Latitude and cycle variations of the photospheric network

Details Latitude and cycle variations of the photospheric network Latitude and cycle variations of the photospheric network

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..152..131m&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 152, no. 1, p. 131-137

Physics

14

Latitude, Network Analysis, Photosphere, Solar Cycles, Variability, Equatorial Regions, Polar Regions, Solar Magnetic Field

Scientific paper

New measurements of the number density of the Network Bright Points
confirm the variation of the density of the photospheric network at the
center of the disk during the solar cycle and that in the period
1983-1985, this number density (i.e. the magnetic flux in the quiet Sun)
was maximum, both at the poles and at the equator.

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