Results 101 to 110 of about 7,879 (179)
Exploring Numerical Correlations: Models and Thermodynamic Kappa
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 +1 more source
Modeling of electrons in the heliosphere [PDF]
PhD (Space Physics), North-West University, Potchefstroom Campus, 2016The propagation and modulation of electrons in the heliosphere play an important part in improving our understanding and assessment of the processes of solar modulation.
Nndanganeni, Rendani Rejoyce
core
Effects of anomalous cosmic rays on the solar wind events in the outer heliosphere
Anomalous cosmic-rays (ACRs) are thought to be originated from the acceleration of pickup ions (PUIs) at the termination shock or interplanetary shocks, and play important role for the plasma dynamics in the outer heliosphere. Due to limited observation,
Yucheng Zhou +5 more
doaj +1 more source
Energetic particles in the heliosphere
This monograph traces the development of our understanding of how and where energetic particles are accelerated in the heliosphere and how they may reach the Earth. Detailed data sets are presented which address these topics. The bulk of the observations
Simnett, George M
core +1 more source
The examination of small-scale magnetic-field structures in the solar wind using two spacecraft
To explore some properties of small-scale magnetic structures in the solar wind at 1 AU, measurements from the THEMIS-ARTEMIS mission with two spacecraft in orbit around the Earth’s moon are used.
Joseph E. Borovsky
doaj +1 more source
Expansion of magnetic clouds in the outer heliosphere
Context . A large amount of magnetized plasma are frequently ejected from the Sun as Coronal Mass Ejections (CMEs). A part of these ejections are detected in the solar wind as magnetic clouds (MCs) which have flux rope signatures. Aims. MCs are typically
P Démoulin +3 more
core
The paper presents the results of MHD modeling of corotating interaction regions (CIRs) at distances of 0.1 AU from the Sun (inner boundary) to much larger distances (20–30 AU) in two variants in which the magnetic field on the photosphere (1) is ...
Pavlov Dmitry +6 more
doaj +1 more source
Potential flow models for the heliosphere and their comparision to 3D MHD-neutral simulation
Various models have been proposed for the SW-LISM plasma interaction to study the shape of the heliosphere. According to the Parker model (1961), when SW interacts with the interstellar plasma with a very weak magnetic field “comet- like” cavity is ...
Thagunna, Shanti Kumari
core
The Global Structure of the Heliosphere
As the Sun moves through the local interstellar medium (LISM), it emits charged particles, creating the heliosphere occupied by the plasma of solar origin.
Gary P. Zank +3 more
core +1 more source
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source

