NORDITA logo NORDITA, Stockholm
Astrophysics Group
Postdoctoral fellow
Simon Candelaresi
SU logo KTH logo
home publications/talks cv computing links pictures/movies
Photo of Simon Candelaresi
E-mail  iomsn@nordita.org
Office No. +46 8 5537 8277
Group  Astrophysics and Astrobiology
Address  NORDITA
Roslagstullsbacken 23
10691 Stockholm
Sweden
LinkedIn www.linkedin.com/pub/simon-candelaresi/31/928/688

Research Interests



Helical small-scale turbulent motions lead to an enhancement of magnetic energy. First the small-scale field grows then the field of the largest scale. Due to the conservation of magnetic helicity the large-scale field grows only on resistive time scales.
arxiv:1208.4529 ]


2D hydrodynamics simulation of a Kolmogorov flow with high Reynolds number. A small initial disturbance in the velocity field gets increased by the instability. The colors represent vorticity.


Decay of the Borromean rings in resistive MHD. Two helical structures arise in corners of the simulation domain. Their magnetic helicity is of opposite sign, since the total magnetic heilcity is 0.
Phys. Rev. E, 84(1):016406, 2011 ]
home publications/talks cv computing links pictures/movies