Turbulence in Electrically Conducting Fluids Driven by Rotating and Travelling Magnetic Fields

2009 ◽  
pp. 215-218
Author(s):  
Jörg Stiller ◽  
Kristina Koal ◽  
Hugh M. Blackburn
Keyword(s):  
Magnetic Fields ◽  
Electrically Conducting ◽  
Conducting Fluids

scholarly journals On heteroclinic separators of magnetic fields in electrically conducting fluids

2015 ◽  
Vol 294 ◽  
pp. 1-5 ◽  
Author(s):  
V. Grines ◽  
T. Medvedev ◽  
O. Pochinka ◽  
E. Zhuzhoma
Keyword(s):  
Magnetic Fields ◽  
Electrically Conducting ◽  
Conducting Fluids

3. Spots and magnetic fields

2020 ◽  
pp. 65-99
Author(s):  
Philip Judge
Keyword(s):  
Magnetic Field ◽  
Magnetic Properties ◽  
Magnetic Fields ◽  
Solar Interior ◽  
Solar Dynamo ◽  
The Sun ◽  
Electrically Conducting ◽  
New Science ◽  
The 1960S ◽  
Conducting Fluids

‘Spots and magnetic fields’ explores sunspot behaviour. We have known since 1908 that sunspots are magnetic, but why does the Sun form them at all? Is the Sun extraordinary in this, or is its behaviour in line with other stars? The Sun’s magnetic field is generated by a solar dynamo, which can be partly explained by magnetohydrodynamics (MHD)—the study of the magnetic properties and behaviour of electrically conducting fluids—however, there is no full consensus on the solar dynamo. In the 1960s the new science of helioseismology gave us insights into the Sun’s interior rotation, but we are unable to make truly critical observations in the solar interior.

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