摘要
本文利用ＳｏｌａｒＭｅｓｏｓｐｈｅｒｅＥｘｐｌｏｒｅｅｒ（ＳＭＥ）卫星１９８２年和１９８３年太阳紫外辐射和赤道地区５０－９０ｋｍ臭氧分布的红外观测资料，对臭氧对太阳紫外辐射２７天振荡的响应进行了研究，并且利用大气光化波动模式对其进行了理论计算，计算结果与实测结果基本一致．
A series of studies are preformed concerning the response of mesospheric ozone to the 27-day solar ultlaviolet variations. The studies are bed on SME 1982--1983 solar ultraviolet data and 50--90km equatorial infrared ozone data. A theoretical computation is presented by using atmospheric photochemical wave model. The calculated result is nearly in agreement with that of observations.
出处
《空间科学学报》
CAS
CSCD
北大核心
1996年第2期145-151,共7页
Chinese Journal of Space Science
基金
国家自然科学基金
