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149. " Ackerman, M. (1974). Planet. Space Sei. " Ackerman, M. (1975). Aeronom. Acta No. 142, "NO, N0 2 , and HNOg below 35 km in the Atmosphere. , and Muller, C. (1973). PureAppl. Geophy. , Fontaneila, J. , and Louisnard, N. (1973). , Fontaneila, J. , and Louisnard, N. (1974). Can. J. Chem. , Fontanella, J. , and Müller, C. (1975). Planet. Space Sei. " Anderson, J. G. (1971). J. Geophys. Res. " Bainbridge, A. , and Heidt, L. E. (1966). " Baker, K. , Bishop, R. , and Megill, L. R. (1974). J. Geophys.

1961). Infrared Phys. , and Junge, C. (1969). , and Warneck, P. (1972). J. Geophys. Res. " Shardanand. (1969). Phys. Rev. " Smith, H. J. (1954). Astrophys. J. 119, 438, "The Physical Theory of Meteors. V. " Theon, J. , and Smith, W. S. (1971). In "Mesospheric Models and Related Experi- 50 I. STRUCTURE OF THE A T M O S P H E R E ments" (G. ), p. 131. " Thomas, R. N. (1952). Astrophys, J. 116, 203, "The Physical Theory of Meteors. III. " Thomas, R. , and Whipple, F. L. (1951). Astrophys, J. 114,448, "The Physical Theory of Meteors.

Ranges of data are shown for each date, and authors' uncertainty for a single measurement is shown as a double arrow. R* Ridley et al. (1974), aircraft 9-34° N, afternoon IX 73, and 65^75° N, polar low sun XI 73, chemiluminescence. Range of data is shown. SL Savage et al. (1974), aircraft 25-49° N, midday XI 73-V 74, chemiluminescence. ixHiii 10" Particle»/cm3 Fig. I'll. Semilog plots of estimated concentrations of the oxides of nitrogen versus altitude for an overhead sun. and Fontanella et al.

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