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- W2007023863 abstract "The configuration of sunspot magnetic fields is deduced by using the observational data on the development of type IV radio bursts and Hα-brightening areas over the umbrae of sunspot groups. Since both polarity areas are existent together within the same umbrae, the magnetically neutral regions are usually produced along the areas separating the one polarity area from the other. In the eastern portion of the preceding sunspots, the gradient of sunspot magnetic fields is much steeper compared to all other portions and thus solar proton flares are triggered within or very near this portion. Hα-brightening areas develop mainly above the preceding sunspots and their eastern portion of sunspot groups. This tendency seems to be closely related to the configuration of sunspot magnetic fields and the mechanism of solar proton flares." @default.
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- W2007023863 title "On the magnetic configuration of sunspot groups which produce solar proton flares" @default.
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- W2007023863 doi "https://doi.org/10.1016/0032-0633(70)90065-6" @default.
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