activity
20152021
most citedThe development of a split-tail heliosphere and the role of non-ideal processes: a comparison of the BU and Moscow models

23 citations · 63 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2021★ 23 cited

The development of a split-tail heliosphere and the role of non-ideal processes: a comparison of the BU and Moscow models

M. Kornbleuth, M. Opher, I. Baliukin +11

Global models of the heliosphere are critical tools used in the interpretation of heliospheric observations. There are several three-dimensional magnetohydrodynamic (MHD) heliosphe…

astro-ph.SR2020★ 20 cited

The Confinement of the Heliosheath Plasma by the Solar Magnetic Field as Revealed by Energetic Neutral Atom Simulations

M. Kornbleuth, M. Opher, A. T. Michael +4

Traditionally, the solar magnetic field has been considered to have a negligible effect in the outer regions of the heliosphere. Recent works have shown that the solar magnetic fie…

physics.space-ph2020

The Solar-wind with Hydrogen Ion Exchange and Large-scale Dynamics (SHIELD) model: A Self-Consistent Kinetic-MHD Model of the Outer Heliosphere

Adam T. Michael, Merav Opher, Gabor Toth +2

Neutral hydrogen has been shown to greatly impact the plasma flow in the heliopshere and the location of the heliospheric boundaries. We present the results of the Solar-wind with…

astro-ph.SR2018★ 19 cited

Globally Distributed Energetic Neutral Atom Maps for the "Croissant" Heliosphere

Marc Kornbleuth, Merav Opher, Adam T. Michael +1

A recent study by Opher et al. (2015) suggested the heliosphere has a "croissant" shape, where the heliosheath plasma is confined by the toroidal solar magnetic field. The "croissa…

astro-ph.SR2015★ 1 cited

Magnetized jets driven by the sun: the structure of the heliosphere revisited

M. Opher, J. F. Drake, B. Zieger +1

The classic accepted view of the heliosphere is a quiescent, comet-like shape aligned in the direction of the Sun's travel through the interstellar medium (ISM) extending for 1000'…