Zeeman splitting of the 61 gigahertz oxygen (O-2) line in the mesosphere

被引:13
作者
Hartmann, GK
Degenhardt, W
Richards, ML
Liebe, HJ
Hufford, GA
Cotton, MG
Bevilacqua, RM
Olivero, JJ
Kampfer, N
Langen, J
机构
[1] NATL TELECOMMUN & INFORMAT ADM,INST TELECOMMUN SCI,BOULDER,CO 80303
[2] USN,RES LAB,WASHINGTON,DC 20375
[3] EMBRY RIDDLE AERONAUT UNIV,DEPT PHYS SCI,DAYTONA BEACH,FL 32114
[4] UNIV BERN,IAP,CH-3012 BERN,SWITZERLAND
[5] UNIV BREMEN,IUP,D-28334 BREMEN,GERMANY
关键词
D O I
10.1029/96GL01043
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Zeeman splitting of O-2 molecular states in the Earth's upper atmosphere leads to polarized emission spectra. A 61 GHz radiometer operated as part of tile Millimeter-wave Atmospheric Sounder (MAS), a core payload instrument of the NASA Space Shuttle ATLAS missions, observed such emissions. This instruments high resolution spectrometer (200 kHz) allows us to verify for tile first time Zeeman effect model calculations for the upper atmosphere in some detail. The results suggest some interesting new aspects for the research of the upper atmosphere.
引用
收藏
页码:2329 / 2332
页数:4
相关论文
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