135 citations · 763 across the 41 of their papers we have counts for
7 papers · 1 filter
A Two-Population von Mises--Fisher Distribution of the Magnetic Field Direction in the Young Solar Wind
Gang Li, N. H. Bian, S. Y. Huang +6
The one-point distribution of the magnetic field direction in the young solar wind is found to be a superposition of two populations rather than a single exponential. Using Parker…
Radio polarization from runaway star bowshocks-I. The general case
M. V. del Valle, R Santos-Lima, M Pohl
High velocity stars move through the interstellar medium with V > 30 km/s. When the star has powerful winds, under the appropriate conditions, the interaction of the wind with the…
Diffusion of large-scale magnetic fields by reconnection in MHD turbulence
R. Santos-Lima, G. Guerrero, E. M. de Gouveia Dal Pino +1
The rate of magnetic field diffusion plays an essential role in several astrophysical plasma processes. It has been demonstrated that the omnipresent turbulence in astrophysical me…
Magnetic fields in early protostellar disk formation
Diego F. González-Casanova, Reinaldo Santos-Lima, Alexander Lazarian
We consider formation of accretion disks from a realistically turbulent molecular gas using 3D MHD simulations. In particular, we analyze the effect of the fast turbulent reconnect…
Turbulence and Dynamo Interlinks
E. M. de Gouveia Dal Pino, R. Santos-Lima, G. Kowal +1
The role of turbulence in astrophysical environments and its interplay with magnetic fields is still highly debated. In this lecture, we will discuss this issue in the framework of…
Magnetic Flux Transport by turbulent reconnection in astrophysical flows
Elisabete M. de Gouveia Dal Pino, Márcia R. M. Leão, Reinaldo Santos-Lima +3
The role of MHD turbulence in astrophysical environments is still highly debated. An important question that permeates this debate is the transport of magnetic flux. This is partic…
MHD turbulence-Star Formation Connection: from pc to kpc scales
E. M. de Gouveia Dal Pino, R. Santos-Lima, A. Lazarian +3
The transport of magnetic flux to outside of collapsing molecular clouds is a required step to allow the formation of stars. Although ambipolar diffusion is often regarded as a key…