Comparison of H-alpha synoptic charts with the large-scale solar magnetic field as observed at Stanford

Details Comparison of H-alpha synoptic charts with the large-scale solar magnetic field as observed at Stanford Comparison of H-alpha synoptic charts with the large-scale solar magnetic field as observed at Stanford

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...55...63d&link_type=abstract

Solar Physics, vol. 55, Nov. 1977, p. 63-68. Research supported by the Max C. Fleischmann Foundation

Physics

17

H Alpha Line, Magnetic Field Configurations, Solar Magnetic Field, Astronomical Maps, Field Strength, Magnetic Effects, Magnetic Flux

Scientific paper

Two methods of observing the neutral line of the large-scale photospheric magnetic field are compared: neutral line positions inferred from H-alpha photographs (McIntosh and Nolte, 1975) and observations of the photospheric magnetic field made with low spatial resolution (three minutes) and high sensitivity using the Stanford magnetograph. The comparison is found to be very favorable.

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