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- W1617375897 abstract "Quiescent prominences are associated with neutral lines in the vertical component of the photospheric magnetic field. Three distinct classes may be distinguished (Leroy, 1978) namely: polar crown prominences, those above a bipolar region neutral line and those between two different bipolar regions. It is reasonable to expect differences in the process of formation and resulting structure between these three classes." @default.
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- W1617375897 date "1979-01-01" @default.
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- W1617375897 title "A Magnetic Field Reconnection Model of Quiescent Solar Prominences" @default.
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- W1617375897 doi "https://doi.org/10.1017/s0252921100065404" @default.
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