Statistical properties of solar granulation derived from the SOUP instrument on Spacelab 2

Details Statistical properties of solar granulation derived from the SOUP instrument on Spacelab 2 Statistical properties of solar granulation derived from the SOUP instrument on Spacelab 2

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...336..475t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 336, Jan. 1, 1989, p. 475-494.

Astronomy and Astrophysics

Astrophysics

244

Solar Atmosphere, Solar Granulation, Solar Oscillations, Spacelab, Statistical Analysis, Earth Atmosphere, Image Processing, Root-Mean-Square Errors, Solar Magnetic Field

Scientific paper

Computer algorithms and statistical techniques were used to identify, measure, and quantify the properties of solar granulation derived from movies collected by the Solar Optical Universal Polarimeter on Spacelab 2. The results show that there is neither a typical solar granule nor a typical granule evolution. A granule's evolution is dependent on local magnetic flux density, its position with respect to the active region plage, its position in the mesogranulation pattern, and the evolution of granules in its immediate neighborhood.

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