Atomic Oxygen 630 nm and OH Airglows at Mt. Haleakala, Hawaii in February and November 1993

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著者

    • KITA K.
    • Department of Earth and Planetary Physics, Graduate School of Science, University of Tokyo
    • IWAGAMI N.
    • Department of Earth and Planetary Physics, Graduate School of Science, University of Tokyo
    • OGAWA T.
    • Department of Earth and Planetary Physics, Graduate School of Science, University of Tokyo

抄録

Temporal variations of the all-sky distribution of atomic oxygen 630 nm airglow intensity were observedatMt. Haleakala in Maui Island, Hawaii, to obtain informationonthe dynamics of <I>F</I> region plasma in the equatorial anomaly region. All-sky intensity distribution of the hydroxyl OH(7, 2) band airglow originating from the mesopause region was simultaneously observed to seek any relationship between the dynamical variations of <I>F</I> region plasma and the disturbance in the lower atmosphere. The results of our preliminary analyses of the data obtained in February and November 1993 show that there is no definite correlation in the patterns of all-sky intensity distribution between atomic oxygen 630 nm and OH(7, 2) band airglows in both geomagnetically disturbed and quiet nights. The all-sky intensity pattern of 630 nm is found to be modified during a geomagnetic storm, while that of OH(7, 2) band varies independently of geomagnetic activity.

収録刊行物

  • Journal of geomagnetism and geoelectricity  

    Journal of geomagnetism and geoelectricity 48(3), 337-341, 1996-03 

    Society of Geomagnetism and Earth, Planetary and Space Sciences

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各種コード

  • NII論文ID(NAID)
    10002028817
  • NII書誌ID(NCID)
    AA00698879
  • 本文言語コード
    ENG
  • 資料種別
    ART
  • ISSN
    00221392
  • データ提供元
    CJP書誌  CJP引用  J-STAGE 
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