White light network in the solar photosphere

Details White light network in the solar photosphere White light network in the solar photosphere

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...39..297l&link_type=abstract

Solar Physics, vol. 39, Dec. 1974, p. 297-300.

Physics

4

Astronomical Photography, Light (Visible Radiation), Photosphere, Solar Atmosphere, Faculae, Solar Granulation, Sunspots, Time Response, Velocity Distribution

Scientific paper

Time-averaging technique is performed on a set of white-light pictures obtained at mu = 0.87. After eliminating short-lived granulations, the time-averaged pictures show some large-scale but long-lived brightness patterns which are not recognizable in any of the single-frame snapshots. The patterns are brighter than the background and are co-spatial with the upper photospheric emissions and magnetic fields. These patterns are defined as the white-light network.

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