Publication Date:
2016-06-07
Description:
Very long baseline interferometry observations made with a 3900 km baseline interferometer (Haystack Observatory in Massachusetts to Owens Valley Observation in California) were used to estimate changes in the X-component of the position of the Earth's pole and in UT1. These estimates are compared with corresponding ones from lunar laser ranging, satellite laser ranging, satellite Doppler, and stellar observations.
Keywords:
EARTH RESOURCES AND REMOTE SENSING
Type:
Radio Interferometry; p 33-44
Format:
application/pdf