Distribution of distances between bright nodes of the solar facula

Details Distribution of distances between bright nodes of the solar facula Distribution of distances between bright nodes of the solar facula

Sep 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974avest...8..177k&link_type=abstract

Astronomicheskii Vestnik, vol. 8, July-Sept. 1974, p. 177-181. In Russian.

Astronomy and Astrophysics

Astronomy

Faculae, Photosphere, Solar Atmosphere, Spatial Distribution, Spectroheliographs, Brightness, Maxima, Solar Flux Density, Statistical Distributions, Tables (Data)

Scientific paper

Photoheliograms obtained with a photospheric telescope are used to plot the distribution of all possible distances between the bright nodes of the facular area in the blue region of the spectrum (lambda = 410 millimicrons). The facular area is characterized by two parameters: the most probable least separation of nodes (= 17,000 km) and the period of alternation of the maxima in the distribution area (= 15,000). This can be explained by assuming that the nodes are located on the borders of cells with a radius of 15,000 km, preferably at the intersection of three neighboring cells.

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