Satellite magnetic anomalies with a smooth spectral transition to long wavelengths

0556785 - ASÚ 2023 RIV NL eng J - Článek v odborném periodiku
Sebera, Josef - Bezděk, Aleš - Ebbing, J.
Satellite magnetic anomalies with a smooth spectral transition to long wavelengths.
Physics of the Earth and Planetary Interiors. Roč. 324, March (2022), č. článku 106843. ISSN 0031-9201. E-ISSN 1872-7395
Grant CEP: GA MŠMT(CZ) LTT18011
Institucionální podpora: RVO:67985815
Klíčová slova: geomagnetic field * magnetic anomaly * iterative filter
Obor OECD: Physical geography
Impakt faktor: 2.3, rok: 2022
Způsob publikování: Omezený přístup
https://doi.org/10.1016/j.pepi.2022.106843

In most cases, the magnetic field anomalies from satellite data and models are determined by using a cut-off degree that splits the Earth's internal magnetic field (supposed to be of the core and lithospheric origin) into long-wavelength and a short-wavelength parts. This practice allows to effectively compare the signal of both components with other models and controls the signal content as well. In this study an alternative approach is followed to provide the components in long and short wavelengths without cutting the spectrum. Instead, we seek iteratively for the signal loss when the magnetic signal (from degree 1 to the maximum degree of the model) is propagated from the core-mantle boundary to satellite altitude. The problem is generally non-unique, it is required that the signal fit has to follow the slope of the geomagnetic spectrum over the lowest degrees (the degrees least affected by the magnetic lithosphere). The tool operates in the spatial domain the spectral slope criterion is met after the procedure ends by selecting an appropriate solution. The method can be applied to the vector components individually as soon as they are given in the Earth-fixed Earth-centered frame, for which the integral equation is valid. The obtained magnetic anomalies have different spectral properties because the transition from the long wavelengths to the short wavelengths becomes smooth, although the appropriate number of iterations is questionable. It is found that the long-wavelength signal hands over the magnitude dominance to the short-wavelength part at around degrees 16 to 18.
Trvalý link: http://hdl.handle.net/11104/0331651