2014
DOI: 10.1016/j.epsl.2013.11.020
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Core-flow constraints on extreme archeomagnetic intensity changes

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Cited by 59 publications
(88 citation statements)
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“…The rate of change of geomagnetic intensity during this period is ∼6 μT/century or 47% per century (calculated from the lowest value at ∼2250 BCE and highest value at ∼1300 BCE). This variation is consistent with the upper bounds of ∼0.62 μT/yr suggested by Livermore et al (2014) but not as fast as the one reported by Gómez-Paccard et al (2012) with a rate that varies from ∼12 to ∼80 μT/century between 600-1300 CE in western Europe and much lower than the one reported by Shaar et al (2011) in which the intensity changes ∼30 μT in 30 yrs (910-890 BCE) in Levantine area. But a six-fold change of the field (2 × 10 22 -13 × 10 22 Am 2 ) in less than 1000 yrs is still abrupt.…”
Section: Rapid Change In Field Intensitysupporting
confidence: 90%
“…The rate of change of geomagnetic intensity during this period is ∼6 μT/century or 47% per century (calculated from the lowest value at ∼2250 BCE and highest value at ∼1300 BCE). This variation is consistent with the upper bounds of ∼0.62 μT/yr suggested by Livermore et al (2014) but not as fast as the one reported by Gómez-Paccard et al (2012) with a rate that varies from ∼12 to ∼80 μT/century between 600-1300 CE in western Europe and much lower than the one reported by Shaar et al (2011) in which the intensity changes ∼30 μT in 30 yrs (910-890 BCE) in Levantine area. But a six-fold change of the field (2 × 10 22 -13 × 10 22 Am 2 ) in less than 1000 yrs is still abrupt.…”
Section: Rapid Change In Field Intensitysupporting
confidence: 90%
“…The reference B 0 (t) is the mean of the ensemble of 1000 A_FM archeomagnetic field models published by Licht et al [2013]. In order to construct B sp i (t), we adopt the optimized core flow methodology of Livermore et al [2014] and operate at Earth's core surface: for a given geomagnetic field configuration, and a given amount of available kinetic energy (specified in terms of an imposed root-mean-square velocity u rms ), this approach provides the optimal core flow u opt that generates the fastest instantaneous rate of change of geomagnetic intensity, dF∕dt, at a given site on Earth's surface (from now on the Timna-30 archeological site, with longitude = 34.95 ∘ E and latitude = 29.77 ∘ N). In order to account for our uncertain knowledge of the geomagnetic field at the core surface and to build reliable statistics, we consider, at each T i , 1000 different realizations of that field.…”
Section: Geomagnetic Field Modelsmentioning
confidence: 99%
“…In order to account for our uncertain knowledge of the geomagnetic field at the core surface and to build reliable statistics, we consider, at each T i , 1000 different realizations of that field. For each realization, Gauss coefficients from spherical harmonic degree = 1 to the truncation L B =135 [Livermore et al, 2014] are specified as follows: coefficients from = 1 to = 5 are those of one member of the A_FM ensemble at epoch T i (a different member for each realization). Degrees 6 to L B are next populated following the stochastic method presented by Livermore et al [2014].…”
Section: Geomagnetic Field Modelsmentioning
confidence: 99%
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