On magnetic field of rotating bodies

Author(s):  
M. V. Davidovich
Nature ◽  
1948 ◽  
Vol 161 (4090) ◽  
pp. 450-450 ◽  
Author(s):  
H. T. H. PIAGGIO

Nature ◽  
1948 ◽  
Vol 161 (4094) ◽  
pp. 598-599
Author(s):  
NIELS ARLEY

Nature ◽  
1947 ◽  
Vol 159 (4046) ◽  
pp. 658-666 ◽  
Author(s):  
P. M. S. BLACKETT

1990 ◽  
Vol 140 ◽  
pp. 27-28 ◽  
Author(s):  
A.Z. Dolginov

Difficulties of the dynamo and alternative theories of the magnetic field generation are briefly discussed. The correlation between η = lg μ/μo and ζ = lg J/Jo for rotating celestial bodies is considered. μ is the magnetic and J the angular momentum of the body. Existing theories do not explain such a correlation, and it may be an evidence for some new fundamental interaction.


1951 ◽  
Vol 29 (6) ◽  
pp. 470-479 ◽  
Author(s):  
George Luchak

A phenomenological theory, based on a relativistically covariant generalization of Maxwell's equations to include gravitational fields, is developed to account for the magnetic fields of massive rotating bodies. The equations yield the Wilson–Blackett expression for the magnetic moment of the earth and stars but give no magnetic field for mass-bodies moving without rotation in their own gravitational fields. They indicate that the magnetic field due to the motion of the earth in its orbit is negligibly small compared to the field due to its rotational motion, and they provide a possible explanation for the variable magnetic fields of light-variable stars.


1967 ◽  
Vol 31 ◽  
pp. 381-383
Author(s):  
J. M. Greenberg

Van de Hulst (Paper 64, Table 1) has marked optical polarization as a questionable or marginal source of information concerning magnetic field strengths. Rather than arguing about this–I should rate this method asq+-, or quarrelling about the term ‘model-sensitive results’, I wish to stress the historical point that as recently as two years ago there were still some who questioned that optical polarization was definitely due to magnetically-oriented interstellar particles.


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