Comment on “First Observation of Mesosphere Response to the Solar Wind High‐Speed Streams” by W. Yi et al.

dc.contributor.author	Lakhina, G S
dc.date.accessioned	2021-08-03T08:26:36Z
dc.date.available	2021-08-03T08:26:36Z
dc.date.issued	2019
dc.identifier.citation	Journal of Geophysical Research – Space Physics, 124, doi: 10.1029/2018JA026447	en_US
dc.identifier.uri	http://library.iigm.res.in:8080/xmlui/handle/123456798/65
dc.description.abstract	While Yi, Reid, Xue, Younger, Spargo, et al. (2017, http://doi:10.1002/2017JA024446) 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 ~20‐ to 50‐keV electron precipitation into the auroral zone atmosphere (diffuse auroras) during HSS intervals can cause the observed effects in the mesosphere.	en_US
dc.title	Comment on “First Observation of Mesosphere Response to the Solar Wind High‐Speed Streams” by W. Yi et al.	en_US
dc.type	Article	en_US