EARTH ORIENTATION PARAMETERS FROM SATELLITE LASER RANGING

dc.contributor.authorPavlis, Erricos C.
dc.date.accessioned2020-10-13T17:23:32Z
dc.date.available2020-10-13T17:23:32Z
dc.date.issued2004-06
dc.description14th International Laser Workshop, San Fernando, Spain, June 7 - 11, 2004en_US
dc.description.abstractWe present the new re-analysis of Satellite Laser Ranging (SLR) data to LAGEOS 1/2 and ETALON 1/2 for the definition of the Terrestrial Reference Frame (TRF) and its crust-fixed orientation (Earth Orientation Parameters –EOP). The TRF plays an important role in the multi-technique monitoring of temporal variations in the gravitational field and its very low degree and order components. This area is becoming extremely important with the launch of recent and future geopotential mapping missions for the referencing and calibration of the data and products from these missions. Satellite laser ranging (SLR) has for a long time monitored the continuous redistribution of mass within the Earth system through concomitant changes in the Stokes coefficients of the terrestrial gravity field. Seasonal changes in these coefficients have also been closely correlated with mass transfer in the atmosphere and oceans. The hydrological cycle contributions however are the most difficult to measure accurately so far. This latest analysis of the 1993-present SLR data set from SLR data for the International Earth Rotation Service (IERS) TRF (ITRF) development includes the weekly monitoring of such compound changes in the low degree and order harmonics. Along with the static parameters of the TRF we have determined a time series of variations of its origin with respect to the center of mass of the Earth system (geocenter) and the orientation parameters (pole coordinates and length of day) of the TRF, at daily intervals. The data were obtained by the ILRS global tracking network and they were reduced using NASA Goddard’s GEODYN/SOLVE II software, resulting in a final RMS error of ~8 mm –close to the data noise level. We will discuss our solution, compare it to EOP series inferred from other techniques, and examine their spectrum.en_US
dc.description.urihttps://cddis.nasa.gov/lw14/docs/papers/sci9p_epm.pdfen_US
dc.format.extent8 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.genrepresentations (communicative events)
dc.identifierdoi:10.13016/m2qxon-naro
dc.identifier.citationE. C. Pavlis, EARTH ORIENTATION PARAMETERS FROM SATELLITE LASER RANGING, 14th International Laser Workshop, https://cddis.nasa.gov/lw14/docs/papers/sci9p_epm.pdfen_US
dc.identifier.urihttp://hdl.handle.net/11603/19823
dc.language.isoen_USen_US
dc.publisherNASAen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Joint Center for Earth Systems Technology
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Physics Department
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis is a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleEARTH ORIENTATION PARAMETERS FROM SATELLITE LASER RANGINGen_US
dc.typeTexten_US

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