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(11) Rodgers, M. O.; Bradshaw, J, D.;. Sandholm, S. T.; et al./. Geophys. Res. ... Center for Atmospheric Research. He re- ceived his B.S. degree in p...
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measurement techniques. In fact, the broad acceptance that OH concentra­ tions can be accurately m e a s u r e d will probably not be realized until a successful intercomparison of several different instruments under a vari­ ety of conditions is achieved. Thus, in the near future several OH instru­ ments will be tested in informal intercomparisons, and a formal inter­ comparison (i.e., w i t h " b l i n d " submission of m e a s u r e m e n t s ) will probably be made two or three years down the road. This does not, however, mean that nothing useful will be done until that time. Some OH m e a s u r e m e n t s are already being t a k e n seriously and are beginning to inspire researchers to work on newly identified problem areas. For some time, long-path ab­ sorption studies conducted near ur­ ban European sites have suggested t h a t measured OH concentrations are consistently lower t h a n those p r e d i c t e d by fast p h o t o c h e m i c a l model calculations. In 1991 the in­ tercomparison in the Colorado moun­ t a i n s of the l o n g - p a t h absorption and the i o n - a s s i s t e d chemical in­ s t r u m e n t s m e n t i o n e d earlier was also part of a limited photochemistry study. Whereas agreement between the two instruments was reasonably

good, the OH concentrations m e a ­ sured were three to five times lower than calculated values (27). This re­ sult has led to the belief that not all OH losses were being accounted for a n d t h a t u n m e a s u r e d compounds might be responsible at least in part for the discrepancy. An i n t e r c o m p a r i s o n w a s m a d e during this past summer at the same location and with the same investi­ gators as in the latter intercompari­ son, but with the addition of an in situ low-pressure LIF OH measure­ ment technique. This intercompari­ son c o n t a i n e d a p h o t o c h e m i s t r y study portion t h a t emphasized the identification and quantification of hydrocarbon species that could be re­ s p o n s i b l e for OH loss. T h u s , OH m e a s u r e m e n t s are already helping identify areas where additional in­ vestigation is needed, and OH mea­ surements will gain more credibility with each successful intercompari­ son.

What next? Although OH measurements are be­ coming both more credible and more sensitive, generally they are not be­ coming any simpler or less expen­ sive, a n d the applications of such measurements must be well planned.

938 A · ANALYTICAL CHEMISTRY, VOL. 65, NO. 21, NOVEMBER 1, 1993

REPORT The measurement of OH by itself is of little value; in order for a n OH measurement to provide new insight, it must be imbedded in a reasonably complete photochemistry study. A realistic goal for such studies would be to further our u n d e r s t a n d i n g of the natural photochemical processes that control the chemical and physi­ cal properties of the E a r t h ' s atmo­ sphere. In addition, although photochem­ istry is often considered to be prima­ rily a mechanism for producing the strong oxidants that help cleanse the atmosphere, these same oxidants also react with atmospheric constitu­ ents, such as sulfur compounds, to form some very nonvolatile products, such as sulfuric and methane sulfon­ ic acid. These compounds leave the gas phase at their first opportunity, resulting in aerosol growth and, u n ­ der the proper conditions, probably new particle formation. The result­ ing aerosol growth/production can then have both direct and indirect ef­ fects on the scattering of incident so­ lar radiation and thus affect climate (31). Although sulfur may not play a major role in determining OH con­ centrations, OH and related a t m o ­ spheric oxidants probably do play major roles in controlling s u l f a t e aerosol formation. As these types of processes in the natural atmosphere are better understood, the effects of natural and anthropogenic emissions must be studied on both a local and a global basis. Eventually, the effects of future emission scenarios will be not only understood but also accu­ rately predicted. The location, times, and types of future emissions might be chosen in such a way as to mini­ mize t h e i r d e t r i m e n t a l effects or even optimize their positive effects on the environment. Although OH h a s l a r g e l y eluded m e a s u r e m e n t since its importance was recognized more t h a n two decades ago, contin­ ued advances in a number of technol ogies over the next decade will make its m e a s u r e m e n t not only possible but also well tested and available us­ ing a variety of different techniques. To t a k e the next few steps along the road to a better understanding of the natural tropospheric photochem­ ical process, several other measure­ ment advances are also required. Im­ p r o v e m e n t s m u s t be m a d e in our ability to m e a s u r e H 0 2 , which can act as a reservoir for OH and is also a strong atmospheric oxidant spe­ cies. Less emphasis has been placed on the measurement of H 0 2 than on OH and, as a result (despite its typi-

cally much higher atmospheric con­ centration), its accurate m e a s u r e ­ ment has also been elusive. Improved identification and quantification of the organic compounds p r e s e n t in the atmosphere (especially oxygen­ ated species) is required if the loss of OH and the production of organoperoxy compounds (commonly referred to as R0 2 ) are to be properly taken into account. This is not a simple problem, because the speciation of these compounds probably v a r i e s greatly with location. When OH measurements are made at highly polluted sites such as ur­ ban and i n d u s t r i a l a r e a s or a r e a s heavily affected by biomass burning, it is hard to say how much more dif­ ficult it will be to take accurate mea­ surements. It is quite possible, how­ ever, t h a t the measurement will be easier to perform t h a n to interpret. As air masses become highly inhomogeneous (chemically), air flows extremely complex, and surface ef­ fects far from negligible, the ability to measure OH may add little to our understanding of the photochemistry of this highly polluted environment. Continued improvement, not only of OH m e a s u r e m e n t technology b u t also of the ability to characterize the chemistry, dynamics, and history of an air mass, is necessary to meet our future goals of u n d e r s t a n d i n g and predicting the behavior of the n a t u ­ ral atmosphere and the effects of an­ thropogenic perturbations.

phys. Res. 1990, 95, 16427. (16) Hoell, J. M. NASA Conf. Pub. 2332, 1982. (17) Heaps, W. S.; McGee, T. J.J. Geophys. Res. 1985, 90, 7913. (18) Stimpfle, R. M.; Anderson, J. G. Geo­ phys. Res. Lett. 1988, 15, 1503. (19) Stimpfle, R. M.; Wennberg, P. O.; Lapson, L. B.; Anderson, J. G. Geophys. Res. Lett. 1990, 17, 1909. (20) Hard, T. M.; O'Brien, R. J.; Cook, T. B.; Tsongas, G. A. Appl. Opt. 1979, 18, 3216. (21) Crosley, D. R.; Hoell, J. M. NASA Conf. Pub. 2448, 1986. (22) Chan, C. Y.; Hard, Τ. Μ.; Mehrabzadeh, Α. Α.; et a l . / Geophys. Res. 1990, 95, 18569. (23) Bradshaw, J. D.; Rodgers, M. O.; Davis, D. D. Appl. Opt. 1984, 23, 2134. (24) Bradshaw, J. D.; Van Dijk, C. Mea­ surement of Atmospheric Gases, SPIE 1433 1991; Vol. 91. (25) Sandholm, S. T.; Bradshaw, J. D.; Dorris, K. S.; et a l . / Geophys. Res. 1990, 95 10155 (26)' Eisele, F. L.; Tanner, D. J. / Geophys. Res. 1991, 96, 9295. (27) Mount, G. H.; Eisele, F. L. Science 1992 256 1187 (28) Prinn,'R. G. Geophys. Res. Lett. 1985, 12, 597. (29) Prinn, R.; Cunnold, D.; Rasmussen, R.; et al. Science 1987, 238, 945. (30) Felton, C. C; Sheppard, J. C; Camp­ bell, M. V. Environ. Set. Technol. 1990, 24, 1841. (31) Charlson, R. J.; Schwartz, S. E.; Hales, J. M.; et al. Science 1992, 255, 423.

Fred L. Eisele (left) holds a joint appoint­ ment as principal research scientist at the Georgia Institute of Technology and as se­ nior research associate at the National Center for Atmospheric Research. He re­ ceived his B.S. degree in physics from Rensselaer Polytechnic Institute in 1970 and his Ph.D. in physics from the Univer­ sity of Vermont in 1975. He is currently developing sensitive selected-ion chemical ionization MS techniques for measuring trace atmospheric compounds. John D. Bradshaw is a principal re­ search scientist at the Georgia Institute of Technology. He received his Ph.D. in 1980 from the University of Florida, where he studied analytical applications ofLIF methods. His research interests in­ clude the development of field-based se­ quential multiphoton and photofragmen­ tation LIF sensors for measuring trace levels of compounds in the atmosphere.

...short of it.

References (1) Albritton, D. L.; Fehsenfeld, F. C ; Tuck, A. F. Science 1990, 250, 75. (2) Kolb, C. E. Rev. Geophys. 1991, 29 Sup­ plement, 25. (3) Logan, J. Α.; Prather, M. J.; McElroy, W. M. /. Geophys. Res. 1981, 86, 7210. (4) Atkinson, R. Chem. Rev. 1986, 86, 69. (5) Crosley, D. R. "SRI Conference Re­ port MP92-135"; SRI International: Menlo Park, CA, December 1992. (6) Mount, G. H.J. Geophys. Res. 1992, 97, 2427. (7) Hubler, G.; Perner, D.; Piatt, U.; Tonnissen, Α.; Ehhalt, D. H./. Geophys. Res. 1984, 89, 1309. (8) Armerding, W.; Herbert, Α.; Spiekermann, M.; Walter, J.; Comes, F. J. FreseniusZ. Anal. Chem. 1991, 340, 654. (9) Baardsen, E. L.; Terhune, R. W. Appl. Phys. Lett. 1972, 21, 209. (10) Davis, L. I.; Guo, C; James, J. V.; et al./ Geophys. Res. 1985, 90, 12835. (11) Rodgers, M. O.; Bradshaw, J. D.; Sandholm, S. T.; et al./. Geophys. Res. 1985, 90, 12819. (12) Beck, S. M.; Bendura, R. J.; McDougal, D. S.; et a l . / Geophys. Res. 1987, 92, 1977. (13) Copeland, R. Α.; Jeffries, J. B.; Cros­ ley, D. R. Chem. Phys. Lett. 1987, 138, 425. (14) Copeland, R. Α.; Wise, M. L.; Cros­ ley, D. R./ Phys. Chem. 1988, 92, 5710. (15) Smith, G. P.; Crosley, D. R.J. Geo­

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