The calcium K-line network in coronal holes

Details The calcium K-line network in coronal holes The calcium K-line network in coronal holes

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...52..343m&link_type=abstract

Solar Physics, vol. 52, May 1977, p. 343-348.

Physics

3

Chromosphere, K Lines, Solar Corona, Stellar Spectrophotometry, Calcium, Data Reduction, Far Ultraviolet Radiation, Histograms, Magnetic Field Configurations, Magnetic Flux, Spectroheliographs

Scientific paper

Microphotometry of calcium K-line photographs in the regions of polar coronal holes shows that the chromospheric network exterior to a hole has a slightly broader intensity distribution than that inside the hole itself, a fact which can be attributed to a greater number of bright network elements outside the hole. These bright elements presumably represent the enhanced network resulting from the dispersal of magnetic flux from old active regions, a hypothesis which is consistent with current ideas of coronal-hole formation.

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