Exploring Numerical Correlations: Models and Thermodynamic Kappa [PDF]
McComas et al. (2025) introduced a numerical experiment, where ordinary uncorrelated collisions between collision pairs are followed by other, controlled (correlated) collisions, shedding light on the emergence of kappa distributions through particle ...
Nicholas V. Sarlis +2 more
doaj +2 more sources
Observations of the Outer Heliosphere, Heliosheath, and Interstellar Medium [PDF]
W S Kurth, John D Richardson
exaly +2 more sources
Solar wind with Hydrogen Ion charge Exchange and Large-Scale Dynamics (SHIELD) DRIVE Science Center
Most stars generate winds and move through the interstellar medium that surrounds them. This movement creates a cocoon formed by the deflection of these winds that envelops and protects the stars. We call these “cocoons” astrospheres. The Sun has its own
Merav Opher +48 more
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Global insight into a complex-structured heliosphere based on the local multi-point analysis
From 29 January to 7 February 2022, the heliosphere was structured with large-scale interacting substructures that appeared with significant dissimilarities at distant observations separated longitudinally by ∼34°.
Sanchita Pal +9 more
doaj +1 more source
Manifestation of solar wind corotating interaction regions in GCR intensity variations
The regions of interaction between solar wind streams of different speed, known as corotating interaction regions, form an almost constantly existing structure of the inner heliosphere.
Krainev M. B. +9 more
doaj +1 more source
The Heliosphere and Local Interstellar Medium from Neutral Atom Observations at Energies Below 10 keV [PDF]
André Galli +2 more
exaly +2 more sources
Numerical modeling of solar wind and coronal mass ejection in the inner heliosphere: A review
The predictions of plasma parameters in the interplanetary medium are the core of space weather forecasts, and the magnetohydrodynamics (MHD) numerical simulation is an important tool in the prediction of plasma parameters.
Man Zhang +12 more
doaj +1 more source
The Structure of the Large-Scale Heliosphere as Seen by Current Models [PDF]
Jens Kleimann +2 more
exaly +2 more sources
Interstellar neutral (ISN) helium atoms penetrating the heliosphere are used to find the flow velocity and temperature of the very local interstellar medium near the heliosphere.
P. Swaczyna +3 more
doaj +1 more source
About Cosmic Ray Modulation in the Heliosphere
Cosmic ray fluxes in the heliosphere are modulated by solar wind with an embedded solar interplanetary magnetic field. The solar activity changes with a period of ~11 year, and this is the main reason for the observed 11-year variations of cosmic ray ...
Yuri Stozhkov +2 more
doaj +1 more source

