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- W2026591736 abstract "Abstract Using the potential field model, we have calculated the magnetic structure of the coronal condensation, which appeared on the east limb of the solar disk at the 22 September 1968 eclipse. The comparison between calculated magnetic field geometry and observed contour of the coronal condensation shows general agreement. From this analysis, we see that the magnetic field extending to the lower coronal region is approximately the potential field during the steady period of an active region. The observed contour of the coronal condensation may be considered as the projection of the magnetic tubes of the active region on the plane perpendicular to the line of sight. The matter flows along the magnetic field lines." @default.
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- W2026591736 date "1978-12-01" @default.
- W2026591736 modified "2023-09-26" @default.
- W2026591736 title "Magnetic fields in a coronal condensation" @default.
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- W2026591736 doi "https://doi.org/10.1016/0146-6364(78)90019-1" @default.
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