3 papers
astro-ph.GA2009
Interaction of HVCs with the Outskirts of Galactic Disks: Turbulence
A. Santillan, F. J. Sanchez-Salcedo, J. Kim +2
There exist many physical processes that may contribute to the driving of turbulence in galactic disks. Some of them could drive turbulence even in the absence of star formation. F…
astro-ph2008
The Role of the Random Magnetic Fields in the ISM: HVCs Numerical Simulations
A. Santillan, J. Kim, F. J. Sanchez-Salcedo +2
We know that the galactic magnetic field possesses a random component in addition to the mean uniform component, with comparable strength of the two components. This random compone…
astro-ph2008
MHD Remote Numerical Simulations: Evolution of Coronal Mass Ejections
L. Hernandez-Cervantes, A. Santillan, A. R. Gonzalez-Ponce
Coronal mass ejections (CMEs) are solar eruptions into interplanetary space of as much as a few billion tons of plasma, with embedded magnetic fields from the Sun's corona. These p…