Coronal polar plumes
- Cite this article as:
- Newkirk, G. & Harvey, J. Sol Phys (1968) 3: 321. doi:10.1007/BF00155166
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There is some (although only weak) regularity in the projected spacing of plumes with a mean separation of ≈ 7 × 104 km.
The relation between plumes and various surface features is examined. Although little direct evidence can be assembled, we conclude that a direct connection exists between plumes and photospheric faculae, bright K3 faculae, and the small-scale magnetic structure present in the chromospheric network. It is hypothesized that plumes originate at the bright cores of the rosettes which lie along the chromospheric network. The distribution of magnetic field in the corona above a surface covered with idealized chromospheric network cells is calculated. The fact that the shape and size of the magnetic flux tubes originating from the rosette agrees with that of observed plumes supports the hypothesis.