@Article{TakahashiBaBuGoNaTsFu:1999:ReAiOH,
               author = "Takahashi, Hisao and Batista, Paulo Prado and Buriti, R. A. and 
                         Gobbi, Delano and Nakamura, T. and Tsuda, T. and Fukao, S",
                title = "Response of the airglow OH emission, temperature and mesopause 
                         wind to the atmospheric wave propagation over Shigaraki, Japan",
              journal = "Revista Eletr{\^o}nica da Faculdade de Farm{\'a}cia",
                 year = "1999",
               volume = "51",
               number = "7-8",
                pages = "863--875",
             keywords = "ASTROF{\'{\I}}SICA, aeroluminesc{\^e}ncia, radia{\c{c}}{\~a}o 
                         atmosf{\'e}rica, propaga{\c{c}}{\~a}o de ondas, mesopausa, 
                         airglow, atmospheric radiation, wave propagation, mesopause.",
             abstract = "Simultaneous observations of the night airglow OH (6, 2) band 
                         emission intensity and rotational temperature, by a sky scanning 
                         airglow spectrophotometer, and meteor winds, by a middle and upper 
                         atmosphere radar (MU radar), were carried out at Shigaraki (34.9 
                         degree N, 136.1 degree E), Japan, from October 29 to November 11, 
                         1994, as the first phase of a campaign, and from July 25 to July 
                         31, 1995 as the second phase. Horizontal structures in the OH 
                         emission intensity and rotational temperature were monitored 
                         optically, together with the background wind and its wave induced 
                         fluctuations, measured by MU radar. Since the MU radar makes a 
                         direct measurement of the vertical wavelength, and the OH 
                         spectrophotometer makes a direct measurement of the horizontal 
                         wavelength, the two techniques are mutually complementary to 
                         determine intrinsic wave parameters. Gravity waves with intrinsic 
                         periods of 2 to 9 hours, horizontal wavelengths of 500 to 3000 km 
                         and vertical wavelengths of 12 to 75 km were identified. Between 
                         the two different observation techniques, there is a reasonable 
                         agreement in the inferred wave characteristics.",
                 issn = "1808-0804",
                label = "9346",
           targetfile = "1999_takahashi.pdf",
        urlaccessdate = "02 maio 2024"
}