Please use this identifier to cite or link to this item:
http://library.iigm.res.in:8080/xmlui/handle/123456798/65| Title: | Comment on “First Observation of Mesosphere Response to the Solar Wind High‐Speed Streams” by W. Yi et al. |
| Authors: | Lakhina, G S |
| Issue Date: | 2019 |
| Citation: | Journal of Geophysical Research – Space Physics, 124, doi: 10.1029/2018JA026447 |
| 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. |
| URI: | http://library.iigm.res.in:8080/xmlui/handle/123456798/65 |
| Appears in Collections: | UAS_Reprints |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| LakhinaGS_etal_JGR_2019.pdf | 268.5 kB | Adobe PDF | View/Open |
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