The wavelength dependence of granulation /0.38-2.4 microns/

Details The wavelength dependence of granulation /0.38-2.4 microns/ The wavelength dependence of granulation /0.38-2.4 microns/

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...54...31a&link_type=abstract

Solar Physics, vol. 54, Sept. 1977, p. 31-33.

Physics

6

Luminous Intensity, Solar Granulation, Wavelengths, Solar Physics, Statistical Analysis, Stellar Luminosity

Scientific paper

Using two pinhole photometers the intensity of the undisturbed photosphere was recorded simultaneously in six and in four wavelength regions. The rms value of the intensity variation in each of the 10 wavelength regions decreases slightly with increasing value of the heliocentric angle; this result confirms recent observations by other authors and supports the critique of the results given by Edmonds (1964). The detection of a secondary maximum in the wavelength dependence of the intensity variation at 1.5 microns is reported.

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