Statistics – Computation
Scientific paper
Mar 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..124...15a&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 124, no. 1, 1989, p. 15-22.
Statistics
Computation
7
Benard Cells, Magnetic Flux, Optical Thickness, Photosphere, Solar Atmosphere, Solar Granulation, Abundance, Computational Astrophysics, Infrared Scanners, Iterative Solution, Limb Darkening, Temperature Distribution
Scientific paper
Conventional wisdom dictates that the 1.642-micron H(-) opacity minimum is the best window to the depths of the solar photosphere. However, the violet continuum near 0.4 micron exhibits a larger intensity response to small thermal perturbations at depth, and thus might offer an even better view of the subsurface roots of granulation cells and magnetic flux tubes.
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