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changes in temperature and O partial pressure suggest that
2
competition between thermal decomposition of CH SCH O~
3
2
radicals and reaction with O may be a major source of MTF
2
formation in the present reaction system. Since the yield of
MTF is fairly low this implies that under conditions in the
atmosphere where the chemistry of CH SCH O ~ is not con-
5
6
7
8
9
3
2 2
trolled by reaction with NO, i.e. the remote MBL, the pro-
duction of MTF will also be low. It would be interesting to
calculate the results for lower temperatures since the impor-
tance of the MTF product pathway from CH SCH O~ ] O ,
3
2
2
if operative, should increase with decreasing temperature.
Unfortunately, this can only be resolved when temperature
kinetic data for OH ] MTF become available. The above
considerations are presently still very speculative. In order to
properly gauge the importance of the various MTF producing
pathways from CH SCH O ~ reactions it will be necessary to
10 C. OÏDowd, M. H. Smith, I. E. Consterdine and J. A. Lowe,
Atmos. Environ., 1997, 31, 73.
3
2 2
investigate the various channels individually.
11 A. Pszenny, W. Keene, C. OÏDowd, M. Smith and P Quinn,
IGACtivities News L ett., 1998, 11, 6.
12 F. Campolongo, A. Saltelli, N. R. Jensen, J. Wilson and J. Hjorth,
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4. Summary
13 A. R. Ravishankara, Y. Rudich, R. Talukdar and S. B. Barone,
Philos. T rans. R. Soc. L ondon, Ser. A, 1997, 332, 171.
14 S. B. Barone, A. A. Andrew and A. R. Ravishankara, Faraday
Discuss., 1995, 100, 39.
The OH radical initiated oxidation of DMS has been investi-
gated as a function temperature and O partial pressure. For-
2
mation of SO , DMSO, DMSO , MSIA, MSA, OCS, MTF
2
2
and SO 2~ was observed. The observed formation behaviour
of SO and DMSO with variation in temperature and O
partial pressure is in line with current mechanistic models
involving addition and abstraction channels. The data support
that DMSO, formed in the reaction of a DMSÈOH adduct
15 G. S. Tyndall and A. R. Ravishankara, Int. J. Chem. Kinet., 1991,
23, 483.
4
2
2
16 F. Yin, D. Grosjean and J. H. Seinfeld, J. Atmos. Chem., 1990, 11,
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17 A. J. Hynes, R. B. Stoker, A. J. Pounds, T. McKay, J. D. Brad-
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with O , is the major product of the OH ] DMS addition
2
channel. The observation of high yields of methane sulÐnic
18 A. J. Hynes, P. H.Wine and D. H. Semmes, J. Phys. Chem., 1986,
acid also support that further OH-radical induced oxida-
tion of DMSO results in formation of the acid in substantial
yield. Preliminary ion chromatographic analyses of
DMSOÈH O Èair photolysis systems show quite deÐnitely
90, 4148.
19 I. V. Patroescu, I. Barnes, K. H. Becker and N. Mihalopoulos,
Atmos. Environ., 1999, 33, 25.
20 S. SÔrensen, H. Falbe-Hansen, M. Mangoni, J. Hjorth and N. R.
Jensen, J. Atmos. Chem., 1996, 24, 299.
2
2
that methane sulÐnic acid is formed in the reaction of OH
with DMSO, more experiments need to be performed before
information on the yield can be given. However, the experi-
ments here on DMS and the preliminary work on DMSO
show that in assessing the contribution of DMS to CCN for-
mation in the remote MBL consideration of the fate of MSIA
21 I. Barnes, K. H. Becker and I. Patroescu, Atmos. Environ., 1996,
30, 1805.
22 I. Barnes, V. Bastian, K. H. Becker and D. Martin, in Biogenic
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ACS Symp. Ser. 393, American Chemical Society, Washington,
DC, 1989, p. 476.
23 S. P. Urbanski, R. E. Stickel and P. H. Wine, J. Phys. Chem.,
(oxidation to form SO or MSA, formation of new particles or
1998, 102, 10,522.
2
uptake by existing particles) is an important aspect in the
24 I. Barnes, K. H. Becker and I. Patroescu, Geophys. Res. L ett.,
1994, 21, 2389.
chemistry of DMS which needs to be taken into account.
MSIA chemistry is presently not adequately represented in
atmospheric chemical models. The results of the present study
suggest that the role of the chemistry of MSIA in controlling
the contribution of DMS to CCN formation in the remote
MBL will be become increasingly important with decreasing
temperature since the importance of the DMSO producing
channel increases with decreasing temperature.
25 I. Patroescu, I. Barnes and K. H. Becker, J. Phys. Chem., 1996,
100, 17,207.
26 T. S. Bates, J. A. Calhoun and P. K. Quinn, J. Geophys. Res.,
1992, 97, 9859.
27 I. Barnes, K. H. Becker and N. Mihalopoulos, J. Atmos. Chem.,
1994, 18, 267.
28 H. Beyer, Diploma Thesis, Bergische Universitat Wuppertal, June
1998.
29 E. C. Tuazon, H. MacLeod, R. Atkinson and W. P. L. Carter,
Environ. Sci. T echnol., 1986, 20, 383.
30 R. Atkinson, D. L. Baulch, R. A. Cox, R. F. Hampson, Jr., J. A.
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Acknowledgements
Financial support for this work by the European Commission
and the BTMF within the AFS project is gratefully
acknowledged.
31 O. Hertel, J. Christensen and ^. Hov, Atmos. Environ., 1994, 28,
2431.
32 A. J. Hynes and P. H. Wine, J. Atmos. Chem., 1996, 24, 23.
33 A. A. Turnipseed, S. B. Barone and A. R. Ravishankara, J. Phys.
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