Charles C. Counselman

TL;DR: In this paper, the authors proposed a method of ambiguity resolution for short-baseline interferometric observations of GPS, which is suitable for observations made with antennas of low directive gain.

TL;DR: The Pioneer Venus data relevant to the dynamics and thermodynamics of the atmosphere is summarized and interpreted in this paper, where the authors summarize and interpret the Pioneer Venus observations relevant to both the day and night side.

TL;DR: In this paper, an analysis of 1389 measurements, accumulated between 1970 and 1974 of echo delays of laser signals transmitted from Earth and reflected from cube corners on the Moon show gravitational binding energy to contribute equally to Earth's inertial and passive gravitational masses to within the estimated uncertainty of 1.5%.

TL;DR: The results of the Pioneer Venus differential long-baseline interferometry experiment are presented in this article, where the velocity component of the probes as they fell to the surface of Venus was calculated from the Doppler shift of the received signal, and the other two orthogonal components were determined by long baseline interferences.

TL;DR: The Mark III very-long-baseline interferometry (VLBI) system allows recording and later processing of up to 112 megabits per second from each radio telescope of an interferometer array, which allows detection and study of compact sources with flux densities under 1 millijansky.