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  • 1
    Publication Date: 2020-02-12
    Description: We present an analytical approach to compute the curvature effect by the new analytical solutions of coseismic deformation derived for the homogeneous sphere model. We consider two spheres with different radii: one is the same as earth and the other with a larger radius can approximate a half-space model. Then, we calculate the coseismic displacements for the two spheres and define the relative percentage of the displacements as the curvature effect. The near-field curvature effect is defined relative to the maximum coseismic displacement. The results show that the maximum curvature effect is about 4 per cent for source depths of less than 100 km, and about 30 per cent for source depths of less than 600 km. For the far-field curvature effect, we define it relative to the observing point. The curvature effect is extremely large and sometimes exceeds 100 per cent. Moreover, this new approach can be used to estimate any planet's curvature effect quantitatively. For a smaller sphere, such as the Moon, the curvature effect is much larger than that of the Earth, with an inverse ratio to the earth's radius.
    Language: English
    Type: info:eu-repo/semantics/article
    Format: application/pdf
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  • 2
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    In:  XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
    Publication Date: 2023-09-12
    Description: Spherical wavelets and radial basis functions are used for getting multiscale features of local gravity anomalies. Several earth’s geopotential models and altimetric gravity anomalies are used in modelling. The difference of Gauss (DOG) spherical wavelets and radial basis functions are used to establish a model by using the gravity anomalies from the earth’s geopotential models and that from altimetric data. The results showed multiscale features of the gravity anomalies. This method is useful for inversion of gravity field by multisource data fusion and seafloor topography inversion.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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  • 3
    Publication Date: 2023-09-12
    Description: Plasmaspheric hiss is an electromagnetic wave mode that occurs ubiquitously in the high-density plasmasphere and contributes crucially to the dynamic behavior of the Earth’s Van Allen radiation belts. While plasmaspheric hiss is commonly considered to be a broadband emission with frequencies from ∼100 Hz to several kHz, here we report Van Allen Probes measurements of unambiguous banded signatures of plasmaspheric hiss, uniquely characterized by an upper band above ∼200 Hz, a lower band below ∼100 Hz and a power gap in between. In statistics, banded plasmaspheric hiss occurs with the probability ~8% in the postnoon sector within 2.5-5.0 Earth radii, showing strong dependence on geomagnetic and solar wind conditions. Based upon observations, this talk will also discuss the possible mechanism(s) that may account for the formation of banded hiss waves.
    Language: English
    Type: info:eu-repo/semantics/conferenceObject
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