The time-averaged magnetic field in numerical dynamos with non-uniform boundary heat flow

By P. Olson, U. Christensen. 2002

174 citations recorded by the source corpus.

Subfields: Atmospheric Science, Geophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/b9693a200e82b8c0b5de902ffadc3e42e0d1dafb

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atmospheric Science

1. G. Hulot
2. Julien Aubert
3. U. Christensen
4. Nils Olsen
5. Mioara Mandea
6. P. Olson
7. Paul J. Tackley
8. Christopher C. Finlay

In Geophysics

1. U. Christensen
2. Mioara Mandea
3. G. Hulot
4. Christopher C. Finlay
5. Julien Aubert
6. Nils Olsen
7. Paul J. Tackley
8. Catherine Constable

In Molecular Biology

1. U. Christensen
2. Julien Aubert
3. G. Hulot
4. P. Olson
5. Mioara Mandea
6. Nils Olsen
7. Christopher C. Finlay
8. Catherine Constable

Citations in the corpus

• Conditions for Earth-like geodynamo models (2010, background): “Finally, their number (two in each hemisphere) and possible stationarity would likely again reflect a possible degree and order two heat flow heterogeneity at the CMB (Gubbins et al., 2007; Olson and Christensen, 2002), which is not accounted for in simple dynamo models.”
• Scaling properties of convection-driven dynamos in rotating spherical shells and application to planetary magnetic fields (2006, background): “(Olson et al. 1999; Ishihara & Kida 2002), the influence of lower mantle heterogeneity on magnetic field properties (Glatzmaier et al. 1999; Bloxham 2000a,b; Olson & Christensen 2002; Bloxham 2002; Christensen & Olson 2003; Kutzner & Christensen 2004) and the generation of planetary magnetic field”
• The Magnetic Field of Planet Earth (2010, background): “This has led to very stimulating results (e.g. Bloxham 2000; Olson and Christensen 2002; Christensen and Olson 2003; Gubbins et al. 2007; Willis et al. 2007; Aubert et al. 2008b; Davies et al. 2008).”
• The paleomagnetism of single silicate crystals: Recording geomagnetic field strength during mixed polarity intervals, superchrons, and inner core growth (2006, background): “A change in heat flux at the core-mantle RG1002 Tarduno et al.: PALEOMAGNETISM OF SINGLE SILICATE CRYSTALS 2 of 31 RG1002 boundary induced by large-scale mantle flow [e.g., Glatzmaier et al., 1999; Olson and Christensen, 2002; Christensen and Olson, 2003] could affect the energetics of the dynamo.”
• Dipole moment scaling for convection-driven planetary dynamos (2005, methodology): “Numerical data from different numerical dynamo calculations were extracted from a variety independently conducted, systematic modeling studies [12,18,26–32].”
• Dynamics and evolution of the deep mantle resulting from thermal, chemical, phase and melting effects (2012, background): “Large lateral variations can prevent a dynamo (Olson and Christensen, 2002), while more moderate variations influence the pattern of core convection (Amit and Choblet, 2010), geomagnetic reversal paths (Gubbins, 1998) and the growth pattern of the inner core (Aubert et al., 2008).”