Closed magnetic structures in the chromosphere and in the transition region

Details Closed magnetic structures in the chromosphere and in the transition region Closed magnetic structures in the chromosphere and in the transition region

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..112..233m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 112, no. 2, 1987, p. 233-253.

Physics

5

Chromosphere, Density Wave Model, H Alpha Line, Magnetic Field Configurations, Solar Oscillations, Transition Points, Carbon, Solar Limb

Scientific paper

Using simultaneous observations of the same solar regions in the lines Hα and C IV 1548 Å, the authors have derived schematic models of closed magnetic lines from dynamical constraints. They conclude that the magnetic loops are closed at higher levels above facular than above non-facular regions. This result remains valid whatever the assumed density models are, even by taking into account the 3 min oscillations. The center-to-limb behaviour is well predicted by taking into account the relative opacity in the chromosphere and transition region.

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