public final class ReferencePointsDisplacement extends Object
Computes the displacement of reference points due to the effect of the solid Earth tides.
Modifier and Type | Method and Description |
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static Vector3D |
poleTidesCorrections(AbsoluteDate date,
Vector3D point)
Computes the displacement of reference points due to the effect of the pole tides.
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static Vector3D |
solidEarthTidesCorrections(AbsoluteDate date,
Vector3D point,
Vector3D sun,
Vector3D moon)
Computes the displacement of reference points due to the effect of the solid Earth tides.
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public static Vector3D solidEarthTidesCorrections(AbsoluteDate date, Vector3D point, Vector3D sun, Vector3D moon) throws PatriusException
See IERS conventions 2010, chapter 7, section 7.1.1 "Effects of the solid Earth tides" ftp://tai.bipm.org/iers/conv2010/chapter7/tn36_c7.pdf
date
- date of computation in UTCpoint
- geocentric position of the point (in ITRF Frame)sun
- geocentric position of the sun (in ITRF Frame)moon
- geocentric position of the moon (in ITRF Frame)PatriusException
- if some data cannot be read or if some
file content is corruptedpublic static Vector3D poleTidesCorrections(AbsoluteDate date, Vector3D point) throws PatriusException
See IERS conventions 2010, chapter 7, section 7.1.4 "Rotational deformation due to polar motion: Secular polar motion and the pole tide" ftp://tai.bipm.org/iers/conv2010/chapter7/tn36_c7.pdf
date
- date of computation in UTCpoint
- geocentric position of the point (in ITRF Frame)PatriusException
- thrown if pole computation failedCopyright © 2023 CNES. All rights reserved.