Results 21 to 30 of about 720 (196)
Using Lyman-α to probe the interior and edges of the heliosphere
Understanding the role of neutral atoms in the heliospheric interface (between the bow shock and heliopause) is critical to identifying dynamics within our local bubble.
Majd Mayyasi +9 more
doaj +1 more source
A POROUS, LAYERED HELIOPAUSE [PDF]
7 pages, 4 ...
Swisdak, M., Drake, J. F., Opher, M.
openaire +2 more sources
On the Vitality, or Lack Thereof, in Heliospheric and Coronal Physics
Abstract Heliospheric physics is the study of all phenomena in the solar wind, which carves out the heliosphere from the local interstellar medium. Coronal physics is the study of all phenomena in the solar corona, which creates the supersonic wind and all disturbances and variations contained therein.
Len A. Fisk
wiley +1 more source
Ensemble Forecasts of Solar Wind Connectivity to 1 Rs Using ADAPT‐WSA
Abstract The solar wind which arrives at any location in the solar system is, in principle, relatable to the outflow of solar plasma from a single source location. This source location, itself usually being part of a larger coronal hole, is traceable to 1 RS along the Sun's magnetic field, in which the entire path from 1 RS to a location in the ...
D. E. da Silva +3 more
wiley +1 more source
Abstract The last two decades of cosmic ray research have been eventful, to say the least. The Voyager spacecraft explored the outer‐most regions of the heliosphere and eventually left our local astrosphere to explore the galaxy. At the same time, the Parker Solar Probe spacecraft, amongst many other exciting recent missions, is exploring the inner ...
R. Du Toit Strauss
wiley +1 more source
Abstract We report the concentrations and isotope ratios of light noble gases (He, Ne, Ar) in 10 small basalt fragments derived from lunar regolith soils at the Apollo 12 landing site. We use cosmic ray exposure (CRE) and shielding condition histories to consider their geological context.
Mark C. Nottingham +7 more
wiley +1 more source
1I/‘Oumuamua as an N2 Ice Fragment of an exo‐Pluto Surface: I. Size and Compositional Constraints
Abstract The origin of the interstellar object 1I/‘Oumuamua has defied explanation. We perform calculations of the non‐gravitational acceleration that would be experienced by bodies composed of a range of different ices and demonstrate that a body composed of N2 ice would satisfy the available constraints on the non‐gravitational acceleration, size ...
Alan P. Jackson, Steven J. Desch
wiley +1 more source
Unified Picture of the Local Interstellar Magnetic Field from Voyager and IBEX
Prior to the Voyagers’ heliopause crossings, models and the community expected the magnetic field to show major rotations across the boundary. Surprisingly, the field showed no significant change in direction from the heliospheric Parker Spiral at either
J. S. Rankin +4 more
doaj +1 more source
The charge-exchange induced coupling between plasma-gas counterflows in the heliosheath [PDF]
Many hydrodynamic models have been presented which give similar views of the interaction of the solar wind plasma bubble with the counterstreaming partially ionized interstellar medium.
H. J. Fahr
doaj +1 more source
Observations by the Voyager 1 and 2 plasma wave instruments may have provided evidence of the edge of the solar system by “remote sensing.” The two plasma wave receivers detected a weak signal near 3 kHz during late 1983 and early 1984 while the spacecraft were approximately 13 AU (Voyager 2) and 21 AU (Voyager 1) from the sun.
William S. Kurth +3 more
openaire +1 more source

