activity
20162021
most citedThree-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence

87 citations · 139 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2021

The strength and structure of the magnetic field in the galactic outflow of M82

Enrique Lopez-Rodriguez, Jordan Guerra, Mahboubeh Asgari-Targhi +1

Galactic outflows driven by starbursts can modify the galactic magnetic fields and drive them away from the galactic planes. Here, we quantify how these fields may magnetize the in…

astro-ph.GA2020

The Role of the Critical Ionization Velocity Effect in Interstellar Space and the Derived Abundance of Helium

Gerrit L. Verschuur, Joan T. Schmelz, Mahboubeh Asgari-Targhi

Gaussian analysis of new, high-angular-resolution interstellar 21-cm neutral hydrogen emission profile structure more clearly reveals the presence of the previously reported signat…

astro-ph.SR201987 cited

Three-dimensional simulation of the fast solar wind driven by compressible magnetohydrodynamic turbulence

Munehito Shoda, Takeru Ken Suzuki, Mahboubeh Asgari-Targhi +1

Using a three-dimensional compressible magnetohydrodynamic (MHD) simulation, we have reproduced the fast solar wind in a direct and self-consistent manner, based on the wave/turbul…

astro-ph.SR201752 cited

The Heating of Solar Coronal Loops by Alfven Wave Turbulence

Adriaan A. van Ballegooijen, Mahboubeh Asgari-Targhi, Alexander Voss

In this paper we further develop a model for the heating of coronal loops by Alfven wave turbulence (AWT). The Alfven waves are assumed to be launched from a collection of kilogaus…

astro-ph.SR2016

Heating and Acceleration of the Fast Solar Wind by Alfvén Wave Turbulence

A. A. van Ballegooijen, M. Asgari-Targhi

We present numerical simulations of reduced magnetohydrodynamic (RMHD) turbulence in a magnetic flux tube at the center of a polar coronal hole. The model for the background atmosp…