Solar Wind Speed Prediction via Graph Attention Network
Abstract The solar wind is a plasma flow formed by the expansion of the high‐temperature corona and propagates in the interplanetary space with speeds between 200 km/s and 900 km/s. Accurate solar wind speed prediction and longer lead time will help mitigate the impact of solar storms on aerospace e...
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| Main Authors: | Yanru Sun, Zongxia Xie, Haocheng Wang, Xin Huang, Qinghua Hu |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2022-07-01
|
| Series: | Space Weather |
| Subjects: | |
| Online Access: | https://doi.org/10.1029/2022SW003128 |
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