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相关论文: Magnetic Field Generation in Planets and Satellite…

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The purpose of this communication is to suggest that the mechanism for generating the geomagnetic field and the energy source for powering it are one and the same, a nuclear georeactor at the center of the Earth. Toward this end, I: i)…

地球物理 · 物理学 2007-08-28 J. Marvin Herndon

Understanding the nature of the matter comprising the Solar System is crucial for understanding the mechanism that generates the Earth's geomagnetic field and the magnetic fields of other planets and satellites. The commonality in the Solar…

综合物理 · 物理学 2009-03-27 J. Marvin Herndon

The Earth's magnetic field is generated by dynamo action driven by convection in the outer core. For numerical reasons, inertial and viscous forces play an important role in geodynamo models; however, the primary dynamical balance in the…

地球与行星天体物理 · 物理学 2016-06-08 David W. Hughes , Fausto Cattaneo

Possibilities and difficulties of applying the theory of magnetic field generation by convection flows in rotating spherical fluid shells to the Giant Planets are outlined. Recent progress in the understanding of the distribution of…

地球与行星天体物理 · 物理学 2009-06-02 F. H. Busse , R. D. Simitev

Magnetohydrodynamic simulations of fully convective, rotating spheres with volume heating near the center and cooling at the surface are presented. The dynamo-generated magnetic field saturates at equipartition field strength near the…

天体物理学 · 物理学 2007-05-23 W. Dobler , M. Stix , A. Brandenburg

A thermodynamic model for the generation of magnetic fields in the planets is proposed, considering crossed effects between gravitational and electric forces. The magnetic field of the Earth is estimated and found to be in agreement with…

天体物理学 · 物理学 2007-05-23 F. X. Alvarez

The theory of planetary dynamos and its applications to observed phenomena of planetary magnetism are outlined. It is generally accepted that convection flows driven by thermal or compositional buoyancy are the most likely source for the…

流体动力学 · 物理学 2009-04-14 F. H. Busse , R. D. Simitev

We describe the generation of the electric current flowing along the external magnetic field in the system of massive charged fermions, possessing anomalous magnetic moments and electroweakly interacting with background matter. This current…

高能物理 - 唯象学 · 物理学 2019-06-07 Maxim Dvornikov

Possible origins of the magnetic fields of neutron stars include inheritance from the main sequence progenitor and dynamo action at some stage of evolution of progenitor. Inheritance is not sufficient to explain the fields of magnetars.…

天体物理学 · 物理学 2009-06-23 H. C. Spruit

The origin of cosmic magnetism is an issue of fundamental importance in astrophysics. We review here some of the ideas of how large scale magnetic fields in the universe, particularly in galaxies and galaxy clusters could arise. The popular…

天体物理学 · 物理学 2009-06-23 Kandaswamy Subramanian

Enormous progress has been made on observing stellar magnetism in stars from the main sequence through to compact objects. Recent data have thrown into sharper relief the vexed question of the origin of stellar magnetic fields, which…

太阳与恒星天体物理 · 物理学 2015-06-24 Lilia Ferrario , Andrew Melatos , Jonathan Zrake

In order to address the generation of neutron star magnetic fields, with particular focus on the dichotomy between magnetars and radio pulsars, we consider the properties of dynamos as inferred from other astrophysical systems. With…

高能天体物理现象 · 物理学 2022-02-23 Christopher J. White , Adam Burrows , Matthew S. B. Coleman , David Vartanyan

Today, the generation of magnetic fields in solar-type stars and its relation to activity and rotation can coherently be explained, although it is certainly not understood in its entirety. Rotation facilitates the generation of magnetic…

天体物理学 · 物理学 2009-11-13 A. Reiners , A. Scholz , J. Eislöffel , G. Hallinan , E. Berger , M. Browning , J. Irwin , M. Küker , S. Matt

The Sun is a magnetically active star and is the source of the solar wind, electromagnetic radiation and energetic particles which affect the heliosphere and the Earths atmosphere. The magnetic field of the Sun is responsible for most of…

太阳与恒星天体物理 · 物理学 2026-02-04 Soumitra Hazra

Magnetic buoyancy is believed to drive the transport of magnetic flux tubes from the convection zone to the surface of the Sun. The magnetic fields form twisted loop-like structures in the solar atmosphere. In this paper we use helical…

太阳与恒星天体物理 · 物理学 2011-09-28 Jörn Warnecke , Axel Brandenburg

A new generation mechanism of the magnetic field in an inhomogeneous collisionless plasma with a beam component is proposed. We show that even though the current and charge neutralities are initially satisfied, the current neutrality is…

高能天体物理现象 · 物理学 2020-06-17 Yutaka Ohira

The mechanism by which the Earth's magnetic field is generated is thought to be thermal convection in the metallic liquid iron core. Computational considerations previously restricted most numerical simulations to a regime where the…

地球物理 · 物理学 2017-01-17 Andrey Sheyko , Christopher Finlay , Jean Favre , Andrew Jackson

The origin of the magnetic field in galaxies is an open question in astrophysics. Several mechanisms have been proposed related, in general, with the generation of small seed fields amplified by a dynamo mechanism. In general, these…

天体物理学 · 物理学 2009-10-30 O. D. Miranda , M. Opher , R. Opher

A self-consistent statistical approach to the problem of planetary and stellar magnetism is suggested. The mechanism of magnetic field generation in the astronomical objects, where the existence of fields is associated with the axial…

天体物理学 · 物理学 2015-06-24 S. N. Arteha

This chapter is build from three 1.5 hours lectures given in Udine in april 2018 on various aspects of Earth's core dynamics. The chapter starts with a short historical note on the discovery of Earth's magnetic field and core (section 1).…

地球物理 · 物理学 2019-05-28 Renaud Deguen , Marine Lasbleis
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