Lauren James

Apr 24, 2023 | agupubs.onlinelibrary.wiley.com | Lauren James |Christopher Scott |Luke Barnard |Mathew J. Owens

Modeling the Solar Wind Speed: BRaVDA or MAS? Earlier in Section 2.1, we explored the difference in the solar wind structure near Earth for CR2077 where by HUXt propagated inner boundary speed conditions from MAS and BRaVDA. In summary, it was found that the data assimilated scheme was better at recreating the speed structures observed by ACE, especially for the duration and maximum speed of fast streams.