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Autor:
Kalman J. Knizhnik, Micah J. Weberg, Ajeet Singh Zaveri, Ignacio Ugarte-Urra, Yi-Ming Wang, Lisa A. Upton, Elena Provornikova
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 154 (2024)
A significant challenge facing heliospheric models is the lack of full Sun observational coverage. The lack of information about the farside photospheric magnetic field necessitates the use of various techniques to approximate the structure and appea
Externí odkaz:
https://doaj.org/article/f9044aa541794dbeb205b729c5d0b9ee
