טוען...
The multi-scale nature of the solar wind
The solar wind is a magnetized plasma and as such exhibits collective plasma behavior associated with its characteristic spatial and temporal scales. The characteristic length scales include the size of the heliosphere, the collisional mean free paths of all species, their inertial lengths, their gy...
שמור ב:
| הוצא לאור ב: | Living Rev Sol Phys |
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| Main Authors: | , , |
| פורמט: | Artigo |
| שפה: | Inglês |
| יצא לאור: |
Springer International Publishing
2019
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| נושאים: | |
| גישה מקוונת: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6934245/ https://ncbi.nlm.nih.gov/pubmed/31929769 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1007/s41116-019-0021-0 |
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