@Article{TsurutaniHajrEcheLakh:2019:YiEtAl,
               author = "Tsurutani, Bruce T. and Hajra, Rajkumar and Echer, Ezequiel and 
                         Lakhina, Gurbax S.",
          affiliation = "{California Institute of Technology} and National Atmospheric 
                         Research Laboratory, Gadanki, India and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Indian Institute of 
                         Geomagnetism}",
                title = "Comment on “First observation of mesosphere response to the solar 
                         wind high\‐speed streams” by W. Yi et al",
              journal = "Journal of Geophysical Research: Space Physics",
                 year = "2019",
               volume = "124",
               number = "10",
                pages = "8165--8168",
                month = "Oct.",
             keywords = "HSS, Mesosphere, Chorus, wave-particle interaction.",
             abstract = "While Yi, Reid, Xue, Younger, Spargo, et al. (2017, ) described 
                         the observational results showing solar wind high-speed stream 
                         (HSS) impacts on the mesosphere over Antarctica, the specific 
                         physical mechanism behind them was not discussed. We discussed 
                         here how magnetospheric wave-particle interactions and energetic 
                         similar to 20- to 50-keV electron precipitation into the auroral 
                         zone atmosphere (diffuse auroras) during HSS intervals can cause 
                         the observed effects in the mesosphere.",
                  doi = "10.1029/2018JA026447",
                  url = "http://dx.doi.org/10.1029/2018JA026447",
                 issn = "2169-9402",
             language = "en",
           targetfile = "tsurutani_comment.pdf",
        urlaccessdate = "26 abr. 2024"
}