcel traveled a distance of ∼1.5 km. Other, unpublished in situ measurements of ship plumes indicate that after 8–10 min at the latest the plume NO content is below 20 %–30 % for all ships. In view of these findings, as the plumes investigated in our study are mostly older than 10 min, we expect and assume the steady state to be already reached.

The lifetime of NO2 is on the order of several hours, but as the timescales investigated here are shorter, we expect the influence to be small.

## 3.3 Plume trajectories and plume modeling

For a more quantitative treatment of the ship emissions, the exhaust plumes and their movement over time need to be considered. Here, ship plume trajectories have been calculated as simple forward trajectories combined with a Gaussian plume model. On a 10 s time grid, at each time step, each point-shaped plume air parcel is moved from its old position to a new position, which depends on wind direction and speed. Each ship emits a new plume air parcel per time step at the respective ship position, thus creating a chain-line-like string of plume air parcels. By starting with an initialization period of 3 h before the respective measurement time, old plumes from ships that passed by the island before and already left the region of interest can be included in maps as those shown in Fig. 4.

Table 2Atmospheric stability classification scheme based on surface wind speed and solar insolation: A – very unstable; B – moderately unstable; C – slightly unstable; D – neutral. The additional stability classes E for slightly stable and F for stable occur only at night. For A–B take the average of stability parameters (Table 3) for A and B.

Plume broadening and dispersion over time is accounted for by modeling the width and height of the plumes with a Gaussian plume model , an often used model for point source emitters like power plants. It describes the vertical and horizontal plume dispersion with two Gaussian curves and links the pollutant emission rate Q, the mean wind speed U (in x direction), and the horizontal and vertical dispersion coefficients σy and σz to the concentration C at the point (x, y, z):

$\begin{array}{}\text{(4)}& C\left(x,y,z\right)=\frac{Q}{\mathrm{2}\mathit{\pi }\phantom{\rule{0.125em}{0ex}}U\phantom{\rule{0.125em}{0ex}}{\mathit{\sigma }}_{y}\phantom{\rule{0.125em}{0ex}}{\mathit{\sigma }}_{z}}\phantom{\rule{0.125em}{0ex}}\mathrm{exp}\left(\frac{-{y}^{\mathrm{2}}}{\mathrm{2}\phantom{\rule{0.125em}{0ex}}{\mathit{\sigma }}_{y}^{\mathrm{2}}}\right)\phantom{\rule{0.125em}{0ex}}\mathrm{exp}\left(\frac{-\left(z-H{\right)}^{\mathrm{2}}}{\mathrm{2}\phantom{\rule{0.125em}{0ex}}{\mathit{\sigma }}_{z}^{\mathrm{2}}}\right),\end{array}$

where the vertical coordinate z is corrected for the effective stack height H (the effective height of the plume center line), the sum of the stack height, and the initial plume rise.

The dispersion coefficients σy and σz are the standard deviations of the Gaussian shaping functions and depend on atmospheric stability. A simple classification scheme defining six different stability classes ranging from very unstable (A) to stable (F) based on wind speed and solar insolation (Pasquill1961) is shown in Table 2. One set of empirical functions for the dispersion coefficients σy and σz as functions of the along-wind distance x is given by :

$\begin{array}{}\text{(5)}& {\mathit{\sigma }}_{y}\left(x\right)=a\cdot {x}^{\mathrm{0.894}}\end{array}$

and

$\begin{array}{}\text{(6)}& {\mathit{\sigma }}_{z}\left(x\right)=c\cdot {x}^{d}+f,\end{array}$

where the distance from the source x is input in kilometers to retrieve σ in meters. The stability-dependent empirical constants a, c, d, and f are given in Table 3, partially with a distinction between x≤1 km and x>1 km (Martin1976).

Table 3Empirical stability parameters for the computation of the horizontal and vertical dispersion coefficients σy, σz (Martin1976) for the different atmospheric stability classes according to . For intermediate stability classes like A–B, averages of parameter values for A and B are taken.

As the ships are moving point sources, the course of the plume does not only depend on the wind direction but also on the previous pathway of the ship. The ships move with a certain direction and speed, thus creating an apparent wind . It is therefore not sufficient to run the Gaussian plume model for each ship position on each time step, it has to be combined with the simple forward trajectories, as each plume air parcel has been emitted at a different location. This is done by running the Gaussian plume model for the respective stability class that fits the prevailing weather conditions and creating look-up tables (LUTs) for the plume width and height depending on the distance from the emission point. For each plume air parcel in the trajectory this LUT is then evaluated at the distance this plume parcel traveled since its emission, to retrieve the plume width at this location. The plume width and height LUTs are gained from the Gaussian plume model by going through every x distance in 10 m steps (a 10 m×10 m grid is used) and checking in the across-wind direction at which distance from the plume centerline the concentration drops under a certain threshold level (in this study: 1∕e) compared to the maximum concentration at the plume centerline at this respective x distance. By introducing this kind of normalization, the exact values of the multiplicative factors Q (emission rate) and U (wind speed) become irrelevant for the computation. For the plume width this LUT can be applied to all ships, but for the plume height, as this depends on the stack height, the LUTs have to be computed for each individual ship separately, as their stack heights differ. As neither ship height nor stack height is contained in the broadcasted AIS data, the stack height has to be researched for each ship individually. In this study it was estimated from pictures of a ship by comparing the stack height to the standardized height of the loaded containers. This is not so much of a problem here, as the plume height plays no role in the visual representation of the plumes in the maps (as they represent an aerial view) but only for the detailed analysis of specific plumes of specific ships.

For the method for deriving in plume NO2 VMRs from MAX-DOAS (and airborne imaging DOAS) measurements described in Sect. 4.4, knowledge of the plume width (and height) is sufficient, so the concentration or emission rate is not modeled here. Plume chemistry like NO-to-NO2 titration and NO2 loss reactions and NO2 lifetime is neglected. Another source of uncertainty is the fact that the Gaussian plume model only describes an average plume. Each snapshot in time of a real plume will in general not look like a Gaussian plume, but if multiple snapshots are averaged over a certain time period, the average shape should approach a Gaussian plume shape. Using the Gaussian plume model for the plume trajectories is therefore only an approximation.

4 Results
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## 4.1 Onion-peeling approach applied to ship emission measurements

Figure 3a shows the measured NO2 DSCDs in 0.5 elevation for the 335 azimuth direction (compare Fig. 1b) on 26 May 2014. The NO2 shows sharp peaks, which originate from shipping emissions, with rapid changes of NO2 levels between consecutive measurements of up to 1 order of magnitude. The small, but nonzero baseline between the peaks shows an ambient NO2 pollution, which is enhanced in the morning hours. The background NO2 signal may originate from land-based sources but may also contain residual, diluted shipping emissions. The morning enhancement might be due to the morning traffic rush hour or boundary layer height changes.

As a result of the longer light path, the NO2 columns measured in the visible range are larger than in the UV range. The difference between visible and UV columns, ΔDSCD, shows concurrent peaks for some of the cases, with varying relative height. The peak at 12:50 UTC is not visible in the ΔDSCD, indicating that the plume must be closer to the instrument than the UV scattering point.

Figure 3Differential slant column densities of NO2 (a), horizontal effective path lengths (b), and horizontal path-averaged volume mixing ratios of NO2 on 26 May 2014 in 0.5 elevation and 335 azimuth for the UV (purple) and visible spectral ranges (green) and their difference (orange) (c).

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Figure 3b shows the corresponding effective horizontal light path lengths derived from the measured O4 DSCDs. For a clear-sky day like this, path lengths are quite constant over time.

Figure 3c shows the horizontal path-averaged NO2 volume mixing ratios retrieved from the NO2 DSCDs by using the O4 scaling approach with the path lengths for UV and visible ranges shown in Fig. 3b, as well as the volume mixing ratio on the path difference calculated via Eq. (3). The baselines of all three curves agree very well, showing that the ambient NO2 background pollution is well mixed in the boundary layer and homogeneously distributed along all light path sections. However, the sharp peaks originating from ship emission plumes have different relative heights, showing that the corresponding NO2 field is inhomogeneous. The strong NO2 signal at 12:50 UTC without enhanced NO2 VMR on the path difference, resembling situation (a) in Fig. 2, will be further investigated in the next section.

## 4.2 Northerly wind situations

For northerly winds, the pollution plumes emitted from the ships are blown towards the radar tower, resulting in enhanced NO2 concentrations south of the shipping lane (compare Fig. 1b). To the north of the shipping lane, concentrations should be low, resembling situation (a) in Fig. 2.

In Fig. 4, a 12 min sequence of consecutive MAX-DOAS measurements on 26 May 2014 starting at 12:46 UTC (14:46 LT) is shown for more detailed investigation of the strong NO2 signal already seen in Fig. 3c at 12:50 UTC. Plotted in each map are the length and location of the UV path and ΔL as colored lines, with color representing the respective path-averaged NO2 VMR. In situ NO2 VMRs are shown as colored dots at the measurement site. Also shown are ship positions and course from AIS data, plume trajectories (see Sect. 3.3), and wind speed and direction measured by the weather station on Neuwerk.

Figure 4Sequence of maps showing 15 consecutive measurements in 0.5 elevation on 26 May 2014, starting at 12:46 UTC (14:46 LT): the extent of the UV path and ΔL and corresponding path-averaged NO2 VMRs are shown as colored lines. In situ NO2 VMRs are shown as a colored dot at the location of the measurement site. Magenta triangles show the ship position and course (sharp tip), with larger triangles for larger ships. The modeled plumes are shown in gray, with the lightness of the gray shading representing the plume age. Wind direction and speed are shown with meteorological wind barbs.

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The sequence of maps shows two ships (magenta triangles) on the shipping lane, moving in opposite directions. The larger ship (length 351 m) moves westward, and the smaller ship (length 151 m) moves eastward. The locations of the two plumes (gray shaded stripes) differ considerably due to the different movement directions of the ships and the curved shape of the shipping lane around the island.

For the plume modeling, the stability class C representing slightly unstable conditions has been chosen based on the wind speed and the strong solar insolation on this clear-sky day.

In Fig. 4, panel 1, the MAX-DOAS measurements at 12:46:24 UTC in the 335 azimuth direction are shown. The horizontal path-averaged NO2 VMRs are low (<1 ppb NO2) and agree very well between the different path segments as well as with the in situ measurements, showing that the ambient background NO2 is homogeneously well mixed in the boundary layer. The fact that the plume from the smaller ship shows up only slightly in the measurements might be due to low emissions from this comparatively small ship and the dilution of the already strongly dispersed plume, as the plume model predicts a vertical extent of the plume of ∼400 m and a plume width of 1200–1300 m at a plume age of 700–800 s.

Figure 4, panels 2 to 4 (5, 35, and 65 azimuth, respectively) show enhanced NO2 VMRs (up to 4 ppb) along the UV path close to the instrument, likely due to the plume of the big ship and low VMRs along ΔL further away from the instrument. Although MAX-DOAS measurements show enhanced NO2 between the site and UV scattering point, the plume has not reached the radar tower yet and in situ values therefore stay low.

Figure 4, panel 5 shows the measurements in the 310 viewing direction, which are similar to the measurements in 335 azimuth angle in panel 1.

In Fig. 4, panels 6 to 10, the plume approaches the radar tower and in situ values begin to rise. MAX-DOAS VMRs are again high close to the radar tower and low in the north of the shipping lane. Due to different angles of intersection between the plume and line of sight, the MAX-DOAS path-averaged UV VMR is different, showing the highest value of  5 ppb when measuring alongside the plume (panel 6) and much lower values when measuring orthogonally to it (e.g., panel 3). A small NO2 enhancement of 4×1015 molec. cm−2 is seen in the zenith sky measurements around 12:50 UTC, which is gone at 12:55 UTC, indicating that at least part of the plume was located above the MAX-DOAS instrument. As the zenith sky measurements are used as a sequential reference for the off-axis measurements, this causes a small canceling effect when using the sequential reference. As off-axis DSCDs are on the order of 1×1017 molec. cm−2 reaching up to 1.4×1017 molec. cm−2 as can be seen from Fig. 3, the overall impact on the path-averaged VMRs is very small, on the order of 2 % to 4 %.

Starting with Fig. 4, panel 9 the in situ instrument measures even higher values, which are not represented in the figure as the color scale extending up to 5 ppb is saturated. Reaching 6.1 ppb in panel 9, the measured NO2 VMR increases further until panels 10 and 11, where it peaks at 8.3 and 8.9 ppb, respectively. In panel 12 the measured NO2 VMR has dropped to 6.3 ppb but afterwards increases again due to the second plume, reaching 6.6, 6.8, and 7.1 ppb in panels 13 to 15. After panel 15, the value increases further to 8.8 ppb and goes down again to ambient background concentrations. This means that the in situ instrument measured two overlapping plumes. The maximum in situ NO2 VMRs are much higher compared to the MAX-DOAS measurements because the in situ instrument directly measures the NO2 VMR inside the plume and the MAX-DOAS instrument delivers path-averaged values, which underestimate the local VMR inside the plume. The fact that the plume overpass is seen earlier in the MAX-DOAS zenith sky measurements than in the in situ measurements indicates that wind speeds are higher at higher altitudes, so that the upper part of the plume crossed the radar tower earlier than the lower part.

In Fig. 4, panel 11 the ship plume has moved out of the narrow line of sight of the MAX-DOAS instrument and measured NO2 values drop rapidly to ambient concentrations on both path segments. Panels 11 to 14 show all low MAX-DOAS measurements, while the plumes of both ships hit the radar tower, leading to a very high in situ signal.

In Panel 15 the larger ship has moved further away from the instrument, leading for the first time in this sequence to a higher concentration along ΔL, far away from the instrument, than close by. Comparing the locations of the MAX-DOAS paths with the ship position and modeled plume in detail, however, indicates a much larger intersect of the plume with the UV path than with ΔL. This might be an example showing the uncertainty (overestimation) in the path length estimation due to negligence of the correction factor as discussed in Sect. 3.1.

Figure 5 shows again, but in more detail, the measurements of the ship and plume positions from panel 10. To highlight the entire retrieved two-dimensional NO2 field in the measurement region along the shipping lane, the four previous MAX-DOAS measurements are shown as well, which were measured between 30 s and 3 min before. The strong horizontal gradient between enhanced NO2 concentrations close to the site and low concentrations further away for such a north wind situation is clearly visible in the figure.

Figure 5Map showing a zoom in onto panel 10 of Fig. 4 and the four previous MAX-DOAS observations, which have been measured between 30 s and 3 min before the current observation. Horizontal light path lengths (UV path and ΔL) and corresponding path-averaged volume mixing ratios of NO2 are shown as colored lines and the in situ NO2 VMR as a colored dot at the location of the instrument. Magenta triangles show the ship position and course, with larger triangles for larger ships. The modeled plumes are shown in gray, with the lightness of the gray shading representing the plume age. Please keep in mind that ship and plume position were different for the past measurements. Wind direction and speed are shown with a meteorological wind barb.

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## 4.3 Southerly wind situations

The second selected case study shows a diametrically opposite situation: for southerly winds the emitted pollution plumes are blown to the north of the shipping lane (compare Fig. 1b), further away from the instruments. As a result, NO2 concentrations south of the shipping lane, close to the instruments, should be low, resembling situation (b) in Fig. 2. On-site in situ instruments are not able to measure the ship emission plumes.

Figure 6 shows a 12 min sequence of consecutive measurements on 13 August 2014 starting at 12:35 UTC (14:35 LT). It shows MAX-DOAS path-averaged NO2 VMRs as well as in situ measurements. Shown are also ship positions and course from AIS data, plume trajectories (see Sect. 3.3), and wind speed and direction measured by the weather station on Neuwerk.

Figure 6Sequence of maps showing 15 consecutive measurements in 0.5 elevation on 13 August 2014, starting at 12:35 UTC (14:35 LT). The extent of the UV path and ΔL and corresponding path-averaged NO2 VMRs are shown as colored lines. In situ NO2 VMRs are shown as a colored dot at the location of the measurement site. Magenta triangles show the ship position and course (sharp tip), with larger triangles for larger ships. The modeled plumes are shown in gray, with the lightness of the gray shading representing the plume age. Wind direction and speed are shown with meteorological wind barbs.

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In the map sequence, three ships can be seen in the shipping lane, two large ones (336 and 365 m) and a smaller one (100 m). As all ships move in the same, eastward, direction, the plume trajectories are almost parallel. Apart from the ship emission plumes, another plume crosses the area of interest, originating from the two directly adjacent coal-fired power plants in Wilhelmshaven, located at 53.57 N, 8.14 E, at a distance of about 50 km, southwest of the measurement site. Using the 10 m a.g.l. wind speed of (7.5±1.0) m s−1, the plume age is estimated to be around 110 min, and even shorter taking into account that wind speed increases with height.

For the plume modeling, the stability class C representing slightly unstable conditions has been selected based on the wind speed and the strong solar insolation on this clear-sky day.

Figure 6, panel 1 shows the MAX-DOAS measurement at 12:35:31 UTC in the 310 azimuth direction. The horizontal path-averaged NO2 VMR along the UV light path is low (∼0.6 ppb) and along ΔL slightly enhanced (∼1 ppb), meaning low NO2 close to the instrument and enhanced NO2 further away (than the UV scattering point). The source for the enhanced NO2 signal along ΔL could be either the small ship's plume or plumes from the more distant power plants.

The next measurement in Fig. 6, panel 2 at 335 azimuth gives similar results. In this viewing direction the plume of the small ship is not in the line of sight of the instrument, indicating that the plume originating from the power plants is the source of the slightly enhanced NO2 VMR along ΔL.

In Fig. 6, panel 3 (5 azimuth) the MAX-DOAS instrument is measuring towards the two adjacent plumes of the two large ships, one located close to the UV scattering point and the other one further away. NO2 VMR is high (∼2 ppb) behind the UV scattering point and medium high (∼1 ppb) closer to the instrument.

Panel 4 (35 azimuth) again shows high values far away from the instrument and medium high values close by.

In panel 5 (65 azimuth), only one of the two plumes is in the line of sight and is further away than the UV scattering point, leading to enhanced NO2 along ΔL and low (ambient) NO2 along the UV path.

Panels 6 and 7 are similar to panels 1 and 2, showing that the situation in these viewing directions has not changed 4 min later.

In panel 8, 4 min after panel 3, the plumes of the two big ships traveled a bit further northward, making the gradient between NO2 VMRs on UV path and ΔL even stronger.

Panels 10 to 12 are similar to panels 5 to 7.

In panels 13 to 15, the plumes of the two big ships are now clearly only probed by the visible light path giving enhanced NO2 concentrations along ΔL and low, ambient NO2 concentrations along the UV path.

In all 15 consecutive measurements shown in the map sequence the in situ instrument measured constantly low values. This indicates that for southerly winds it cannot detect ship emission plumes at this site. Measured NO2 VMRs agree very well with ambient NO2 VMRs from the MAX-DOAS instrument, retrieved south of the shipping lane along the UV path.

Figure 7 again shows in more detail the measurements of ship and plume positions from panel 15. To highlight the entire retrieved two-dimensional NO2 field in the measurement region along the shipping lane, the four previous MAX-DOAS measurements are shown as well, which have been measured between 30 s and 3.5 min before. This highlights the horizontal gradient between low NO2 concentrations close to the site and enhanced concentrations further away, northward of the shipping lane, demonstrating that with MAX-DOAS it is feasible to measure ship emission plumes under conditions unfavorable for in situ measurements.

Figure 7Map showing a zoom in onto panel 15 of Fig. 6 and also the four previous MAX-DOAS observations, which were measured between 30 s and 3.5 min before the current observation. Horizontal light path lengths and corresponding path-averaged volume mixing ratios of NO2 are shown as colored lines and the in situ NO2 VMR as a colored dot at the location of the instrument. Magenta triangles show the ship position and course, with larger triangles for larger ships. The modeled plumes are shown in gray, with the lightness of the gray shading representing the plume age. The broader plume in the eastern part of the map originates from the Wilhelmshaven power plants. Please keep in mind that ship and plume position were different for the past measurements. Wind direction and speed are shown with a meteorological wind barb.

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## 4.4 Computation of in-plume NO2 volume mixing ratios using plume modeling and validation with airborne imaging DOAS measurements

In addition to visualizing the two-dimensional NO2 field over the shipping lane, plume modeling allows us to retrieve in-plume NO2 VMRs from the MAX-DOAS measurements. For a demonstration of the method, a day was chosen on which simultaneous airborne imaging DOAS measurements were performed, which can be used to validate both the plume modeling and the MAX-DOAS in-plume NO2 VMRs.

### 4.4.1 Computation of in-plume NO2 VMRs

The O4 scaling and onion-peeling method yields NO2 VMRs, which are averaged along a certain effective horizontal light path. In the general case that the plume does not cover the entire path, the retrieved path-averaged VMR is lower than the in-plume VMR. Thus, to retrieve the in-plume VMR, the fraction of the path probing the plume and thus the plume width has to be known. An estimate for the plume width is provided by the combination of forward trajectory and Gaussian plume model implemented in this study.

Figure 8Map showing the MAX-DOAS path-averaged VMRs (colored lines) and AirMAP vertical columns of NO2 (broad image stripe beneath) on 21 August 2013 around 9:53 UTC (11:53 LT). As the plotted physical quantities are entirely different (VMRs and columns), color scale agreements are not expected (and completely random). Magenta triangles show current ship positions and course, and magenta numbers denote the ship length. The modeled plumes (for the MAX-DOAS measurement time) are shown in gray, with the lightness of the gray shading representing the plume age. The time difference between AirMAP and MAX-DOAS measurements is indicated in the map at specific parts of the flight track. Wind direction and speed are shown with a meteorological wind barb.

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Figure 8 shows MAX-DOAS path-averaged NO2 VMRs and modeled plumes on 21 August 2013 around 09:53 UTC (11:53 LT). Also shown are AirMAP vertical columns of NO2, which are used for validation in the second part of this section (see Sect. 4.4.2 for more details).

The Gaussian plume model was run for a stability class of B–C, which was selected due to the moderate insolation (cloudy in the morning, later clearing up) and wind speeds between 3 and 4 m s−1. For this intermediate stability class B–C, representing slightly to moderately unstable conditions, the mean of the parameter values for B and C from Table 3 is taken. Wind speed and direction are taken from the weather station on Scharhörn.

Along ΔL where one of the modeled plumes is located, MAX-DOAS measured enhanced NO2 compared to the ambient background NO2 measured along the UV path. This plume is from the 277 m ship that left the map region to the west. At the intersection of plume and MAX-DOAS line of sight, the plume air parcels had traveled a distance of (2180±30) m in (660±10) s since emission and the plume model yields a width of (720±20) m. The selection of the stability class clearly has a strong influence on the modeled plume width, as the more unstable class B yields (870±20) m and the more stable class C yields (580±20) m. This span of values gives a more realistic error estimate. The MAX-DOAS line of sight “hits” the plume at an angle of approximately 70, so the resulting effective plume width is (760±160) m.

For the computation of the MAX-DOAS average in-plume NO2 VMR, the partial horizontal column inside the plume has to be determined as only scaling the VMR would not account for the background signal. The three panels in Fig. 9 show the MAX-DOAS DSCDs of NO2 for the lowest five elevation angles measured in the UV and visible spectral ranges, as well as their differences, ΔDSCD.

Figure 9MAX-DOAS differential slant column densities of NO2 in the UV (a) and visible (b) spectral ranges as well as their difference ΔDSDC (c) for the five lowest elevation angles for the azimuthal viewing direction of 335. The vertical gray line indicates the AirMAP plume overpass time.

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At 09:53 UTC a ΔDSDC of 1.3×1016 molec. cm−2 is measured along a 2.4 km ΔL. The UV measurement of 3.0×1016 molec. cm−2 along a 7.7 km LUV can be used to estimate the background signal along ΔL. With the modeled plume width $b=\left(\mathrm{760}±\mathrm{160}\right)\phantom{\rule{0.125em}{0ex}}\mathrm{m}=\left(\mathrm{76}\phantom{\rule{0.125em}{0ex}}\mathrm{000}±\mathrm{16}\phantom{\rule{0.125em}{0ex}}\mathrm{000}\right)\phantom{\rule{0.125em}{0ex}}\mathrm{cm}$ this yields, for the column inside the plume,

$\begin{array}{rl}{\text{DSCD}}_{\mathrm{plume}}& =\mathrm{\Delta }\text{DSCD}-{\text{DSCD}}_{\mathrm{background}}\\ & =\mathrm{\Delta }\text{DSCD}-{\text{DSCD}}_{\mathrm{UV}}\cdot \frac{\mathrm{\Delta }L-b}{{L}_{\mathrm{UV}}}\\ & =\left(\mathrm{6.9}±\mathrm{3.1}\right)×{\mathrm{10}}^{\mathrm{15}}\phantom{\rule{0.125em}{0ex}}\mathrm{molec}.\phantom{\rule{0.125em}{0ex}}{\mathrm{cm}}^{-\mathrm{2}},\end{array}$

where the associated uncertainty has been computed with Gaussian error propagation from the uncertainties of the retrieved DSCDs (±10 %), path lengths (±20 %), and modeled plume width (see above) assuming independent random uncertainties in the individual variables.

The average VMR inside the plume is given by

$\begin{array}{rl}& {\text{VMR}}_{\mathrm{plume}}=\frac{{\text{DSCD}}_{\mathrm{plume}}}{b\cdot {n}_{\mathrm{air}}}=\left(\mathrm{3.6}±\mathrm{1.8}\right)×{\mathrm{10}}^{-\mathrm{9}}\\ & \phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}=\left(\mathrm{3.6}±\mathrm{1.8}\right)\phantom{\rule{0.125em}{0ex}}\mathrm{ppb},\end{array}$

where ${n}_{\mathrm{air}}=\mathrm{2.54}×{\mathrm{10}}^{\mathrm{19}}$ molec. cm−3 is the number density of air for the measured pressure of 1025.2 hPa and temperature of 19.2 C. The total uncertainty has again been computed with error propagation.

### 4.4.2 Validation

As already indicated above, a comparison to on-site in situ trace gas analyzers is well suited to validate the MAX-DOAS ambient NO2 background values, but fails for in-plume concentrations in many constellations. For unfavorable wind conditions, like southerly winds, the in situ instrument does not detect the plumes at all. The spatial resolution of satellite instruments is not sufficient to resolve individual ship plumes, even with the Sentinel 5 precursor satellite (3.5×7 km2; ).

Airborne imaging DOAS measurements, as have been performed in the region of interest during the NOSE (for German “Nord-Ost-See-Experiment” meaning “North and Baltic seas experiment”) campaign (Meier2018) on 21 August 2013, are the ideal method for validation of our results. Mapping of the MAX-DOAS line of sights, as has been performed during NOSE, allows us to compare the approximate plume position retrieved from the onion-peeling MAX-DOAS method and that from the plume modeling to the real plume position.

Delivering high-resolution NO2 maps of the plumes, the airborne measurements can be used to validate both the plume positions calculated with simple forward trajectories and the plume width retrieved from the Gaussian plume model. By incorporating plume height information from either plume modeling or the vertical elevation scans of the MAX-DOAS instrument, an average in-plume NO2 VMR can be computed from the airborne vertical column measurements and compared to the result from the MAX-DOAS instrument.

The Airborne imaging Differential Optical Absorption Spectroscopy instrument for Measurements of Atmospheric Pollution (AirMAP), installed on a Cessna research aircraft of the Freie Universität Berlin for the measurements, is a push-broom imaging DOAS instrument. Scattered sunlight from below the aircraft is collected by a wide-angle objective and coupled into a bundle of 35 sorted optical fibers. The image of the vertically stacked fibers is then dispersed by an imaging grating spectrometer and mapped onto a frame transfer CCD. The total field of view of around 52 leads to a ground swath width similar to the flight altitude. With this setup, 35 across-track pixels are measured simultaneously with an exposure time of 0.5 s, leading to a spatial resolution better than 50 m when the aircraft is flying at 1600 m altitude. For more detailed information on the instrument see and .

In the AirMAP data analysis, differential slant column densities of NO2 were retrieved in a fit window of 425–450 nm using the settings described in . For the retrieval of NO2 vertical column densities, air mass factors were calculated for an NO2 box profile assuming constant NO2 in the lowest 500 m, in an atmosphere without aerosols and for a constant surface reflectance of 0.05. This box profile height is an educated guess on an upper limit for the typical vertical plume extent for older ship plumes, which the plume modeling has proven to be in the right order of magnitude.

Figure 8, already mentioned in the previous subsection, shows, in addition to the MAX-DOAS path-averaged VMRs, the AirMAP vertical columns of NO2 for a ship plume measured on 21 August 2013 around 09:53 UTC (11:53 LT). At about that time, the aircraft flew along the MAX-DOAS 335 azimuth line of sight crossing the shipping lane and mapping multiple ship plumes. Enhanced NO2 is measured where the aircraft overpassed the plumes, revealing the location and horizontal extent of the plumes. The southernmost plume was also covered by the MAX-DOAS instrument's NO2 measurement in the visible spectral range. As a result, the path-averaged NO2 VMR along ΔL shows enhanced values compared to the ambient background NO2 measured along the UV path, indicating a plume somewhere along ΔL, which is validated by the airborne measurements. Along the UV path, AirMAP NO2 vertical column densities (VCDs) are significantly lower, confirming the assumption of ambient background pollution.

The time difference between both measurements of less than 20 s is very small, especially considering the integration time of the MAX-DOAS instrument of 10 s. The position of the plume (calculated with a forward trajectory) and the horizontal extent of the plume (computed with the Gaussian plume model) match the real plume positions measured by AirMAP very well. The plumes further north were measured by AirMAP around 1 min later, enough time for the wind to blow the plumes northward so that the positions do not fully coincide with the plume forward trajectories, which have been computed for the MAX-DOAS measurement time. Inspecting the AirMAP measurements in detail reveals that the real plumes are not as smooth as the modeled plumes and show some irregularities and random fluctuations caused by turbulence. This deviation is expected, as the Gaussian plume model used here assumes a steady state and describes a (long) time-averaged picture of a plume. Nevertheless, the modeled plume widths fit quite well. These results provide confidence in the modeled plume trajectories as well as in the onion-peeling approach to detect locally enhanced NO2 levels in the ΔL light path segment.

For the validation of the in-plume NO2 VMR by AirMAP, one has to consider the crucial differences in viewing geometries which are sketched in Fig. 10. The MAX-DOAS instrument measures (slightly slanted) horizontal transects of the plume and can scan the plume vertically by using different elevation angles. The AirMAP instrument, measuring in the nadir direction downward from the aircraft, observes vertical transects of the plume. The AirMAP measurements deliver vertical columns of NO2 between ground and aircraft, but no information about the vertical location of the NO2 inside the column. By assuming a box profile for the near-ground NO2 layer (the plume), one can derive mixing ratios from the vertical columns, but for this the vertical extent of the plume has to be known. This plume height h can either be taken from the plume modeling or can roughly be estimated from the MAX-DOAS vertical scan measurements if the distance to the plume is known, as it is from the airborne measurements.

Figure 10Sketch of the different measurement geometries of ground-based MAX-DOAS and airborne imaging DOAS instruments when measuring a ship plume. While the MAX-DOAS instrument scans the plume vertically, the AirMAP instrument measures in the nadir direction. Distances, heights, and sizes are not to scale.

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The Gaussian plume model delivers a height of (320±20) m reaching from the ground to this height at the respective distance from the emission point (see above) for the selected stability class B–C and for a stack height of 40 m estimated from pictures of the ship and an assumed initial plume rise of 10 m. Again, the selection of the stability class has an influence on the modeled plume height, with (420±20) m retrieved for the more unstable class B and (230±20) m for the more stable class C, with the span giving again an idea on the uncertainty introduced by the selection of the stability class.

For the estimation from the MAX-DOAS measurements, we need to reconsider Fig. 9, showing the MAX-DOAS DSCDs of NO2 for UV and visible spectral ranges as well as the ΔDSCD. The UV measurements in Fig. 9a show the typical elevation angle dependency for tropospheric absorbers, with the longest light paths and therefore highest DSCDs in the lowest elevation angles. When the instrument points further up (i.e., higher elevation angles), the light path length through the troposphere decreases, giving smaller DSCDs.

Comparing Fig. 9b, showing the visible measurements, to Fig. 9a, the values are in general larger due to the longer light path length for longer wavelengths but show a similar separation except for the “gap” between the low elevations (0.5, 1.5) and higher elevations (2.5, 3.5, 4.5). This implies that there is even more additional NO2 in the lower elevations than is expected from the longer light path effect. The gap is even more pronounced when inspecting the ΔDSCD shown in Fig. 9c. This excess NO2 most certainly originates from the ship emission plume. Assuming that the plume vertically fills the whole vertical field of view of the 0.5 and 1.5 elevation, an upper boundary for the plume height h can be calculated. The field of view of the instrument is around 1.0. Thus the plume is observed at a solid angle of 2.0 (compare Fig. 10). At a distance of 9.6 km (see below), this corresponds to a plume height of $h=\mathrm{9.6}\phantom{\rule{0.125em}{0ex}}\mathrm{km}\cdot \mathrm{tan}\mathrm{2}{}^{\circ }\approx \mathrm{335}$ m. This result is in good agreement with the plume modeling result of (320±90) m.

Figure 11AirMAP vertical columns of NO2 as a function of distance (lower axis) or time (upper axis) for the flight track section shown in Fig. 8. Panel (b) is a zoom in on the gray shaded area. Horizontal arrows denote the horizontal effective light paths.

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Figure 11a shows NO2 VCDs from AirMAP as a function of distance to the radar tower for the flight track section shown in Fig. 8. The 35 individual viewing directions were binned to 5 (1:7, 8:14, 15:21, 22:28, and 29:35) to reduce the noise. Although additional binning would reduce the noise even further, it would also smear out the plume signal since the flight track crosses the plume not orthogonally but at an angle of about 70 (see Fig. 8). A strong enhancement of NO2 is observed at a distance of about 9.1 to 10.1 km, as was expected from the MAX-DOAS NO2 enhancement along ΔL. Figure 11b shows the measurements of the plume in more detail, revealing the distance shift of the plume position in the different AirMAP viewing directions due to the slanted angle between flight direction and plume. The NO2 enhancement caused by the plume is roughly Gaussian-shaped in all five binned viewing directions, confirming that the Gaussian plume model gives a good approximation of the plume shape, although maximum values and peak widths differ due to the turbulent fluctuations.

The measured vertical columns are total columns between flight altitude and ground level. To retrieve the local enhancement of NO2 inside the plume, the estimated background column containing ambient NO2 is subtracted from the total NO2 column:

$\begin{array}{rl}& {\text{VC}}_{\mathrm{plume}}={\text{VC}}_{\mathrm{total}}-{\text{VC}}_{\mathrm{background}}\\ & \phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}=\left(\mathrm{7.0}±\mathrm{2.0}\right)×{\mathrm{10}}^{\mathrm{15}}\phantom{\rule{0.125em}{0ex}}\mathrm{molec}.\phantom{\rule{0.125em}{0ex}}{\mathrm{cm}}^{-\mathrm{2}}\\ & \phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}-\left(\mathrm{3.2}±\mathrm{1.0}\right)×{\mathrm{10}}^{\mathrm{15}}\phantom{\rule{0.125em}{0ex}}\mathrm{molec}.\phantom{\rule{0.125em}{0ex}}{\mathrm{cm}}^{-\mathrm{2}}\\ & \phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}\phantom{\rule{0.25em}{0ex}}=\left(\mathrm{3.8}±\mathrm{2.2}\right)×{\mathrm{10}}^{\mathrm{15}}\phantom{\rule{0.125em}{0ex}}\mathrm{molec}.\phantom{\rule{0.125em}{0ex}}{\mathrm{cm}}^{-\mathrm{2}}\end{array}.$

Possible error sources for the AirMAP measurements are fitting uncertainties on the retrieved DSCDs, uncertainties on the surface reflectance, the assumed profile shape, and aerosols, while uncertainties on the NO2 amount in the reference spectrum cancel out when subtracting the background, yielding a maximum overall uncertainty on the NO2 VCD of about 30 % .

The NO2 columns measured horizontally (MAX-DOAS) and vertically (AirMAP) through the plume are different. This is expected because the horizontal and vertical extent of the plume differ – the plume width being approximately 2 times larger than its height. For a quantitative comparison, the in-plume NO2 column density needs to be converted to an average in-plume VMR.

${\text{VMR}}_{\mathrm{plume}}=\frac{{\text{VC}}_{\mathrm{plume}}}{h\cdot {n}_{\mathrm{air}}},$

yielding (4.7±3.0) ppb for h=320 m (from plume model) or (4.5±2.7) ppb for h=335 m (from MAX-DOAS), where the overall uncertainty has been computed with error propagation.

This result is in reasonably good agreement with the average in-plume VMR of (3.6±1.8) ppb derived from the MAX-DOAS measurements combined with the Gaussian plume model. Having the AirMAP measurements for validation, the plume width computed by the plume model can be compared to the AirMAP measurements (Fig. 11). Using the same threshold as for the modeling, 1∕e, this gives a plume width b of 600–700 m, or an effective plume width of ${b}_{\mathrm{eff}}=\left(\mathrm{690}±\mathrm{53}\right)$ m due to the 70 angle between plume and flight direction. These values are in good agreement with the slightly higher values of $b=\left(\mathrm{720}±\mathrm{150}\right)$ and ${b}_{\mathrm{eff}}=\left(\mathrm{760}±\mathrm{160}\right)$ m, computed by the model, again confirming the validity of the Gaussian plume modeling approach for this study. Using the more accurate plume width estimate from the AirMAP measurements, the MAX-DOAS in-plume VMR changes to a value of (4.0±1.8) ppb giving an even better agreement with the AirMAP results. A thorough inspection of the AirMAP measurements along the UV path of the MAX-DOAS instrument (see Fig. 8) reveals that there is a slight decrease in ambient NO2 background pollution observed along the UV path from the radar tower towards the UV scattering point and towards the plume location. Estimating the background column along ΔL from the UV path, where the MAX-DOAS instrument delivers only one averaged value, thus might lead to a small bias in the background correction. If too much NO2 is subtracted, the MAX-DOAS in-plume DSCD and VMR might be underestimated, which could explain the lower MAX-DOAS value compared to the AirMAP result.

Another possible explanation for the lower MAX-DOAS values could be the underestimation of the VMR due to overestimation of path lengths because of negligence of correction factors as mentioned in Sect. 3.1.

Figure 12 presents another AirMAP overpass over several plumes from 10 min earlier, again showing good agreement between the measured plume position and the approximate plume positions derived from the onion-peeling MAX-DOAS method. It shows even better how modeled plumes and real plume positions measured by AirMAP fit together. A computation of in-plume VMRs is not possible in this case, as two plumes are located along ΔL and they are also not fully covered by ΔL.

Figure 12Map showing the MAX-DOAS path-averaged VMRs (colored lines) and AirMAP vertical columns of NO2 (broad image stripe beneath) on 21 August 2013 around 09:43 UTC (11:43 LT). Magenta triangles show current ship positions and course, and magenta numbers denote the ship length. The modeled plumes (for the MAX-DOAS measurement time) are shown in gray, with the lightness of the gray shading representing the plume age. The time difference between AirMAP and MAX-DOAS measurements is indicated in the map at specific parts of the flight track. Wind direction and speed are shown with a meteorological wind barb.

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5 Conclusions
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The present study describes a novel application of the onion-peeling MAX-DOAS approach to measurements of shipping emissions to estimate the two-dimensional pollutant distribution in the strongly inhomogeneous NO2 field over a shipping lane. The ability to probe air masses at different horizontal distances to the instrument to derive the approximate ship plume positions in the measurement area is shown on the basis of selected case studies out of the 3-year measurement period on the island Neuwerk. Located in the German Bight, 6–7 km south of the main shipping lane from the North Sea into the river Elbe, the island was selected as an ideal site for the onion-peeling MAX-DOAS approach as it is a suitable distance from the shipping lane for exploiting the use of UV and visible radiation to probe the emission plumes released from the passing ships.

To determine the horizontal light path lengths for the onion peeling, a simple approach using the trace gas column of the oxygen collision complex, O4, has been applied. To compare the measurements on the shorter UV path with the measurements on the longer visible path, path-averaged volume mixing ratios have been derived from the measured column amounts of NO2. For the onion peeling, a separate NO2 VMR along the path difference, usually located over or close to the shipping lane several kilometers away from the instrument, has been computed from UV and visible measurements, allowing us to compare NO2 values close to the instrument (along the UV path) and several kilometers away (along the path difference).

It is shown that for northerly wind directions, the onion-peeling MAX-DOAS method can detect enhanced NO2 concentrations close to the instrument south of the shipping lane and low NO2 concentrations north of the shipping lane. For southerly wind directions, low NO2 values are measured close to the site south of the shipping lane and enhanced NO2 values are measured to the north of the shipping lane, demonstrating that the MAX-DOAS instrument can detect pollution several kilometers away from the instrument under wind directions unfavorable for in situ measurements.

A combination of simple forward trajectories and a Gaussian plume model has been implemented to model the ship plumes, allowing us to compute in-plume NO2 volume mixing ratios from the MAX-DOAS measurements, which is demonstrated exemplarily for a plume measured on 21 August 2013.

For validation of both the plume modeling and the MAX-DOAS results, airborne imaging DOAS measurements taken by the AirMAP instrument during the NOSE campaign on this very same day have been used. AirMAP's measured plume positions agree well with the ones estimated by using the onion-peeling MAX-DOAS approach showing that MAX-DOAS measurements can be used to derive the approximate position of ship emission plumes. The good agreement of modeled plume positions and shapes with AirMAP measurements shows that simple forward trajectories combined with a Gaussian plume model look-up table approach provide sufficient accuracy to model the two-dimensional NO2 field over the shipping lane.

By incorporating information about the vertical plume extent from either plume model or MAX-DOAS vertical scan measurements, an in-plume NO2 VMR has been derived from AirMAP measurements, too. AirMAP and MAX-DOAS in-plume VMRs agree well within their error margins, confirming the validity of the onion-peeling MAX-DOAS approach and the presented method to derive in-plume NO2 VMRs from MAX-DOAS measurements.

To conclude, the presented measurements provide a real world demonstration that the onion-peeling approach works for MAX-DOAS measurements and can successfully be applied to investigate air pollution by ships and to derive in-plume NO2 volume mixing ratios for ships passing the instrument at a distance of several kilometers.

Data availability
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Data availability.

The data used in this study are available from the cited references and directly from the authors upon request.

Author contributions
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Author contributions.

ASe and EP built the MAX-DOAS instrument; ASe, FW, EP, LK and BMÜ set up and operated the MAX-DOAS and in situ instruments on the radar tower. AR developed the DOAS retrieval code and measurement software and provided technical support. ASe performed the analysis of the MAX-DOAS data, provided the figures and wrote the manuscript. ASc and AM set up and operated the AirMAP imaging DOAS instrument during the NOSE campaign and AM provided the AirMAP level 2 data. TR is operator for the Cessna Research Aircraft from the FU Berlin and assisted preparing the flights. AR, FW, SS and JB supported data interpretation. All authors contributed to the writing of the paper.

Competing interests
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Competing interests.

The authors declare that they have no conflict of interest.

Acknowledgements
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Acknowledgements.

The research project which facilitated the reported study was funded in part by the German Federal Maritime and Hydrographic Agency (Bundesamt für Seeschifffahrt und Hydrographie, BSH) and the University of Bremen. The authors thank the Waterways and Shipping Office Cuxhaven (Wasser- und Schifffahrtsamt, WSA), the Hamburg Port Authority (HPA), the AirMAP and NOSE teams, and the FU Berlin for their help and support. Many thanks to the editor, Michel Van Roozendael, and to the two anonymous referees for their valuable comments and suggestions, which helped to improve this publication.

Financial support
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Financial support.

The article processing charges for this open-access publication were covered by the University of Bremen.

Review statement
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Review statement.

This paper was edited by Michel Van Roozendael and reviewed by two anonymous referees.

References
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