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Oblique and rippled heliosphere structures from the Interstellar Boundary Explorer

Past analysis has shown that the heliosphere structure can be deduced from correlations between long-scale solar wind pressure evolution and energetic neutral atom emissions. However, this required spatial and temporal averaging that smoothed out small or dynamic features of the heliosphere. In late...

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Detalles Bibliográficos
Autores principales: Zirnstein, Eric J., Shrestha, Bishwas L., McComas, David J., Dayeh, Maher A., Heerikhuisen, Jacob, Reisenfeld, Daniel B., Sokół, Justyna M., Swaczyna, Paweł
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9744672/
https://www.ncbi.nlm.nih.gov/pubmed/36531130
http://dx.doi.org/10.1038/s41550-022-01798-6

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