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First-year sea-ice contact predicts bromine monoxide (BrO) levels better than potential frost flower contact

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Reactive halogens are responsible for boundary-layer ozone depletion and mercury deposition in Polar Regions during springtime. To investigate the source of reactive halogens in the air arriving at Barrow, Alaska, we measured BrO, a marker of reactive halogen chemistry, and correlated its abundance with airmass histories derived from meteorological back trajectories and remotely sensed sea ice properties. The BrO is found to be positively correlated to first-year sea-ice contact (R2=0.55), and weakly negatively correlated to potential frost flower (PFF) contact (R2=0.04). These data indicate that snow contaminated with sea salts on first-year sea ice is a more probable bromine source than are frost flowers. Recent climate-driven changes in Arctic sea ice are likely to alter frost flower and first year sea ice prevalence, suggesting a significant change in reactive halogen abundance, which will alter the chemistry of the overlying Arctic atmosphere.
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and halogen
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Atmos. Chem. Phys. Discuss., 6, 11051–11066, 2006
www.atmos-chem-phys-discuss.net/6/11051/2006/
© Author(s) 2006. This work is licensed
under a Creative Commons License.
Atmospheric
Chemistry
and Physics
Discussions
First-year sea-ice contact predicts
bromine monoxide (BrO) levels better
than potential frost flower contact
W. R. Simpson
1
, D. Carlson
1
, G. Hoenninger
1,2,
, T. A. Douglas
3
, M. Sturm
3
,
D. Perovich
3
, and U. Platt
2
1
Geophysical Institute and Department of Chemistry, University of Alaska Fa irbanks,
Fairbanks, AK 99775-6160, USA
2
Institute for Environmental Physics, University of Heidelberg, Im Neuenheimer Feld 229,
69120 Heidelberg, Germany
3
U.S. Army Cold Regions Research and Engineering Laboratory, P.O. Box 35170, Fort
Wainwright, AK 99703-0170, USA
deceased
Received: 23 October 2006 Accepted: 6 November 2006 Published: 7 November 2006
Correspondence to: W. R. Simpson (wrs@uaf.edu)
11051
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Abstract
Reactive halogens are responsible for boundary-layer ozone depletion and mercur y
deposition in Polar Regions during springtime. To investigate the source of reactive
halogens in the air arriving at Barrow, Alaska, we measured BrO, a marker of reactive
halogen chemistry, and correlated its abundance with airmass histories derived from5
meteorological back trajectories and remotely sensed sea ice properties. The BrO is
found to be positively correlated to first-year sea-ice contact (R
2
=0.55), and weakly
negatively correlated to potential frost flower (PFF) contact (R
2
=0.04). These data
indicate that snow contaminated with sea salts on first-year sea ice is a more probable
bromine source than are frost flowers. Recent climate-driven changes in Arctic sea ice10
are likely to alter frost flower and first year sea ice prevalence, suggesting a significant
change in reactive halogen abundance, which will alter the chemistry of the overlying
Arctic atmosphere.
1 Introduction
During late winter and spring, oxidation chemistry in the Arctic troposphere shifts from15
being dominated by ozone photochemistry to being dominated by halogen chemistry,
especially reactive bromine chemistry. This shift has profound influences that range
from depletion of tropospheric ozone to deposition of mercury to alteration of the fate
and lifetime of organic pollutants (Barrie et al., 1988; Schroeder et al., 1998). The
majority of the bromine atoms responsible for ozone depletion and mercury deposi-20
tion come from salts containing bromide (Br-) that originate from the ocean and are
oxidized to bromine atomic radicals through an autocatalytic reaction pathway known
as the bromine explosion (Fan and Jacob, 1992; McConnell et al., 1992). The trans-
fer mechanism by which the salts become atmospherically accessible is not currently
understood, yet this mechanism plays a fundamental role in activating halogens that25
deposit airborne contaminants (e.g. Hg) to the terrestrial cryosphere.
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Two hypotheses have been presented for the mechanism of bromide salt transport
from the ocean to reactive bromine in the atmosphere. Frost flowers, which are highly
saline, have been proposed to provide the surface from which bromine is released
(Rankin et al., 2002). Kaleschke et al. (2004) and co-workers used remotely sensed
sea ice data to predict where frost flowers may be forming on sea ice. They introduced5
a proxy they called potential frost flowers (PFF), which is calculated by a thermody-
namic model of sea ice and frost flower growth and found that PFF is correlated with
BrO detected by satellite (Kaleschke et al., 2004). Jones et al. (2006) found that ozone
depletion events detected at Halley Bay, Antarctica were correlated with airmass mo-
tions that brought air in contact with a large coastal polyna that often produces frost10
flowers. Snow contaminated with salts, which are prevalent on first-year sea ice, has
also been proposed to be the surface from which bromine is released. Direct mass-
spectroscopic evidence of release of Br
2
and BrCl (precursors of BrO) from snow (Fos-
ter et al., 2001), and depletions of Br- in coastal snow (Simpson et al. , 2005) provide
evidence for the salty snow hypothesis. Satellite observations (Wagner et al., 2001)15
and ground-based observations of BrO in Antarctica (Frieß et al., 2004) also point to
first-year ice as an important region for bromine activation.
Freezing sea water separates ice from brine, which is a concentrated salt solution.
Some of this brine is forced to the new ice surface, causing high initial surface salini-
ties of 50–100 parts per thousand by weight (‰, where Arctic Ocean sea-water salin-20
ity 30‰). As the ice ages, the surface salinity decreases to approximately 5–10‰.
Snow on the sea ice is contaminated by salts when brine wicks up the snow or the
wind scours the snow to re-expose saline surfaces or salt aerosols deposit to the snow
(Domine et al., 2004). Sea ice that sur vives the summer has a much lower surface
salinity because the brine drains away during summer melting. Therefore, multi-year25
sea ice (MYI) and land surfaces contain less atmospherically accessible salt and are
less likely to be reactive halogen sources than first-year sea ice (FYI). Frost flowers
form when open leads or polynyas freeze over and small nodules in the forming ice act
as condensation nuclei for vapor deposition of angular ice crystals that look like deli-
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cate flowers. The flowers wick brine from the sea-ice surface producing highly saline
(100‰) crystals with specific surface areas similar to that of surface hoar (Domine
et al., 2005; Perovich and Richter-Menge, 1994).
2 Methods
The contact time of an air parcel with potential frost flowers (PFF) or first-year ice5
(FYI) is calculated by combining back-trajectory analysis, which provides air motion
and temperature with remotely sensed sea ice data, which provides information on
where open water and ice are present. In the PFF calculation, open water is assumed
to be freezing over and producing new frost flowers with increasing eciency as the
temperature decreases (Kaleschke et al. , 2004). Figure 1 shows an example of this10
calculation where a trajectory passes near a coastal polynya in the vicinity of Banks
Island, Canada.
2.1 PFF calculation
For each hour during the winter/spring of 2005, we calculate a 72 h back trajector y
at 50 m arrival height using the HYSPLIT trajectory model (Draxler and Rolph, 2003).15
In the time period shown (DOY 80–120), there are 960 total trajectories considered.
Other arrival heights (of 100 and 300 m) were explored and shown to have similar re-
sults. The open water fraction, assumed to be 1 sea ice concentration, comes from
ASI algorithm (Kaleschke et al., 2001) sea-ice maps (based upon AMSR-E data) at the
6.25 km resolution downloaded from http://www.seaice.de/. Airmasses are propagated20
back along the prescribed trajectory and minutes of contact with open water are calcu-
lated on a pixel-by-pixel basis using the appropriate daily sea-ice map. For example, if
the trajectory spends 30 min in a particular pixel, and the sea-ice fraction is 66% in that
pixel, then there are (10.66) × 30 min =10 min of open water contact for this pixel. We
then use the PFF parameterization (Kaleschke et al., 2004) based upon the parcel’s25
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temperature to calculate the percent of open water that could maximally be covered
by frost flowers. Continuing the example, say the PFF parameterization indicates 50%
PFF coverage. We then multiply the 10 min in this pixel by 0.5 to get 5 min of PFF
contact. The PFF contact is then summed over the entire 72 h trajectory to get the total
PFF contact for the airmass arriving at Barrow at the arrival time. If the trajectory goes5
over 1 km height, it is assumed to no longer have sea-ice contact. This 1 km height
was chosen as a typical height of the convective cloud that would be in the presence
of a lead.
Airmass dispersion occurs in the atmosphere but is not accounted for in the trajec-
tory calculation. Additionally, inaccurate meteorological fields cause back trajectory10
errors. Therefore, we added a feature to the calculation where the average sea ice
concentration in a circle centered at the trajectory’s calculated position is used instead
of simply the immediate pixel of the calculated position. This circle increases in radius
as time is propagated backwards at 2 km/hr. This “diusion” rate is about 1/10th of the
wind speed and results in a radius of 140 km three days before arrival. Substituting15
this algorithm for the simple pixel-by-pixel calculation smoothed some high-frequency
noise in the PFF time series, and was chosen as more realistic. In the example shown
in Fig. 1, the PFF contact is with the polynya areas near Banks Island, Canada and
arises from the radial averaging algorithm causing overlap of the trajectory with the
open water shown in that vicinity.20
We performed many tests where the recently past sea ice conditions (up to 5 days
earlier) were considered instead of the current sea-ice conditions. The idea of these
tests was to see if frost flowers that may have formed a few days before the trajec-
tory passed over a pixel were responsible for halogen activation. None of these tests
showed significantly better correlation with BrO, and thus we present the results using25
the formulation used by Kaleschke et al. (2004) because it has been accepted in the
literature.
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2.2 First-year sea-ice contact calculation
First year ice (FYI) contact is calculated in a similar manner along the same trajectories,
following the method of Frieß et al. (2004). Regions of older ice (second year or older)
were identified through examination of QuikSCAT sea ice backscatter coecient, which
is a proxy for sea ice age (Voss et al., 2003). The QuikSCAT data were downloaded5
from http://www.ifremer.fr/. We found that the region of older ice is relatively stationary
during the 40-day period of analysis. Therefore, one mask of old sea ice, shown in
yellow in Fig. 1, was generated from the observation on DOY 100 (10 April 2005). With
this mask, we identify regions of first-year sea ice and sum the ice fraction times the
contact time for each pixel along the trajectory. If the trajector y indicates that the parcel10
is at an altitude over 100 m (twice the 50 m arrival height), we consider the contact with
the surface is lost and do not accumulate any first-year sea-ice contact.
2.3 Chemical measurements
Bromine monoxide (BrO) and ozone were measured continually at Barrow, Alaska
(71.3 N, 156.7 W) over the winter and spring of 2005. Bromine monoxide was mea-15
sured by multiple-axis dierential optical absorption spectroscopy (MAX-DOAS) (Hoen-
ninger and Platt, 2002). Measurements were made at multiple viewing elevations to
separate stratospheric BrO from tropospheric BrO and to derive vertical profiles of
the BrO concentration. Strict inversion of the data to concentration profiles is compli-
cated by radiation transfer issues. Therefore, we chose the dierence in slant column20
density (DSCD) of BrO between a 2-degree elevation angle measurement and a near-
coincident zenith measurement to quantify the tropospheric BrO abundance. The high
degree of correlation shown in this work argues for the accuracy of this simple quan-
tification of BrO. For clear-sky conditions, 10
14
molecule cm
2
DSCD corresponds to
about a 5 parts per trillion by volume (pptv) mixing ratio in a 1 km thick mixed layer. The25
peak values shown here are 30 pptv, which is similar to values seen at other Arctic lo-
cations where halogen activation is prevalent (Hausmann and Platt, 1994; Hoenninger
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and Platt, 2002; Tuckermann et al., 1997). Hourly in-situ ozone mixing ratios were mea-
sured by the National Oceanic and Atmospheric Administration (NOAA) Earth Systems
Research Laboratory/Global Monitoring Division (ESRL/GMD).
3 Results
Figure 2 shows time series of ozone, BrO, FYI contact, and PFF contact for Barrow,5
Alaska. Ozone and BrO are generally anticorrelated, as expected because BrO de-
stroys ozone. Because it requires time for BrO to destroy ozone, the anticorrelation is
not precise, and BrO is considered a better marker of halogen activation. The BrO data
follow the FYI contact remarkably well, particularly the rapid variations during the pe-
riod DOY 110 to 119. In contrast, the BrO shows little relationship to PFF. The largest10
BrO events (DOY 110 to 112) occur after very little PFF contact, while the largest PFF
contact event, DOY 115, is correlated with essentially no BrO. Therefore, PFF appears
unrelated to BrO.
There are two days where FYI contact is high but BrO is near zero, DOY 88 and 97.
Both of these days have extremely low ozone, nearly always <1 ppbv, as indicated by15
the red coloring of all BrO data when O
3
<1 ppbv. At these low ozone levels, reactive
bromine (the sum of the concentrations of Br and BrO) partitions to Br atoms because
the ozone necessary to form BrO is absent. Therefore, the absence of BrO on DOY 88
and 97 is expected, and we exclude these data from later analysis.
Figure 3 shows the correlations of BrO with FYI and BrO with PFF contact. BrO20
is positively correlated with FYI contact while BrO is weakly anticorrelated with PFF.
Although the functional form of the relationship between BrO and FYI is unknown, a
simple linear model appears to fit well and can explain 55% of the variance in BrO
(R
2
=0.55). This correlation is quite impressive given inaccuracies in the trajectory
model and inevitable variations in other important meteorological parameters, such as25
wind speed and inversion height. On the other hand, a linear model of the depen-
dence of BrO on PFF can explain <5% of the variance (R
2
=0.04), and the slope of the
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correlation is opposite to the expectation that PFF should produce BrO. The intercept
of this correlation, which indicates significant BrO in the absence of PFF contact also
does not make sense. These findings clearly indicate that contact with first-year sea
ice provides the majority of reactive bromine to airmasses that arrive at Barrow during
the ozone depletion season.5
4 Discussion
The potential frost flower algor ithm was chosen for this work because Kaleschke et al.
(2004) reported that PFF from large polynya areas spatially matched regions of en-
hanced BrO detected by satellite. In the Kaleschke study, PFF came mostly from large
coastal polynyas because those areas are a major source of open water in the Polar10
Regions. In our study, we also find that most airmasses with high PFF contacts can
be traced to coastal polynyas or leads. Although there is commonly a lead a few kilo-
meters from Barrow, this lead opens when winds drive ice away from the shore, and
this lead seldom aects airmasses that blow onshore to the Barrow site. Therefore, the
leads/polynyas that contribute to PFF typically impact the airmass days before arrival at15
Barrow and the overall PFF contact time is quite low. If the influence of polynyas/leads
occurs relatively local to the source, their influence could have diminished before air-
masses impact Barrow, which might explain the lack of correlation seen here. If it is
the case that PFF produces only a local eect, then there must be another source of
reactive bromine, associated with sea ice, to explain the high levels of BrO observed20
at Barrow in this study.
In the Jones et al. (2006) study, ozone depletion was observed when airmasses
passed over a coastal polyna, which they interpreted as being covered by frost flowers
and these frost flowers providing reactive bromine to deplete the ozone. The trajecto-
ries shown in the Jones et al. paper also pass across areas of first-year sea ice before25
traversing the coastal polynya, so it is possible that a sea-ice source of bromine caused
their ozone depletions instead of the interpretation that frost flowers caused the ozone
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depletion. In our analysis of data arriving at Barrow, the dierent mechanisms of PFF
contact and FYI contact allow the PFF and FYI contact time series to be very dierent
and allow separation of the sources. It is unclear from the Jones et al. analysis whether
potential frost flower contact and first-year sea-ice contacts are dierent in their data.
Therefore, we cannot speculate on whether their data uniquely point to frost flowers5
as the source of reactive bromine, but simply note that their data probably could be
alternatively interpreted as due to first-year sea-ice contact.
Our study clearly shows that first-year sea ice is correlated with reactive halogen
production, but we need to consider what specific property of these geographic areas
is responsible for the halogen production. Ice motion, even in the middle of the pack,10
causes cracks to form such that on the order of a percent of the ice area is open water.
Given cold temperatures, these open leads freeze over, forming surface brine. Frost
flower formation additionally requires supersaturated water vapor, which depends on
the presence of nearby open leads to source the water vapor (Andreas et al., 2002).
Because small leads may be dicult to detect by satellite remote sensing, we cannot15
preclude the possibility that some frost flowers have formed in the first-year ice even
though the calculated PFF contact is very small for these trajectories. As brine and
frost-flower covered areas age, on the time scale of a few days, they may be covered by
snow or the frost flowers could be blown away by wind (Perovich and Richter-Menge,
1994). Therefore, frost flower formation is temporally transient in addition to being20
spatially limited. The property of frost flowers thought to make up for these limiting
factors is their specific surface area (the ice surface area per mass), which was initially
estimated to be very large (Rankin et al., 2002). However, the specific surface area of
frost flowers has recently been shown to be much smaller and similar to that of snow
(Domine et al., 2005), making frost flowers appear less likely as the bromine source.25
Overall, frost flowers that may be present in the first-year ice would only provide a
saline surface over small areas and for short periods of time.
Snow contaminated by salts is ubiquitous in the FYI area. Snow on sea ice has a
wide distribution of depths and large areas are only covered by shallow snow that can
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be influenced by brine wicking from the sea ice surface. Snow on FYI is also shallower
(mean depth 20 cm) and less prevalent than snow on MYI (Sturm et al., 2002). Studies
from Antarctica have shown snow salinities of 5‰ commonly occur at heights up to
20 cm in the snow pack (Massom et al., 2001), and summertime measurements from
the Arctic show highly variable snow salinity with an average of 1‰ that may have been5
reduced by summer brine drainage (Eicken et al., 2002). Wind pumping of air through
snow also increases the depth within the snowpack to which sea salts can become
atmospherically accessible. Frost flowers could produce aerosols that contaminate
the snow surface and this snow could later release bromine, leading to correlation with
first-year sea-ice but not PFF. From these observations, we find that saline snow on the10
first-year sea ice is ubiquitous and contains significant quantities of salts necessary for
halogen activation. Therefore, the common source of salty snow appears more likely
than the transient and spatially limited frost flowers that may have formed but have
been undetected by the PFF method.
5 Conclusions15
Potential frost flower contact time, as calculated by meteorological back trajectories
and remotely sensed sea ice features is not well correlated to BrO arriving at Bar-
row, while first-year sea-ice contact is positively correlated to BrO. These data point to
first-year sea ice areas as the major source region for reactive bromine arriving at Bar-
row during the ozone depletion season with salty snow apparently being the bromine20
source mechanism. The Arctic has recently seen dramatic reductions in sea ice cover-
age and increases in air temperatures, with most models predicting further ice losses
(Johannessen et al., 1999; Over peck et al., 2005; Serreze et al., 2003; Stroeve et al.,
2005). This mar ked modification of sea ice coverage is likely to have dierent eects
on formation of first-year sea ice and frost flowers. For example, a warmer Arctic with25
less summer sea ice might have less frost flowers in spring due to warmer tempera-
tures but more saline snow on first-year sea ice. A better mechanistic understanding of
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the relative global importance of these two possible reactive bromine sources is critical
for meaningful prediction of future halogen activation, boundary-layer ozone depletion,
and mercury deposition in the context of a rapidly changing Arctic.
Acknowledgements. This work was supported by the National Science Foundation, under grant
OPP-0435922. Logistical support from the Barrow Arctic Science Consortium is gratefully ac-5
knowledged. We also thank U. Frieß for the suggestion to try correlation of BrO with first-year
sea-ice contact. We thank NOAA for providing the ozone measurements and the HYSPLIT
trajectory model.
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E. C., III, S. C., Gerlach, S. C., Hamilton, L. C., Hinzman, L. D., Holland, M., Huntington,
H. P., Key, J. R., Lloyd, A. H., MacDonald, G. M., McFadden, J., Noone, D., Prowse, T. D.,
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Schlosser, P., and V
¨
or
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osmarty, C.: Arctic System on Trajectory to New, Seasonally Ice-Free
State, Eos Trans. AGU, 86, 309, 2005. 11060
Perovich, D. and Richter-Menge, J. A.: Surface characteristics of lead ice, J. Geophys. Res.,
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Schroeder, W. H., Anlauf, K. G., Barrie, L. A., Lu, J. Y., Steen, A., Schneeberger, D. R., and
Berg, T.: Arctic springtime depletion of mercury, Nature, 394, 331–332, 1998. 11052
Serreze, M. C., Maslanik, J. A., Scambos, T. A., Fetterer, F., Stroeve, J., Knowles, K., Fowler,
C., Drobot, S., Barry, R. G., and Haran, T. M.: A record minimum arctic sea ice extent and10
area in 2002, Geophys. Res. Lett., 30, 1110, doi:10.1029/2002GL016406, 2003. 11060
Simpson, W. R., Alvarez-Aviles, L., Douglas, T. A ., Stu rm, M., and Domine, F.: Halogens in the
coastal snow pack near Barrow, Alaska: Evidence for active bromine air-snow chemistry dur-
ing springtime, Geophys. Res. Lett., 32, L04811, doi:10.1029/2004GL021748, 2005. 11053
Stroeve, J. C., Serreze, M. C., Fetterer, F., Arbetter, T., Meier, W., Maslanik, J., and Knowles,15
K.: Tracking the Arctic’s shrinking ice cover: Another extreme September minimum in 2004,
Geophys. Res. Lett., 32, L04501, doi:10.1029/2004GL021810, 2005. 11060
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B., Unold, W., and Platt, U.: DOAS-observation of halogen radical-catalysed arctic bound-
ary layer ozone destruction du ring the ARCTOC campaigns 1995 and 1996 in Ny-Alesund,
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3-day back trajectory arriving
at Barrow 0Z 13 Apr 05 (DOY 103.0)
Sea Ice map 10 Apr (DOY100)
Brown = Land Yellow = >1yr. ice
Fig. 1. An example of a 3-day back trajectory arriving at Barrow, Alaska. The arrival time is
00:00 UTC on 13 April 05 (DOY 103.0). The sea-ice map is shown for 10 April because the
main contact of these trajectories with open water occurred on that day. The proper sea-ice
map is used for each day of the trajector y calcul ation. The ice map shows brown for land,
a gradation from black to white via blue tones for ice concentration, from AMSR-E data, and
yellow for the area identified as multi-year ice from QuikSCAT sea ice age estimations.
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6
4
2
0
BrO DSCD / 10
14
molec cm
-2
120110100
9080
DOY 2005
50
40
30
20
10
0
O
3
/ ppbv
4000
3000
2000
1000
0
FYI contact / min
8
6
4
2
0
PFF contact / min
Fig. 2. Ozone, Bromine monoxide (BrO), first-year sea-ice contact (FYI), and potential frost
flowers contact (PFF) timeseries in the period DOY 80–120. BrO data colored red occurred
when ozone <1 ppbv.
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6
5
4
3
2
1
0
BrO DSCD / 10
14
molec cm
-2
40003000200010000
FYI contact / minutes
R
2
= 0.55
6
5
4
3
2
1
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BrO DSCD / 10
14
molec cm
-2
76543210
PFF contact / minutes
R
2
= 0.04
Fig. 3. Correlation plots of B rO versus first-year sea-ice contact (left) and potential frost flowers
contact (right). Data colored in red occurred when ozone <1 ppbv and were ignored from the
correlation analysis.
11066
... The active bromine is considered to ultimately derive from sea salt bromide (Platt and Moortgat 1999), but the process that triggers the release of active bromine has yet to be identified conclusively (Bottenheim et al. 2002). The role of frost flowers remains controversial: Rankin et al. (2002), Kaleschke et al. (2004, and Sander et al. (2006) favor them as an important direct source while Simpson et al. (2005 Simpson et al. ( , 2006), Domine et al. (2005) and Kalnajs and Avallone (2006) present arguments that frost flowers do not play a unique role in directly triggering reactive halogen release to the atmosphere. Two catalytic cycles are believed to dominate the net ozone destruction: 2O 3 →3O 2 (Le Bras and Platt 1995; Platt and Lehrer 1997; Wagner et al. 2001). ...
Article
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During the Tropospheric Ozone Production about the Spring Equinox (TOPSE) program, aircraft flights during April 7–11, 2000 revealed a large area air mass capped below ∼500 m altitude over Hudson Bay, Canada in which ozone was reduced from normal levels of 30–40 ppbv to as low as 0.5 ppbv. From some of the in-situ aircraft measurements, back-trajectory calculations, the tropospheric column of BrO derived from GOME satellite measurements, and results from a regional model, we conclude that the event did not originate from triggering of reactive halogen release in the sub-Arctic region of Hudson Bay but resulted from such an event occurring at higher latitudes over the islands of the northern Canada Archipelago and nearby Arctic Ocean with subsequent transport over a distance of 1,000–1,500 km to Hudson Bay. BrOx remained active during this transport despite considerable changes in the conditions of the underlying surface suggesting that chemical recycling during transport dominated any local halogen input from the surface. If all of the tropospheric column density of BrO is distributed uniformly within the surface layer, then the mixing ratio of BrO derived from the satellite measurements is at least a factor of 2–3 larger than derived indirectly from in situ aircraft measurements of the NO/NO2 ratio.
Article
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Long term atmospheric mercury measurements in the Southern Hemisphere are scarce and in Antarctica completely absent. Recent studies have shown that the Antarctic continent plays an important role in the global mercury cycle. Therefore, long term measurements of gaseous elemental mercury (GEM) were initiated at the Norwegian Antarctic Research Station, Troll (TRS) in order to improve our understanding of atmospheric transport, transformation and removal processes of GEM. GEM measurements started in February 2007 and are still ongoing, and this paper presents results from the first four years. The mean annual GEM concentration of 0.93 ± 0.19 ng m<sup>−3</sup> is in good agreement with other recent southern-hemispheric measurements. Measurements of GEM were combined with the output of the Lagrangian particle dispersion model FLEXPART, for a statistical analysis of GEM source and sink regions. It was found that the ocean is a source of GEM to TRS year round, especially in summer and fall. On time scales of up to 20 days, there is little direct transport of GEM to TRS from Southern Hemisphere continents, but sources there are important for determining the overall GEM load in the Southern Hemisphere and for the mean GEM concentration at TRS. Further, the sea ice and marginal ice zones are GEM sinks in spring as also seen in the Arctic, but the Antarctic oceanic sink seems weaker. Contrary to the Arctic, a strong summer time GEM sink was found, when air originates from the Antarctic plateau, which shows that the summertime removal mechanism of GEM is completely different and is caused by other chemical processes than the springtime atmospheric mercury depletion events. The results were corroborated by an analysis of ozone source and sink regions.
Article
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We present Multi AXis-Differential Optical Absorption Spectroscopy (MAX-DOAS) observations of tropospheric BrO carried out on board the German research vessel Polarstern during the Antarctic winter 2006. Polarstern entered the area of first year sea ice around Antarctica on 24 June 2006 and stayed within this area until 15 August 2006. For the period when the ship cruised inside the first year sea ice belt, enhanced BrO concentrations were almost continuously observed. Outside the first year sea ice belt, typically low BrO concentrations were found. Based on back trajectory calculations we find a positive correlation between the observed BrO differential slant column densities (ΔSCDs) and the duration for which the air masses had been in contact with the sea ice surface prior to the measurement. While we can not completely rule out that in several cases the highest BrO concentrations might be located close to the ground, our observations indicate that the maximum BrO concentrations might typically exist in a (possibly extended) layer around the upper edge of the boundary layer. Besides the effect of a decreasing pH of sea salt aerosol with altitude and therefore an increase of BrO with height, this finding might be also related to vertical mixing of air from the free troposphere with the boundary layer, probably caused by convection over the warm ocean surface at polynyas and cracks in the ice. Strong vertical gradients of BrO and O3 could also explain why we found enhanced BrO levels almost continuously for the observations within the sea ice. Based on our estimated BrO profiles we derive BrO mixing ratios of several ten ppt, which is slightly higher than many existing observations. Our observations indicate that enhanced BrO concentrations around Antarctica exist about one month earlier than observed by satellite instruments. From detailed radiative transfer simulations we find that MAX-DOAS observations are up to about one order of magnitude more sensitive to near-surface BrO than satellite observations. In contrast to satellite observations the MAX-DOAS sensitivity hardly decreases for large solar zenith angles and is almost independent from the ground albedo. Thus this technique is very well suited for observations in polar regions close to the solar terminator. For large periods of our measurements the solar elevation was very low or even below the horizon. For such conditions, most reactive Br-compounds might exist as Br2 molecules and ozone destruction and the removal of reactive bromine compounds might be substantially reduced.
Article
Mercury is deposited to the Polar Regions during springtime atmospheric mercury depletion events (AMDEs) but the relationship between snow and ice crystal formation and mercury deposition is not well understood. The objective of this investigation was to determine if mercury concentrations were related to the type and formation of snow and ice crystals. On the basis of almost three hundred analyses of samples collected in the Alaskan Arctic, we suggestthat kinetic crystals growing from the vapor phase, including surface hoar, frost flowers, and diamond dust, yield mercury concentrations that are typically 2-10 times higher than that reported for snow deposited during AMDEs (approximately 80 ng/L). Our results show that the crystal type and formation affect the mercury concentration in any given snow sample far more than the AMDE activity prior to snow collection. We present a conceptual model of how snow grain processes including deposition, condensation, reemission, sublimation, and turbulent diffusive uptake influence mercury concentrations in snow and ice. These processes are time dependent and operate collectively to affect the retention and fate of mercury in the cryosphere. The model highlights the importance of the formation and postdeposition crystallographic history of snow or ice crystals in determining the fate and concentration of mercury in the cryosphere.
Article
Full-text available
We measured halide concentrations of snow and frost flowers in the vicinity of Barrow, Alaska. We find that the ratio of bromide to sodium in frost flowers is slightly enhanced (~10%) as compared to sea water. In contrast, the ratio of bromide to sodium in some snow samples is more than an order of magnitude enhanced, and in other samples is more than an order of magnitude depleted. We interpret the bromide depleted snow as having been processed by heterogeneous chemistry and providing reactive halogen compounds to the atmosphere. The eventual end product of reactive bromine chemistry is HBr that is then deposited over a wide region, enhancing bromide in inland snow samples. Although frost flowers or open leads are likely to be the original source of halides that become reactive halogen gases, we find that the bromide release often occurs subsequent to production of aerosol from marine sources.
Article
Full-text available
Frost flowers grow on newly-formed sea ice from a saturated water vapour layer. They provide a large effective surface area and a reservoir of sea salt ions in the liquid phase with triple the ion concentration of sea water. Recently, frost flowers have been recognised as the dominant source of sea salt aerosol in the Antarctic, and it has been speculated that they could be involved in processes causing severe tropospheric ozone depletion events during the polar sunrise. These events can be explained by heterogeneous autocatalytic reactions taking place on salt-laden ice surfaces which exponentially increase the reactive gas phase bromine (``bromine explosion''). We analyzed tropospheric bromine monoxide (BrO) and the sea ice coverage both measured from satellite sensors. Our model based interpretation shows that young ice regions potentially covered with frost flowers seem to be the source of bromine found in bromine explosion events.
Article
During the ALERT2000 polar sunrise experiment at Alert, Nunavut, Canada, we performed measurements of boundary layer bromine oxide radicals (BrO) by differential optical absorption spectroscopy (DOAS) using scattered sunlight in the spectral range from 320 to 400 nm. For the first time the Multi-Axis-(MAX)-DOAS method was applied to derive vertical profile information of BrO. BrO was observed at slant column densities (SCD) of up to 1015 molecules/cm2 during a 10-day period of complete surface ozone depletion. The largest BrO column densities were found by observing scattered sunlight from 5° above the horizon, and SCDs were decreasing with increasing elevation angles of the light-receiving telescope. For zenith scattered light the lowest absorption was recorded. Radiative transfer modelling and the calculation of air mass factors show that in most cases the bulk of the observed BrO was present in a layer of 1±0.5 km thickness above the surface (in the boundary layer). The inferred extent of the BrO layer agrees very well with the observed height of the ozone depletion layer (Bottenheim et al., Atmos. Environ., 2002) from ozone sonde data. Assuming that BrO layer is well-mixed, volume mixing ratios reached levels of 20–30 ppt BrO. These values are consistent with previous measurements of BrO during low ozone events in the Arctic boundary layer.
Article
In the Alaskan Beaufort Sea, ice properties and surface conditions typical of springtime leads were monitored at three sites during the initial few days of growth. Observations indicate that once the ice thickness reached approximately 2 cm, a thin (~1 mm), highly saline skim of brine formed on the surface. After only a few hours of growth the initially smooth surface of the sea ice developed some small-scale roughness. Frost flowers, the result of ice grown from the vapor phase, quickly formed on the surface of the sea ice and continued to develop during the observations. Possible mechanisms for the development and evolution of the surface skim and frost flowers are discussed. -from Authors
Article
Elevated mercury concentrations have been reported in arctic coastal snow far from emission sources. The mercury is deposited during mercury depletion events (MDEs), a set of photochemical atmospheric reactions involving reactive halogens. The highest mercury concentrations are clustered near the coast, leading to speculation that sea ice or sea ice leads play a role in MDEs. The nature of this connection is not fully understood. We report mercury concentrations up to 820 ng/L in snow and frost flowers along sea ice leads near Barrow, Alaska. These concentrations are nine times higher than values from nearby coastal snow and are almost half of the mercury maximum contaminant level in United States drinking water. The high values were found only near leads that had convective plumes above open water suggesting that the same processes that produce a supersaturated environment for water vapor near sea ice leads may be instrumental in mercury deposition.
Article
In polar regions, severe marine boundary layer ozone depletion episodes (ODEs) are a yearly recurring phenomenon in the spring. Using 9 years of 10-day three-dimensional trajectory calculations, the origin of ODEs at three Arctic observatories is investigated. The analysis indicates that marginal ice zones are potential source regions of ODEs. Those regions do broadly correspond to areas where increased levels of bromine oxide (BrO), an indicator of ozone depletion chemistry, are observed by the GOME satellite. The source region of ODEs, observed at Barrow, Alaska, is found to be about 1 day's travel upwind, in agreement with expectations based on the rate at which O3 depletion chemistry occurs. In contrast, the likely source region for ODEs observed at Alert, Canada, and Zeppelinfjellet, Norway, appears to be located several days' travel upwind, off the Siberian coast. This result may reflect the absence of favorable ice conditions for O3 depletion chemistry nearer those sites. Assuming that O3 depletion occurs at those regions, this implies that air parcels without O3 remain that way for several days or the depletion is slower than current understanding of the O3 depletion chemistry suggests. Rapid changes in O3 mole fractions at those measurement sites appears not to be an indication of fast chemical destruction of ozone but rather are due to abrupt air mass changes. Data for September indicate a much narrower distribution of ozone mole fractions and no particular pattern linking a preferred area with lower mole fractions.
Article
Bromine oxide (BrO) is proposed to be an important agent for tropospheric ozone depletion, as observed in the high Arctic during springtime. In this paper we report measurements of bromine oxide and ozone by Long Path Differential Optical Absorption Spectroscopy (LPDOAS), 8.6-km light path), performed in April 1992 in Alert (82.3°N, 62.2°W). BrO mixing ratios were found between the detection limit of about 4 ppt to 17 ppt. Because of the frequently poor visibility conditions, especially during ozone depletion events, long-signal integration times (sometimes more than 24 hours) were needed, and short-time BrO-peaks might have escaped detection. A pure in situ chemical mechanism based on BrO-catalyzed ozone destruction cannot account for the observed complete depletion of ozone at the observed BrO mixing ratios. On the other hand, it can be argued that the maximum time for chemical ozone depletion (by any mechanism) may not be much longer than 1 day. A simple scenario involving a combination of advection, atmospheric dispersion, and BrO-catalyzed chemical ozne destruction is described, which could explain the observed ozone loss.
Article
Satellite passive microwave observations document an overall downward trend in Arctic sea ice extent and area since 1978. While the record minimum observed in September 2002 strongly reinforced this downward trend, extreme ice minima were again observed in 2003 and 2004. Although having three extreme minimum years in a row is unprecedented in the satellite record, attributing these recent trends and extremes to greenhouse gas loading must be tempered by recognition that the sea ice cover is variable from year to year in response to wind, temperature and oceanic forcings.