Results 101 to 110 of about 2,085 (203)
The Effects of Turbulence on Heliosheath Ions and Implications for Energetic Neutral Atoms
The distribution of ions in the heliosheath—the region between the heliospheric termination shock and the heliopause—is important for understanding remote observations of energetic neutral atoms (ENAs).
Senbei Du +5 more
doaj +1 more source
News Feature: Voyager still breaking barriers decades after launch. [PDF]
Croswell K.
europepmc +1 more source
Large-scale Field-aligned Flows in the Heliosheath
We use a state-of-the-art 3D MHD simulation to show that large-scale thermal pressure gradients in the heliosheath drive suprathermal particles (pickup ions with 1–5 keV) to stream along magnetic field lines faster than the cold bulk solar wind.
Merav Opher +9 more
doaj +1 more source
Slowdown and Heating of Interstellar Neutral Helium by Elastic Collisions Beyond the Heliopause. [PDF]
Swaczyna P +4 more
europepmc +1 more source
We investigate the role of pickup ions (PUIs) in the interaction of a periodically varying solar wind (SW) with the local interstellar medium (LISM).
R. K. Bera +5 more
doaj +1 more source
The Early History of Heliospheric Science and the Spacecraft That Made It Possible. [PDF]
Zank GP +10 more
europepmc +1 more source
Consequences of Hot Electrons for the Structure of the Outer Heliosphere
The temperature of electrons is largely unknown in the outer heliosphere because there is a gap in Voyager measurements from ∼3 eV to 22 keV. Most models assume that the electrons have the same temperature as the bulk cold thermal solar wind (10 ^4 K ...
Ethan Schuyler Bair +5 more
doaj +1 more source
Persistent plasma waves in interstellar space detected by Voyager 1. [PDF]
Koch Ocker S +5 more
europepmc +1 more source
Dust in and Around the Heliosphere and Astrospheres. [PDF]
Sterken VJ +9 more
europepmc +1 more source
INTERSTELLAR MAGNETIC FIELD SURROUNDING THE HELIOPAUSE
This paper presents a three-dimensional analytical solution, in the limit of very low plasma β-ratio, for the distortion of the interstellar magnetic field surrounding the heliopause. The solution is obtained using a line dipole method that is the integration of point dipole along a semi-infinite line; it represents the magnetic field caused by the ...
openaire +1 more source

