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Electron temperature of the solar wind
Solar wind provides an example of a weakly collisional plasma expanding from a thermal source in the presence of spatially diverging magnetic-field lines. Observations show that in the inner heliosphere, the electron temperature declines with the distance approximately as [Formula: see text] , which...
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| Publicado no: | Proc Natl Acad Sci U S A |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
National Academy of Sciences
2020
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7196822/ https://ncbi.nlm.nih.gov/pubmed/32291339 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1917905117 |
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