@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 = "27 abr. 2024"
}