activity
20032009
most citedThree-Dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations

169 citations · 219 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.SR200927 cited

On the Effect of Magnetic Spots on Stellar Winds and Angular Momentum Loss

O. Cohen, J. J. Drake, V. L. Kashyap +1

We simulate the effect of latitudinal variations in the location of star spots, as well as their magnetic field strength, on stellar angular momentum loss to the stellar wind. We u…

physics.space-ph200820 cited

Observational evidence of CMEs interacting in the inner heliosphere as inferred from MHD simulations

N. Lugaz, W. B. Manchester, I. I. Roussev +1

The interaction of multiple Coronal Mass Ejections (CMEs) has been observed by LASCO coronagraphs and by near-Earth spacecraft, and it is thought to be an important cause of geo-ef…

astro-ph2008169 cited

Three-Dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations

Ward Manchester, Angelos Vourlidas, Gabor Toth +6

We numerically model the coronal mass ejection (CME) event of October 28, 2003 that erupted from active region 10486 and propagated to Earth in less than 20 hours causing severe ge…

astro-ph20063 cited

Global Asymmetry of the Heliosphere

Merav Opher, Edward C. Stone, Paulett C. Liewer +1

Opher et al. 2006 showed that an interstellar magnetic field parallel to the plane defined by the deflection of interstellar hydrogen atoms can produce a north/south asymmetry in t…

astro-ph2004

Magnetic Effects Change Our View of the Heliosheath

M. Opher, P. C. Liewer, M. Velli +5

There is currently a controversy as to whether Voyager 1 has already crossed the Termination Shock, the first boundary of the Heliosphere. The region between the Termination Shock…

astro-ph2004

Magnetic Effects at the Edge of the Solar System: MHD Instabilities, the de Laval nozzle Effect and an Extended Jet

M. Opher, P. C. Liewer, M. Velli +6

To model the interaction between the solar wind and the interstellar wind, magnetic fields must be included. Recently Opher et al. 2003 found that, by including the solar magnetic…