@Article{KumarSOGBRSC:2014:RaSaMo,
               author = "Kumar, G. Kishore and Singer, W. and Oberheide, J. and Grieger, N. 
                         and Batista, Paulo Prado and Riggin, D. M. and Schmidt, H. and 
                         Clemesha, Barclay Robert",
          affiliation = "Univ Rostock, Leibniz Inst Atmospher Phys eV, D-18225 
                         Kuhlungsborn, Germany. and Univ Rostock, Leibniz Inst Atmospher 
                         Phys eV, D-18225 Kuhlungsborn, Germany. and Clemson Univ, Dept 
                         Phys \& Astron, Clemson, SC 29634 USA. and Univ Rostock, Leibniz 
                         Inst Atmospher Phys eV, D-18225 Kuhlungsborn, Germany. and 
                         {Instituto Nacional de Pesquisas Espaciais (INPE)} and GATS Inc, 
                         Boulder, CO USA. and Max Planck Inst Meteorol, D-20146 Hamburg, 
                         Germany. and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
                title = "Diurnal tides at low latitudes: Radar, satellite, and model 
                         results",
              journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
                 year = "2014",
               volume = "118",
               number = "A, SI",
                pages = "96--105",
                month = "Oct.",
             keywords = "migrating and non-migrating tides, MLT, meteor radar, TIDI/TIMED, 
                         HAMMONIA.",
             abstract = "Mean winds and tidal signatures in the mesosphere and lower 
                         thermosphere (MLT) region are derived from meteor radar 
                         observations at three sites around 22 degrees S acquired in 2005. 
                         The observed differences of mean winds and tides are discussed in 
                         relation to the meteorological situation in the lower atmosphere 
                         and the possible generation of non-migrating tides. The 
                         longitudinally well separated radar sites allowed the evaluation 
                         of the migrating tidal component. The seasonal variation of 
                         signatures of the diurnal tide derived from ground-based radar 
                         observations, TIDI measurements aboard TIMED satellite, and model 
                         results obtained with HAMMONIA (Hamburg Model of the Neutral and 
                         Ionized Atmosphere) are compared. The ground-based, satellite, and 
                         model results of the total diurnal tide are in good agreement. The 
                         same is true for the migrating diurnal tide obtained from the 
                         radar observations, TIDI observations and from the model studies 
                         of HAMMONIA and GSVVM00 (Global Scale Wave Model).",
                  doi = "10.1016/j.jastp.2013.07.005",
                  url = "http://dx.doi.org/10.1016/j.jastp.2013.07.005",
                 issn = "1364-6826",
                label = "isi 2014-11 KumarSOGBRSC:2014:RaSaMo",
             language = "en",
           targetfile = "DEPOSITAR NA BIBLI 1-s2.0-S136468261300196X-main.pdf",
                  url = "http://dx.doi.org/10.1016/j.jastp.2013.07.005",
        urlaccessdate = "27 abr. 2024"
}