Cite
How the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth -- An analytical model
MLA
Hofmeister, Stefan Johann, et al. How the Area of Solar Coronal Holes Affects the Properties of High-Speed Solar Wind Streams near Earth -- An Analytical Model. 2022. EBSCOhost, https://doi.org/10.1051/0004-6361/202141919.
APA
Hofmeister, S. J., Asvestari, E., Guo, J., Heidrich-Meisner, V., Heinemann, S. G., Magdalenic, J., Poedts, S., Samara, E., Temmer, M., Vennerstrom, S., Veronig, A., Vršnak, B., & Wimmer-Schweingruber, R. (2022). How the area of solar coronal holes affects the properties of high-speed solar wind streams near Earth -- An analytical model. https://doi.org/10.1051/0004-6361/202141919
Chicago
Hofmeister, Stefan Johann, Eleanna Asvestari, Jingnan Guo, Verena Heidrich-Meisner, Stephan G. Heinemann, Jasmina Magdalenic, Stefaan Poedts, et al. 2022. “How the Area of Solar Coronal Holes Affects the Properties of High-Speed Solar Wind Streams near Earth -- An Analytical Model.” doi:10.1051/0004-6361/202141919.