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Earth Rotation Observed by Very Long Baseline Interferometry and Ring Laser

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Abstract

We present a systematic and unified treatment of Earth rotation from the geodetic, astronomical, and geophysical point of view. A precise terminology of precession-nutation and polar motion is of great importance for understanding the interacting physical phenomena leading to rotational irregularities of the Earth. In total, four poles of the equatorial plane are defined for the description of Earth rotation. The various components of the Earth Orientation Parameters, i.e., precession-nutation, polar motion, and universal time (or length of day) are summarized. This paper shows how very long baseline interferometry and ring laser differ in terms of Earth rotation and presents the current state-of-the-art measurement accuracy that can be achieved.

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Abbreviations

CIP:

Celestial Intermediate Pole

e-VLBI:

Electronic VLBI

ENSO:

El Niño Southern Oscillation

EOP:

Earth Orientation Parameters

FCN:

Free Core Nutation

FICN:

Free Inner Core Nutation

GCRF:

Geocentric Celestial Reference Frame

GPS:

Global Positioning System

IAG:

International Association of Geodesy

IAU:

International Astronomical Union

IERS:

International Earth rotation and Reference system Service

IRP:

Instantaneous Rotation Pole

IRV:

Instantaneous Rotation Vector

ITRF:

International Terrestrial Reference Frame

LOD:

Length of day

MJD:

Modified Julian Date

MJO:

Madden-Julian Oscillation

NDFW:

Nearly Diurnal Free Wobble

PM:

Polar motion

PN:

Precession-nutation

SG:

Superconducting gravimeter

UT1:

Universal Time

UTC:

Universal Time Coordinated

VLBI:

Very Long Baseline Interferometry

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Correspondence to P. J. Mendes Cerveira.

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Mendes Cerveira, P.J., Boehm, J., Schuh, H. et al. Earth Rotation Observed by Very Long Baseline Interferometry and Ring Laser. Pure appl. geophys. 166, 1499–1517 (2009). https://doi.org/10.1007/s00024-004-0487-z

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  • DOI: https://doi.org/10.1007/s00024-004-0487-z

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