2013
DOI: 10.5194/nhess-13-3395-2013
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Toward a possible next geomagnetic transition?

Abstract: Abstract. The geomagnetic field is subject to possible reversals or excursions of polarity during its temporal evolution. Considering that: (a) in the last 83 million yr the typical average time between one reversal and the next (the so-called chron) is around 400 000 yr, (b) the last reversal occurred around 780 000 yr ago, (c) more excursions (rapid changes in polarity) can occur within the same chron and (d) the geomagnetic field dipole is currently decreasing, a possible imminent geomagnetic reversal or ex… Show more

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Cited by 30 publications
(25 citation statements)
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“…The SAA region was delimited by the intensity contour line of 32,000 nT. Our results (see Figure 4A) agree with those of De Santis et al (2013) showing how the SAA area extent has been continuously growing. However, our results reveal more details (see Figure 4B): the SAA area extent is increasing with periods of accelerations (1840-1875 and 1900-1960) and decelerations (1975-1900 and FIGURE 4 | SAA extent area (A) and its first time derivative (B) given by the GUFM1 (red points) and IGRF-12 (blue points) models.…”
Section: The Saa During the Last 200 Yearssupporting
confidence: 90%
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“…The SAA region was delimited by the intensity contour line of 32,000 nT. Our results (see Figure 4A) agree with those of De Santis et al (2013) showing how the SAA area extent has been continuously growing. However, our results reveal more details (see Figure 4B): the SAA area extent is increasing with periods of accelerations (1840-1875 and 1900-1960) and decelerations (1975-1900 and FIGURE 4 | SAA extent area (A) and its first time derivative (B) given by the GUFM1 (red points) and IGRF-12 (blue points) models.…”
Section: The Saa During the Last 200 Yearssupporting
confidence: 90%
“…In other words, the decay of the dipolar field increases the extent area of the SAA and decreases the averaged total intensity field at global scale. On the other hand, according to other studies (Hartmann and Pacca, 2009;De Santis et al, 2013), the behavior of the SAA during the last centuries is related to the higher harmonic degrees n = 2 and 3, i.e., the quadrupole and octupole fields. This is an important issue because these non-dipolar contributions play an important role during the geomagnetic reversals that are characterized by high ratios between the non-dipolar over dipolar contribution (e.g., Valet et al, 1999).…”
Section: The Origin Of the Saa: A Case Study For The Last 200 Yearsmentioning
confidence: 74%
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