Results 51 to 60 of about 84,388 (175)
Climate‐Induced Polar Motion: 1900–2100
Abstract It has been demonstrated that the motion of the Earth's rotational pole with respect to the crust—termed polar motion—is increasingly influenced by barystatic processes, that is, continental‐ocean mass redistribution due to melting of polar ice sheets, global glaciers, and variations in terrestrial water storage.
Mostafa Kiani Shahvandi, Benedikt Soja
wiley +1 more source
Phase and amplitude variation of Chandler wobble
Normally, the wobble of the earth has been dealt with in a manner that assumes that the two main periodic components have constant phase and amplitude. An initial assumption of this thesis is that both these parameters can vary with time.
Linton, John Alexander
core +1 more source
Abstract Growing interest in Earth Orientation Parameters (EOP) resulted in various approaches to the EOP prediction algorithms, as well as in the exploitation of distinct input data, including the observed EOP values from various operational data centers and modeled effective angular momentum functions.
Tomasz Kur +50 more
wiley +1 more source
Can we explain the post-2015 absence of the Chandler wobble?
Recent polar motion data do not show a 6-year beat and indicate the absence of the Chandler wobble (CW), whereas we could observe the 6-year beat even in the 1920-40 s when the CW amplitude was known to be smallest.
Ryuji Yamaguchi, Masato Furuya
doaj +1 more source
Revisiting the Excitation of Free Core Nutation
Abstract Earth possesses a Poincaré mode called Free Core Nutation (FCN) due to the misalignment of the rotation axes of the mantle and fluid outer core. FCN is the primary signal in the observations of Celestial Pole Offsets (CPO) and maintained by geophysical mechanisms that are yet to be understood. Earlier studies suggested an origin in Atmospheric
Mostafa Kiani Shahvandi +4 more
wiley +1 more source
Abstract The mass transport of volatiles on Mars represents a seasonally changing load on the surface of the planet. Like on Earth, as mass is redistributed across the planet, the surface responds in a complex manner becoming displaced downwards or upwards.
N. L. Wagner +3 more
wiley +1 more source
The period and Q of the Chandler wobble [PDF]
The calculation of the theoretical period of the Chandler wobble is extended to account for the non-hydrostatic portion of the earth's equatorial bulge and the effect of the fluid core upon the lengthening of the period due to the pole tide. The theoretical period of a realistic perfectly elastic earth with an equilibrium pole tide is found to be 426.7
Smith, Martin L., Dahlen, F. A.
openaire +2 more sources
Excitation of the Earth's Chandler wobble by southern oscillation/El Nino, 1900-1979 [PDF]
The southern oscillation/El Nino (ENSO) is the single most prominent interannual signal in global atmospheric/oceanic fluctuations. The following question is addressed: how important is the angular momentum carried by ENSO in exciting the Earth's ...
Chao, B. F.
core
Abstract The COVID‐19 pandemic prompted critical attention to the performative power of metrics. We suggest that the existential capacities of metrics as a means of pandemic living warrant further consideration. We describe how the COVID‐19 pandemic that came into existence as a public health and political event could only have occurred because of the ...
Vincanne Adams +3 more
wiley +1 more source
Polar motion prediction is an important means to study the dynamics of Earth's rotation and detect the internal structure of the Earth. This paper proposes an LS + iTransformer method that combines the least squares (LS) method with the iTransformer deep
Huizhong Zhu +5 more
doaj +1 more source

