Results 111 to 120 of about 728 (195)
An Anisotropic Plasma Model of the Heliospheric Interface
We present a pioneering model of the interaction between the solar wind and the surrounding interstellar medium that includes the possibility of different pressures in directions parallel and perpendicular to the magnetic field.
Vladimir Florinski +6 more
doaj +1 more source
The Structure of the Large-Scale Heliosphere as Seen by Current Models. [PDF]
Kleimann J +8 more
europepmc +1 more source
Turbulence in the Heliosheath: spectral analysis from Voyager 1 and 2 data [PDF]
The Voyager 2 spacecraft is traveling through the heliosheath, the outermost layer in heliosphere where the solar wind is slowed by the interstellar gas, while Voyager 1 has entered the local interstellar medium.
Gallana, Luca +8 more
core
Four-fluid model and numerical simulations of magnetic structures in the heliosheath
The first part of this paper extends the three-fluid model of Avinash & Zank for magnetic structures in the heliosheath to a four-fluid model consisting of electrons, pick-up ions (PUIs), solar wind ions (SWIs), and neutral hydrogen.
Shaikh, Dastgeer +3 more
core +1 more source
We present the diffusive flow anisotropy vector components for ∼0.5–35 MeV anomalous cosmic-ray (ACR) protons observed during Voyager 2 roll maneuvers for the magnetometer instrument in the inner heliosheath.
A. C. Cummings +4 more
doaj +1 more source
Termination Shock Particle Streaming Upstream at New Horizons
A couple years before Voyager 1 and Voyager 2 (V2) crossed the termination shock (TS), instruments on board both spacecraft observed high intensities of accelerated termination shock particles (TSPs) beaming in opposite directions.
Erick Powell +15 more
doaj +1 more source
Thermodynamic Definitions of Temperature and Kappa and Introduction of the Entropy Defect. [PDF]
Livadiotis G, McComas DJ.
europepmc +1 more source
Search for the heliosheath with Voyager 1 magnetic field measurements [PDF]
The magnetic field measured by Voyager 1 (V1) near 85 AU from 2002.0 to 2003.17 has the expected properties for the heliospheric magnetic field at that distance and epoch of the solar cycle.
Burlaga, L. F. +6 more
core
Exploring the Complex Heliotail Boundary by an Extended Level Set Approach
There is an ongoing debate regarding the shape of the heliotail. Studies have shown that the heliotail may be “comet-like,” extending for thousands of au. Some previous works defined the heliopause using magnetohydrodynamic variables, which only serve as
C. Onubogu +4 more
doaj +1 more source
Pressure Waves in the Heliosheath? [PDF]
openaire +1 more source

