Jno2 at high solar zenith angles in the lower stratosphere

被引:5
作者
Gao, RS
Del Negro, LA
Swartz, WH
Salawitch, RJ
Lloyd, SA
Proffitt, MH
Fahey, DW
Donnelly, SG
Neuman, JA
Stimpfle, RM
Bui, TP
机构
[1] NOAA, Aeron Lab, Boulder, CO 80305 USA
[2] Middlebury Coll, Dept Chem & Biochem, Middlebury, VT 05753 USA
[3] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[4] Univ Maryland, Dept Chem & Biochem, College Pk, MD 20742 USA
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] Univ Colorado, Cooperat Inst Res Environm Sci, Boulder, CO 80309 USA
[7] Natl Ctr Atmospher Res, Boulder, CO 80303 USA
[8] Harvard Univ, Dept Chem, Cambridge, MA 02138 USA
[9] NASA, Ames Res Ctr, Moffett Field, CA 94305 USA
关键词
D O I
10.1029/2000GL012615
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
In situ measurements of NO, NO2, O-3, HO2, ClO, pressure, and temperature have been made at high solar zenith angles (SZA, 70 degrees - 93 degrees) in the lower stratosphere. These measurements are used to derive the photolysis rate of NO2, J(NO2),, using a time-dependent method. The resultant J(NO2) values and the results of a multiple-scattering actinic flux model show a linear relationship throughout the SZA range. The difference of the two sets of J(NO2) values of about 11% suggests that the model scattering calculation is very accurate at high SZA conditions near sunrise and sunset.
引用
收藏
页码:2405 / 2408
页数:4
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