Methods of celestial mechanics

By Gerhard Beutler. 2005

184 citations recorded by the source corpus.

Subfields: Oceanography

View Paper: https://www.semanticscholar.org/paper/aa6dc259a42c628282576c9ab7af1000055756ed

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Oceanography

1. Oliver Montenbruck
2. Peter Steigenberger
3. Urs Hugentobler
4. Rolf Dach
5. J. Brockmann
6. E. Höck
7. P. Fridez
8. Mirko Reguzzoni

Citations in the corpus

• Bernese GNSS Software Version 5.2 (2015, methodology): “Dynamic force models are used to propagate the satellite’s center of mass position and velocity over time by means of numerical integration techniques (Beutler 2005).”
• Enhanced solar radiation pressure modeling for Galileo satellites (2015, background): “At a representative magnitude of 100 nm/s2, it introduces orbital perturbations at the level of 100 m over time scales of one orbital revolution (Beutler 2005; Fliegel and Gallini 1996).”
• First GOCE gravity field models derived by three different approaches (2011, methodology): “This model, comprising eight years of CHAMP data, has been computed with the so-called celestial mechanics approach (Beutler 2005; Beutler et al. 2010) and has a spatial resolution of about 200 km.”