Measurement of the Solar Limb Brightness Profile at 3 MM During the Total Eclipse of 1991 July 11

Astronomy and Astrophysics – Astronomy

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Scientific paper

We observed the solar limb at the point of first contact during the eclipse of 1991 July 11, with a spatial resolution ~ 1.6''. The observations were carried out at the Owens Valley Radio Observatory millimeter interferometer, operating at 3 millimeters. The visibility amplitude and phase were modeled to yield the height of the 3 mm limb above the visible photosphere, and the data were differentiated to yield the brightness profile of the limb in strips ~ 1.6'' wide. We found that the 3 mm limb extends 7.5+/-0.8'' or 5500 km above the visible photosphere, with no evidence of a limb spike. This result, and the overall shape of the limb profile, are similar to the interferometric results of Wannier, Hurford, & Seielstad (1983) obtained with the same intrument but without the benefit of an eclipse. The 3 mm limb, at a temperature of ~ 7200 K, extends to altitudes far beyond the expected location of the transition region in the model of Vernazza, Avrett, & Loeser (1981). A comparison of the 3 mm profile and an offband Hα photograph of the limb reveals a close correspondence between the 3 mm limb and the height of Hα spicules.

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