Abstract
Secular variation, the change in the Earth's magnetic field through time, reflects the energy state of the geodynamo. Secular variation is commonly quantified by paleomagnetists as the standard deviation of the angular distances of the virtual geomagnetic poles to their mean pole, known as the S value. This parameter has long been thought to exhibit latitude dependence [S(λ)], whose origin is widely attributed to a combination of time-varying dipole and non-dipole components. The slope and magnitude ofS(λ) are taken as a basis to understand the geomagnetic field and its evolution. Here we show that S(λ) stems from a mathematical aberration of the conversion from directions to poles, hence directional populations better quantify local estimates of paleosecular variation.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Geowissenschaften > Department für Geo- und Umweltwissenschaften
Geowissenschaften > Department für Geo- und Umweltwissenschaften > Geophysik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 550 Geowissenschaften, Geologie |
ISSN: | 0094-8276 |
Sprache: | Englisch |
Dokumenten ID: | 120084 |
Datum der Veröffentlichung auf Open Access LMU: | 09. Okt. 2024 07:52 |
Letzte Änderungen: | 09. Okt. 2024 07:52 |
DFG: | Gefördert durch die Deutsche Forschungsgemeinschaft (DFG) - 58141235 |