Author:
Kuhn J.R.,Bogart R.,Bush R.,Sá L.,Scherrer P.,Scheick X.
Abstract
The SoHO/MDI experiment generates a continous record of the solar limb brightness using 1.96″ pixels. Because there is no atmospheric blurring, these data allow measurements of solar limb brightness and shape changes with a precision that has not been achieved from the ground. The first results of a 1 month astrometric timeseries from the MDI solar structure program will be described here.
Publisher
Cambridge University Press (CUP)
Cited by
2 articles.
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