摘要: Structure and evolution of large scale photospheric and coronal magnetic fields in the interval 1976-1983 were studied using observations from the Stanford Solar Observatory and a potential field model. The solar wind in the helio... 展开
作者 | Hoeksema, J. T. | ||
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原报告号 | ADA144990 | 总页数 | 232 |
报告类别/文献类型 | AD / NTIS科技报告 | ||
关键词 | Magnetic fields Solar corona Solar cycle Solar wind Scintillation Solar observatories Photosphere Sun |