Twilight observations suggest unknown sources of HOx

被引:79
作者
Wennberg, PO
Salawitch, RJ
Donaldson, DJ
Hanisco, TF
Lanzendorf, EJ
Perkins, KK
Lloyd, SA
Vaida, V
Gao, RS
Hintsa, EJ
Cohen, RC
Swartz, WH
Kusterer, TL
Anderson, DE
机构
[1] CALTECH, Pasadena, CA 91125 USA
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Harvard Univ, Dept Chem, Cambridge, MA 02138 USA
[4] Univ Toronto, Dept Chem, Toronto, ON M5S 1A1, Canada
[5] Univ Colorado, Dept Chem, Boulder, CO 80309 USA
[6] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[7] NOAA, Aeron Lab, Boulder, CO 80307 USA
[8] Univ Calif Berkeley, Berkeley, CA 94720 USA
关键词
D O I
10.1029/1999GL900255
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Measurements of the concentrations of OH and HO2 (HOx) in the high-latitude lower stratosphere imply the existence of unknown photolytic sources of HOx. The strength of the additional HOx source required to match the observations depends only weakly on solar zenith angle (SZA) for 80 degrees < SZA < 93 degrees. The wavelengths responsible for producing this HOx must be longer than 650 nm because the flux at shorter wavelengths is significantly attenuated at high SZA by scattering and absorption. Provided that the sources involve only a single photon, the strength of the bonds being broken must be <45 kcal mole(-1). We speculate that peroxynitric acid (HNO4) dissociates after excitation to an unknown excited state with an integrated band cross section of 2-3 x 10(-20) cm(2) molecule(-1) nm (650 < lambda < 1250 nm).
引用
收藏
页码:1373 / 1376
页数:4
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