Results 101 to 110 of about 720 (196)
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
MAGNETIC FLUX TUBE INTERCHANGE AT THE HELIOPAUSE
The magnetic field measured by Voyager 1 prior to its heliocliff encounter on 2012.65 showed an unexpectedly complex transition from the primarily azimuthal inner-heliosheath field to the draped interstellar field tilted by some 20° to the nominal azimuthal direction.
openaire +1 more source
Analysis of interplanetary solar sail trajectories with attitude dynamics [PDF]
We present a new approach to the problem of optimal control of solar sails for low-thrust trajectory optimization. The objective was to find the required control torque magnitudes in order to steer a solar sail in interplanetary space.
Borggrafe, Andreas +3 more
core +2 more sources
Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe. [PDF]
Brandt PC +42 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
We analyze the count rates of 40–139 keV ions that were measured in situ by the Low Energy Charged Particle instrument on Voyager 1 in order to identify the suprathermal ion anisotropies beyond the termination shock and in the very local interstellar (IS)
Konstantinos Dialynas +5 more
doaj +1 more source
Kelvin–Helmholtz Instability and Energetic Neutral Atoms in the Heliosphere
The Interstellar Mapping and Acceleration Probe (IMAP) mission launched from Earth on 2025 September 24, beginning its commissioning phase as the spacecraft makes its way to Lagrange Point 1.
E. J. Zirnstein +3 more
doaj +1 more source
Solar Wind Forecasting for Long-term Variations of the Global Heliosphere
The large-scale dynamics of the heliosphere is driven by solar activity and variable solar wind (SW) conditions. In situ SW observations inform time-dependent heliosphere modeling efforts but are only available up until the present day, thus restricting ...
Jonathan Gasser +5 more
doaj +1 more source
Anomalous Cosmic Rays and Heliospheric Energetic Particles. [PDF]
Giacalone J +9 more
europepmc +1 more source
The secondary energetic neutral atom (ENA) mechanism proposed to explain the ribbon-like enhancement of ENA emission observed by Interplanetary Boundary Explorer (IBEX) involves a pickup ion (PUI) ring-beam population beyond the heliopause. The stability
Yifan Huang +8 more
doaj +1 more source

