Modeling mesogranules and exploders on the solar surface

Details Modeling mesogranules and exploders on the solar surface Modeling mesogranules and exploders on the solar surface

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...375..775s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 375, July 10, 1991, p. 775-788. Research supported by SERC, USAF, and Lockh

Astronomy and Astrophysics

Astrophysics

42

Kinematic Equations, Normal Density Functions, Solar Granulation, Solar Magnetic Field, Steady Flow, Stellar Models

Scientific paper

Radial outflows in exploders and mesogranules can be modeled by superposing Gaussian source functions. This model is used to explore the relationship between mesogranules and exploders. Although it is demonstarted that there is a mathematical equivalence between mesogranules and exploders distributed normally about the mesogranule centers, the results indicate that the observed mesogranular velocity pattern is not consistent with a flow pattern generated by exploders dropped randomly on the solar surface. Detailed comparisons with observations suggest that the averaged mesogranular velocity is produced by a combination of a persistent outflow from a source together with exploders distributed randomly about its center. Similar analysis also shows supergranules are not the result of random occurrences of mesogranules.

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