Calculations using general relativity determined that the clocks on GPS satellites would be seen by Earth's observers to run 38 microseconds faster per day, and this was corrected for in the design of GPS
Consisted of the United States Navy's submarine-launched ballistic missiles (SLBMs), United States Air Force (USAF) strategic bombers and intercontinental ballistic missiles (ICBMs)
Decades later, during the early years of GPS, civiliansurveying became one of the first fields to make use of the new technology, because surveyors could reap benefits of signals from the less-than-complete GPS constellation years before it was declared operational
In January 1966, a World Geodetic System Committee composed of representatives from the Army, Navy, and Air Force was established to develop a new World Geodetic System
1. In January 1966, a World Geodetic System Committee composed of representatives from the United States Army, Navy and Air Force, was charged with the responsibility of developing an improved WGS
2. Large amounts of Doppler and optical satellite data had become available since the development of WGS60
3. Using the additional data and improved techniques, WGS 66 was produced which served DoD needs for about five years after its implementation in 1967
Originally designed to meet the Navy's requirement for locating ballistic missile submarines and other ships at the ocean's surface, Transit was made available to civilian users in 1967
Researchers at the Applied Physics Laboratory (APL) discovered that measurements of the Doppler shift as the satellite passed by were adequate to determine the entire satellite orbit
Dr. Frank T.McClure of APL noted that conversely, if the satellite orbit were known, position on the earth could be determined using these same Doppler measurements
1. Selected satellite, surface gravity and astrogeodetic data available through 1972 from both DoD and non-DoD sources were used in a Unified WGS Solution (a large scale least squares adjustment)
2. The results of the adjustment consisted of corrections to initial station coordinates and coefficients of the gravitational field