activity
20082020
most citedMHD Waves and Coronal Heating: Unifying Empirical and MHD Turbulence Models

179 citations · 750 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2020

Numerical simulations of shear-induced consecutive coronal mass ejections

D. -C. Talpeanu, E. Chané, S. Poedts +4

Methods: Stealth CMEs represent a particular class of solar eruptions that are clearly distinguished in coronagraph observations, but they don't have a clear source signature. A pa…

physics.space-ph2019

Toward quantitative model for simulation and forecast of solar energetic particle production during gradual events -- II: kinetic description of SEP

D. Borovikov, I. V. Sokolov, Z. Huang +2

Solar Energetic Particles (SEPs) possess a high destructive potential as they pose multiple radiation hazards on Earth and onboard spacecrafts. The present work continues a series…

physics.space-ph2018★ 21 cited

Toward Quantitative Model for Simulation and Forecast of Solar Energetic Particles Production during Gradual Events - I: Magnetohydrodynamic Background Coupled to the SEP Model

D. Borovikov, I. V. Sokolov, I. Roussev +2

Solar Energetic Particles (SEPs) are an important aspect of space weather. SEP events posses a high destructive potential, since they may cause disruptions of communication systems…

physics.space-ph2018★ 22 cited

Fitting and Reconstruction of Thirteen Simple Coronal Mass Ejections

Nada Al-Haddad, Teresa Nieves-Chinchilla, Neel P. Savani +2

Coronal mass ejections (CMEs) are the main drivers of geomagnetic disturbances, but the effects of their interaction with Earth's magnetic field depend on their magnetic configurat…

astro-ph.SR2016★ 78 cited

Heating mechanisms in the low solar atmosphere through magnetic reconnection in current sheets

Lei Ni, Jun Lin, Ilia I. Roussev +1

We simulate several magnetic reconnection processes in the low solar chromosphere/photosphere, the radiation cooling, heat conduction and ambipolar diffusion are all included. Our…

astro-ph.SR2012★ 179 cited

MHD Waves and Coronal Heating: Unifying Empirical and MHD Turbulence Models

Igor V. Sokolov, Bart van der Holst, Rona Oran +6

We present a new global model of the solar corona, including the low corona, the transition region and the top of chromosphere. The realistic 3D magnetic field is simulated using t…