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Observations of the 1991 Eclipse at 3.5 mm Wavelength

Published online by Cambridge University Press:  03 August 2017

S. M. White  and
M. R. Kundu
S. M. White
Affiliation:
Department of Astronomy, University of Maryland, College Park, MD 20742, U.S.A.
M. R. Kundu
Affiliation:
Department of Astronomy, University of Maryland, College Park, MD 20742, U.S.A.

Abstract

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We report preliminary results of the partial eclipse seen from the BIMA millimeter–wavelength interferometer in northern California. The use of an interferometer has many advantages over previous single–dish eclipse observations at 3 mm, and in particular it allows a quite different type of measurement of the height of the “3-mm limb” which is direct and precise: we find it to be 11.9″ ± 0.4″ above the optical limb.

Keywords

eclipsestechniques: interferometricSun: radio radiation
Type
Part 2: Infrared Observations of the 1991 Total Solar Eclipse
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 167 - 172
Copyright
Copyright © Kluwer 1994 

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