Finding the repeat times of the GPS constellation
By Duncan Carr Agnew, Kristine M. Larson. 2006
204 citations recorded by the source corpus.
Subfields: Aerospace Engineering, Oceanography
View Paper: https://www.semanticscholar.org/paper/fddf52105eeb888cff6e261a37e1bbdb20f6128c
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Aerospace Engineering
- Alireza Amiri-Simkooei
- Xavier Collilieux
- Z. Altamimi
- Tonie Van Dam
- Jim Ray
- Matt A. King
- Christopher Stephen Watson
- Peter Steigenberger
In Oceanography
- Alireza Amiri-Simkooei
- Xavier Collilieux
- Z. Altamimi
- Tonie Van Dam
- Jim Ray
- Matt A. King
- Christopher Stephen Watson
- Peter Steigenberger
Citations in the corpus
- Long GPS coordinate time series: Multipath and geometry effects (2009, methodology): “…[ 24 ] In order to provide a non time variable reference orbit, we adopted an artificial configuration that used a fixed 24 satellite constellation, each with a fixed orbit repeat period of 24 h minus 246 s, close to the average GPS satellite orbital repeat time [ Agnew and Larson , 2007].”
- On the nature of GPS draconitic year periodic pattern in multivariate position time series (2013, background): “However, the repeat time of the GPS constellation has an average value over the day corresponding to a daily advance of 246.8 s [Agnew and Larson, 2007].”
- Anomalous harmonics in the spectra of GPS position estimates (2008, methodology): “8 s, which aliases to the same period of about 350 days for the standard 24-hour sampling used by the IGS (Agnew and Larson, 2007). Any local directiondependent observational biases, such as due to multipath, could be expected to show up with a 350-day repeat period. Since high-frequency multipath v”
- Characterization of periodic variations in the GPS satellite clocks (2008, background): “(2007) confirm the suspected significance of systematic once-per-revolution orbital errors and demonstrate that those are largest during eclipse seasons when the satellites in a given orbital plane pass through the Earth’s shadow twice daily (For reference, Agnew and Larson (2007) report an average ”