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...

Descripción completa

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:
Article
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

Internet

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

Ejemplares similares