ICMEs in the inner heliosphere: origin, evolution and propagation effects
This report assesses the current status of research relating the origin at the Sun, the evolution through the inner heliosphere and the effects on the inner heliosphere of the interplanetary counterparts of coronal mass ejections (ICMEs).
Forsyth, R. +38 more
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Connection of Turbulence with Polytropic Index in the Solar Wind Proton Plasma
This paper improves our understanding of the interplay of the proton plasma turbulent heating sources of the expanding solar wind in the heliosphere. Evidence is shown of the connections between the polytropic index, the rate of the heat absorbed by the ...
George Livadiotis
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Corotating interaction regions as seen by the STEREO Heliospheric Imagers 2007 – 2010
T.M. Conlon and A.O. Williams were supported by an STFC, UK studentship and S.E. Milan was supported by STFC grant ST/K001000/1. Date of Acceptance: 08/08/2015NASA’s Solar Terrestrial Relations Observatory (STEREO) mission has coincided with a pronounced
J. A. Davies +7 more
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Editorial: Interplanetary medium variability as observed in the new era of spacecraft missions
Tommaso Alberti +3 more
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MHD processes in the outer heliosphere
The magnetic field measurements from Voyager and the magnetohydrodynamic (MHD) processes in the outer heliosphere are reviewed. A bibliography of the experimental and theoretical work concerning magnetic fields and plasmas observed in the outer ...
Burlaga, L. F.
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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
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Global MHD Modeling of the Solar Corona and Inner Heliosphere for the Whole Heliosphere Interval
With the goal of understanding the three-dimensional structure of the solar corona and inner heliosphere during the “Whole Heliosphere Interval” (WHI), we have developed a global MHD solution for Carrington rotation (CR) 2068.
Jon A. Linker, Zoran Mikic, Pete Riley
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Radial intensity gradients of galactic cosmic rays in the heliosphere at solar maximum: 1D no-shock simulation [PDF]
We study the spatial distribution of galactic cosmic rays in the heliosphere at solar maximum of cycles 21, 22 and 23, using a one-dimensional no-shock model of the cosmic ray transport equation.
R. A. Caballero-Lopez +1 more
doaj
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
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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
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