331 citations · 2.4k across the 59 of their papers we have counts for
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Properties and selected implications of magnetic turbulence for interstellar medium, Local Bubble and solar wind
A. Lazarian, A. Beresnyak, H. Yan +2
Astrophysical fluids, including interstellar and interplanetary medium, are magnetized and turbulent. Their appearance, evolution, and overall properties are determined by the magn…
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…
The Orientation of the Local Interstellar Magnetic Field
M. Opher, E. C. Stone, T. I. Gombosi
The orientation of the local interstellar magnetic field introduces asymmetries in the heliosphere that affect the location of heliospheric radio emissions and the streaming direct…
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…
Effects of a Local Interstellar Magnetic Field on Voyager 1 and 2 Observations
Merav Opher, Edward C. Stone, Paulett C. Liewer
We show that that an interstellar magnetic field can produce a north/south asymmetry in solar wind termination shock. Using Voyager 1 and 2 measurements, we suggest that the angle…
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…