Eclipse radius measurementsMethods for predicting the path edges and reducing observations of total solar eclipses for determining variations of the solar radius are described. Analyzed observations of the 1925 January eclipse show a 0.7 (arc second) decrease in the solar radius during the past fifty years.
Document ID
19820009151
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Dunham, D. W. (Computer Sciences Corp. Greenbelt, MD, United States)