| scholarly article | Q13442814 |
| P6179 | Dimensions Publication ID | 1009539191 |
| P356 | DOI | 10.1038/365541A0 |
| P2888 | exact match | https://scigraph.springernature.com/pub.10.1038/365541a0 |
| P50 | author | Rainer Hollerbach | Q51707501 |
| P2093 | author name string | Chris A. Jones | |
| P2860 | cites work | Geomagnetic Reversals | Q56603667 |
| A geodynamo model incorporating a finitely conducting inner core | Q56838068 | ||
| Generation of magnetic fields by convection in a rotating spherical fluid shell of infinite Prandtl number | Q57926286 | ||
| Mechanism for geomagnetic polarity reversals | Q59071549 | ||
| Morphology of the geomagnetic field and implications for the geodynamo | Q59091178 | ||
| Westward drift, core motions and exchanges of angular momentum between core and mantle | Q59091709 | ||
| P433 | issue | 6446 | |
| P407 | language of work or name | English | Q1860 |
| P304 | page(s) | 541-543 | |
| P577 | publication date | 1993-10-01 | |
| P1433 | published in | Nature | Q180445 |
| P1476 | title | Influence of the Earth's inner core on geomagnetic fluctuations and reversals | |
| P478 | volume | 365 |
| Q63090424 | 56 The Earth's core |
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| Q56326332 | A multi-layered kinematic dynamo model: implications of a stratified upper layer in the Earth's core |
| Q56838060 | A spectral solution of the magneto-convection equations in spherical geometry |
| Q55879456 | A three-dimensional self-consistent computer simulation of a geomagnetic field reversal |
| Q59091124 | An Earth-like numerical dynamo model |
| Q60081233 | Catching the inner core in a spin |
| Q59896541 | Constraints from material properties on the dynamics and evolution of Earth’s core |
| Q56503701 | Constraints on the crystalline structure of the inner core: Mechanical instability of BCC iron at high pressure |
| Q34304910 | Convective-region geometry as the cause of Uranus' and Neptune's unusual magnetic fields |
| Q64388238 | Degree one heterogeneity and hemispherical variation of anisotropy in the inner core fromPKP(BC)-PKP(DF) times |
| Q57942944 | Dynamo action in a uniform ambient field |
| Q59840484 | Effect of the magnetic field at the inner core boundary on the flow in the Earth's core |
| Q60478669 | Evidence for a very-long-term trend in geomagnetic secular variation |
| Q58995105 | Excursions in geomagnetism |
| Q56326530 | Geomagnetic field morphologies from a kinematic dynamo model |
| Q60066237 | Influence of the inner core |
| Q56326470 | Is the geodynamo process intrinsically unstable? |
| Q70941784 | Late Mesoproterozoic magnetostratigraphic results from Siberia: Paleogeographic implications and magnetic field behavior |
| Q63389294 | Low paleointensities recorded in 1 to 2.4 Ga Proterozoic dykes, Superior Province, Canada |
| Q104537926 | On rates of occurrence of geomagnetic reversals |
| Q59334550 | Oscillation or rotation: a comparison of two simple reversal models |
| Q76356891 | Paleomagnetic volcanic data and geometric regularity of reversals and excursions |
| Q55933779 | Recent geodynamo simulations and observations of the geomagnetic field |
| Q60616834 | Recent investigations of the 0-5 Ma geomagnetic field recorded by lava flows |
| Q60704656 | Seismology of the core |
| Q57813173 | Seven thousand year duration for a geomagnetic excursion constrained by230Thxs |
| Q70642683 | Shallow bias of paleomagnetic inclinations in the Paleozoic and Precambrian |
| Q57820110 | Statistical assessment of preferred transitional VGP longitudes based on palaeomagnetic lava data |
| Q47303362 | Structural and temporal requirements for geomagnetic field reversal deduced from lava flows |
| Q34391596 | The Cretaceous superchron geodynamo: observations near the tangent cylinder. |
| Q56326515 | The distinction between geomagnetic excursions and reversals |
| Q57799619 | The implications of non-suppressed geomagnetic secular variation during the Permo-Carboniferous Reversed Superchron |
| Q63389295 | The inner core and the geodynamo |
| Q34391651 | The innermost inner core of the earth: evidence for a change in anisotropic behavior at the radius of about 300 km. |
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