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Seismic imaging of the Sun's far hemisphere and its applications in space weather forecasting
The interior of the Sun is filled acoustic waves with periods of about 5 min. These waves, called “p modes,” are understood to be excited by convection in a thin layer beneath the Sun's surface. The p modes cause seismic ripples, which we call “the solar oscillations.” Helioseismic observatorie...
| Autores principales: | , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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John Wiley and Sons Inc.
2017
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5784405/ https://www.ncbi.nlm.nih.gov/pubmed/29398984 http://dx.doi.org/10.1002/2016SW001547 |