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Anomalously weak solar convection
Convection in the solar interior is thought to comprise structures on a spectrum of scales. This conclusion emerges from phenomenological studies and numerical simulations, though neither covers the proper range of dynamical parameters of solar convection. Here, we analyze observations of the wavefi...
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| Hlavní autoři: | , , |
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| Médium: | Artigo |
| Jazyk: | Inglês |
| Vydáno: |
National Academy of Sciences
2012
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| Témata: | |
| On-line přístup: | https://ncbi.nlm.nih.gov/pmc/articles/PMC3409726/ https://ncbi.nlm.nih.gov/pubmed/22665774 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1073/pnas.1206570109 |
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