Three dimensional simulation of the magnetic stress in a neutron star crust.

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Magnetic field evolution in magnetar crusts through three-dimensional simulations Magnetar activity via the density–shear instability in Hall-MHD Resistive tearing instability in electron MHD: application to neutron star crusts

P2860

Q28603964-42C71923-61F8-4B9B-8F45-9A8662040B13 Q56837953-32820637-5D66-42D9-9EEB-CE3B101EB2FD Q58420751-5F6669FD-8D87-4D51-AB8A-708423244B75

P2860

Three dimensional simulation of the magnetic stress in a neutron star crust.

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http://www.wikidata.org/entity/Q50907018

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Three dimensional simulation of the magnetic stress in a neutron star crust.

@en

Three dimensional simulation of the magnetic stress in a neutron star crust.

@en-gb

Three dimensional simulation of the magnetic stress in a neutron star crust.

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type

Item

label

Three dimensional simulation of the magnetic stress in a neutron star crust.

@en

Three dimensional simulation of the magnetic stress in a neutron star crust.

@en-gb

Three dimensional simulation of the magnetic stress in a neutron star crust.

@nl

prefLabel

Three dimensional simulation of the magnetic stress in a neutron star crust.

@en

Three dimensional simulation of the magnetic stress in a neutron star crust.

@en-gb

Three dimensional simulation of the magnetic stress in a neutron star crust.

@nl

P1154

2-s2.0-84930221827

http://www.w3.org/2001/XMLSchema#string

P1433

Physical Review Letters

P1476

Three dimensional simulation of the magnetic stress in a neutron star crust

@en

P2093

T S Wood

http://www.w3.org/2001/XMLSchema#string

P2860

A variable absorption feature in the X-ray spectrum of a magnetar.

A highly resistive layer within the crust of X-ray pulsars limits their spin periods

Cascades in decaying three-dimensional electron magnetohydrodynamic turbulence

Density-shear instability in electron magneto-hydrodynamics

Hall drift in the stratified crusts of neutron stars

The influence of Hall drift on the magnetic fields of neutron stars

Hall Attractor in Axially Symmetric Magnetic Fields in Neutron Star Crusts

Hall effect in neutron star crusts: evolution, endpoint and dependence on initial conditions

P304

191101

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P31

scholarly article

P356

10.1103/PHYSREVLETT.114.191101

http://www.w3.org/2001/XMLSchema#string

P407

English

P433

http://www.w3.org/2001/XMLSchema#string

P478

114

http://www.w3.org/2001/XMLSchema#string

P50

Rainer Hollerbach

Toby S Wood

P5530

3091077

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P577

2015-05-12T00:00:00Z

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P6179

1040745357

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P698

26024158

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P818

1501.05149

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P953

85457/