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Non-Tidal Ocean Excitation Functions

Non-tidal ocean excitation functions (CHI) can be readily integrated into polar motion by means of the Liouville equation. Excitation functions consider the rotational deformation of the Earth and its associated passive response of equilibrium oceans, the relative angular momentum of the Earth's core, and the effects of mantle anelasticity. CHI is linearly derived from non-tidal ocean angular momentum as described by Gross (2009).

Operational Series

NameOcean ModelData SpanResolutionLatencyComments
ESMGFZ v1.2MPIOMJan 1976 to present3 hours1 dayIB removed

Ocean Model Experiments

NameOcean ModelData SpanResolutionComments
c20010701.chiMITgcmJan 1980 to Mar 20021 day-
ECCO_50yr.chiMITgcmJan 1949 to Dec 200210 days-
ECCO_kf066a2.chiMITgcmJan 1993 to Dec 20081 day-
ECCO_kf066b.chiMITgcmJan 1993 to Dec 20081 day-
ECCO_kf079.chiMITgcmJan 1993 to Mar 20201 day-
ECCO_kf080i.chiMITgcmJan 1993 to Mar 20201 day-

All available experiments can be downloaded here.

*FWF: Net-effects of freshwater fluxes from continental (and atmospheric) storages into the oceans are explicitly considered.

Gross, R. S. (2009), Earth Rotation Variations -- Long Period, In: Herring, T. (ed.), Treatise on Geophysics, Volume 3: Geodesy, p. 239-294, Elsevier, Amsterdam.

Contact

Dr. Henryk Dobslaw
Earth System Modelling

Telegrafenberg
Building A20, room 316
14473 Potsdam
tel. +49 331 288-1974

henryk.dobslaw@gfz.de