Four centuries of geomagnetic secular variation from historical records

By A. Jackson, A. Jonkers, M. Walker. Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2000

1,020 citations recorded by the source corpus.

Subfields: Atmospheric Science, Molecular Biology, Oceanography

View Paper: https://www.semanticscholar.org/paper/d6dfbd93ae862ad439684916399f8052e85d35a6

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Citations in the corpus

The geomagnetic dipole moment over the last 7000 years—new results from a global model (2005, methodology): “2, GUFM [1] and the discrete DGRF/IGRF models (see http://www.”
Solar Forcing for CMIP6 (v3.1) (2016, methodology): “For years 1850–1900, the gufm1 model may be used (Jackson et al., 2000).”
Geomagnetic field for 0–3 ka: 1. New data sets for global modeling (2009, methodology): “…at a rate of about 0.3 a 1 [Merrill et al., 1996], analysis of historical data spanning the past 4 centuries suggests a more complicated view with westward drift prominent in the Indian Ocean/Atlantic hemisphere [Jackson et al., 2000; Bloxham et al., 1989], and more or less absent in the Pacific.”
Improving geomagnetic field reconstructions for 0–3 ka (2011, methodology): “…were chosen by visual comparison of the geomagnetic power spectra of the main field and122 secular variation to those of the historical model gufm1 (Jackson et al., 2000) and the123 International Geomagnetic Reference Field (IGRF 10th generation for 2005, (Maus et al.,124 2005)) in the same way as…”
Persistent high paleosecular variation activity in southern hemisphere for at least 10 000 years (2016, background): “This is an open access article possible mechanism for geomagnetic reversals (Gubbins, 1987), and some (Hulot et al., 2002; Olson, 2002; Olson et al., 2009; De Santis and Qamili, 2015) have suggested the South Atlantic Anomaly may be a precursory signature of an incipient geomagnetic reversal.”
PADM2M: a penalized maximum likelihood model of the 0–2 Ma palaeomagnetic axial dipole moment (2011, methodology): “…timescales, time-varying spherical harmonic models of Earth’s magnetic field derived from historical, archaeomagnetic and/or palaeomagnetic data (Jackson et al. 2000; Korte & Constable 2005; Korte et al. 2009) have yielded insights into dynamo processes (e.g. Amit & Olson 2006; Dumberry &…”
Recent geomagnetic secular variation from Swarm and ground observatories as estimated in the CHAOS-6 geomagnetic field model (2016, background): “The gufm1 model (Jackson et al. 2000) is the definitive source for the historical field from 1590 to 1990.”
Reconstructing Holocene geomagnetic field variation: new methods, models and implications (2014, methodology): “The results are evaluated by comparisons with other models for the same time period and models based on synthetic data sets derived from the historical field model gufm1 (Jackson et al. 2000).”
A reconstruction of radiocarbon production and total solar irradiance from the Holocene 14 C and CO 2 records: implications of data and model uncertainties (2013, background): “…of writing, three reconstructions of the past geomagnetic field are available to us spanning the past 10 kyr (Yang et al., 2000; Knudsen et al., 2008; Korte et al., 2011), shown in Fig.11 together with the VADM value of 8.22× 1022 Am−2 for the period 1840–1990 estimated by Jackson et al.(2000).”
The Magnetic Field of the Earth’s Lithosphere (2010, background): “4.2 Marine Data Measurements Magnetic field measurements made at sea were among the first direct measurements of the magnetic field (Jackson et al. 2000).”
Reconstructing the Holocene geomagnetic field (2011, methodology): “Global geomagnetic field models spanning the past four hundred years [4] have provided a powerful tool for mapping evolving field structure at the surface of Earth’s core, and are widely used for analyses of global and regional field variations.”
The Maunder minimum (1645–1715) was indeed a grand minimum: A reassessment of multiple datasets (2015, methodology): “For example, us-ing a spline of the IGRF (International Geomagnetic Reference Field 4 model after 1900 with the gufm1 model (Jackson et al. 2000) before 1900 we ﬁnd the geomagnetic latitude of Halley’s observatory in Oxford was 60.7 ◦ in 1703 and Edinburgh was at 63.4 ◦ .”
The magnetic structure of convection-driven numerical dynamos (2008, background): “The observation of a tangent cylinder inverse flux patch in the present geomagnetic field (Olson & Aurnou 1999; Jackson et al. 2000; Hulot et al. 2002), although it is weakly constrained and not observed with all field regularizations C© 2008 The Authors, GJI, 172, 945–956 Journal compilation C©…”