2014
DOI: 10.1186/bf03352480
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Atmospheric quasi-14 month fluctuation and excitation of the Chandler wobble

Abstract: A quasi-14 month fluctuation in the atmospheric excitation function for the Earth's wobble is discussed by using the re-analysis data of the European Center for Medium-range Weather Forecast for the 14 years between 1980 and 1993. The spectrum of the atmospheric wind excitation function shows a striking peak near the 14-month period. As a result, the atmospheric (wind plus pressure) excitation function shows exactly the same power as that of the geodetic excitation function inferred from the observed wobble at… Show more

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Cited by 13 publications
(18 citation statements)
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“…The theoretical period is consistent with other estimates of the observed Chandler period based on analyses of polar motion time series (e.g., Vicente & Wilson 1997). However, there is no consensus on the value of Q: depending on the time interval and the analysis method, it ranges from 50 (Furuya & Chao 1996;Kuehne et al 1996) to 180 (Vicente & Wilson 1997;Aoyama et al 2003). Gross (2000) and Brzeziński & Nastula (2002) find intermediate values of ∼140.…”
Section: The Polar Motion Excitation By Fluid Layerssupporting
confidence: 71%
See 1 more Smart Citation
“…The theoretical period is consistent with other estimates of the observed Chandler period based on analyses of polar motion time series (e.g., Vicente & Wilson 1997). However, there is no consensus on the value of Q: depending on the time interval and the analysis method, it ranges from 50 (Furuya & Chao 1996;Kuehne et al 1996) to 180 (Vicente & Wilson 1997;Aoyama et al 2003). Gross (2000) and Brzeziński & Nastula (2002) find intermediate values of ∼140.…”
Section: The Polar Motion Excitation By Fluid Layerssupporting
confidence: 71%
“…According to Celaya et al (1999), Gross (2000), and Brzeziński & Nastula (2002), the CW excitation is accounted for, on average, by the atmosphere and oceans. Following Aoyama et al (2003), atmospheric and ocean-bottom pressure and winds are comparable sources of excitation, intermittently playing a prominent role. Seitz & Schmidt (2005) conclude that the atmospheric and oceanic bottom pressure fluctuations are the prominent cause of the CW variability.…”
Section: Introductionmentioning
confidence: 99%
“…Moreover, there is statistical evidence that the Chandler wobble is predominantly a deterministic process. [25,26,27] Some authors have therefore concluded that the wobble is forced by geophysical fluid circulations [11,12,13,14]. In that case the estimates of Q w obtained by Jeffreys's method do not apply directly (a point stressed in [21], but ignored by some authors).…”
Section: Dissipation and Maintenancementioning
confidence: 99%
“…Proposed solutions to this puzzle have, for the most part, relied either on stochastic perturbations to the Earth's mass distribution [9,10], or on marine and atmospheric circulations that might force the wobble near its resonant ω Ch . [11,12,13,14] Here we propose a new model of the Chandler wobble as a weakly non-linear self-oscillation. Unlike a resonator, a self-oscillator maintains periodic motion at the expense of a power source with no corresponding periodicity [15,16].…”
Section: Introductionmentioning
confidence: 99%
“…Recently, air pressure [Plag, 1997],tropospheric winds [Aoyama and Naito, 2001 ], and ocean-bottom pressure variations [Gross, 2000] have been independently proposed as major contribu tions to the excitation of the Chandler wobble. A 14-to 16-month oscillation (FSO) in the atmosphere-ocean system has also been pro posed as a candidate mechanism that could force a wobble having a frequency close to that of the Chandler resonance [Plag, 1997;Aoyama et al, 2003].…”
Section: Section Newsmentioning
confidence: 99%