Characteristics of Perturbations in Recent Length of Day and Polar Motion

Various features of the existing perturbations in the Earth’s spin rotation are investigated for the recent and most reliable data by spectral analysis, filtering, and comparison with idealized model. First, theory of Earth’s spin rotational perturbation is briefly re-derived in the Earth-fixed coor...

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Main Authors: Sung-Ho Na, Younghee Kwak, Jung-Ho Cho, Sung-Moon Yoo, Sungki Cho
Format: Article
Language:English
Published: The Korean Space Science Society 2013-03-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n1/OJOOBS_2013_v30n1_33.pdf
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author Sung-Ho Na
Younghee Kwak
Jung-Ho Cho
Sung-Moon Yoo
Sungki Cho
author_facet Sung-Ho Na
Younghee Kwak
Jung-Ho Cho
Sung-Moon Yoo
Sungki Cho
author_sort Sung-Ho Na
collection DOAJ
description Various features of the existing perturbations in the Earth’s spin rotation are investigated for the recent and most reliable data by spectral analysis, filtering, and comparison with idealized model. First, theory of Earth’s spin rotational perturbation is briefly re-derived in the Earth-fixed coordinate frame. By spectral windowings, different periodic components of the length of day perturbation are separated, and their characters and excitations are discussed. Different periodic components of polar motion are acquired similarly and described with further discussion of their excitations. Causes of the long time trends of both the length of day and polar motion are discussed. Three possible causes are considered for the newly discovered 490-day period component in the polar motion.
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spelling doaj.art-cf10dcfd2e5745498e503f4ab60c30522024-02-02T13:09:39ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092013-03-01301334110.5140/JASS.2013.30.1.033Characteristics of Perturbations in Recent Length of Day and Polar MotionSung-Ho Na0Younghee Kwak1Jung-Ho Cho2Sung-Moon Yoo3Sungki Cho4Korea Astronomy and Space Science Institute, Daejeon 305-348, KoreaKorea Astronomy and Space Science Institute, Daejeon 305-348, KoreaKorea Astronomy and Space Science Institute, Daejeon 305-348, KoreaKorea Astronomy and Space Science Institute, Daejeon 305-348, KoreaKorea Astronomy and Space Science Institute, Daejeon 305-348, KoreaVarious features of the existing perturbations in the Earth’s spin rotation are investigated for the recent and most reliable data by spectral analysis, filtering, and comparison with idealized model. First, theory of Earth’s spin rotational perturbation is briefly re-derived in the Earth-fixed coordinate frame. By spectral windowings, different periodic components of the length of day perturbation are separated, and their characters and excitations are discussed. Different periodic components of polar motion are acquired similarly and described with further discussion of their excitations. Causes of the long time trends of both the length of day and polar motion are discussed. Three possible causes are considered for the newly discovered 490-day period component in the polar motion.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n1/OJOOBS_2013_v30n1_33.pdflength of daypolar motion
spellingShingle Sung-Ho Na
Younghee Kwak
Jung-Ho Cho
Sung-Moon Yoo
Sungki Cho
Characteristics of Perturbations in Recent Length of Day and Polar Motion
Journal of Astronomy and Space Sciences
length of day
polar motion
title Characteristics of Perturbations in Recent Length of Day and Polar Motion
title_full Characteristics of Perturbations in Recent Length of Day and Polar Motion
title_fullStr Characteristics of Perturbations in Recent Length of Day and Polar Motion
title_full_unstemmed Characteristics of Perturbations in Recent Length of Day and Polar Motion
title_short Characteristics of Perturbations in Recent Length of Day and Polar Motion
title_sort characteristics of perturbations in recent length of day and polar motion
topic length of day
polar motion
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2013/v30n1/OJOOBS_2013_v30n1_33.pdf
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