Abstract
Two-dimensional MHD decaying turbulence is studied by numerical calculations with high resolution. Strong local alignment of velocity fields and magnetic fields is observed. This supports the importance of the cross helicity effect in the dynamo problem.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
