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Long-Term Modulation of Cosmic Rays in Solar Cycles 23–24
Abstract —A major trend in the solar magnetic field that began at the end of solar cycle 22 continues to be observed. The main characteristics of the...
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A Review of the Extended EUV Corona Observed by the Sun Watcher with Active Pixels and Image Processing (SWAP) Instrument
The Sun Watcher with Active Pixels and Image Processing (SWAP) instrument onboard ESA’s PRoject for On Board Autonomy 2 (PROBA2) has provided the...
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Large Scale Modulation: View from the Earth Points
AbstractThe article reports a review of the current results obtained over the past decade in the study of cosmic ray solar modulation. The analysis...
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HiRISE - High-Resolution Imaging and Spectroscopy Explorer - Ultrahigh resolution, interferometric and external occulting coronagraphic science
Recent solar physics missions have shown the definite role of waves and magnetic fields deep in the inner corona, at the chromosphere-corona...
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Current Status of MHD Simulations for Space Weather
In this chapter, we review the status of the art of the three-dimensional (3D) time-dependent magnetohydrodynamic (MHD) models of solar wind. We...
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Future of Solar-Terrestrial Physics
As already noted, solar-terrestrial physics as a whole has already gone far beyond the initial understanding of this term, and the fields of its...
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Modeling Coronal Mass Ejections by CESE MHD Model
Coronal mass ejections (CMEs) consist of large-scale eruptions of magnetized plasma from the Sun, and they are considered to be the major drivers of...
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Future Missions
There will always be a need to monitor and study the Sun, the nearby star that throws huge amounts of high-energy particles and electromagnetic...
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Data-Driven MHD Modeling of Solar Wind
Solar wind is rather than of steady state, but physically dynamic corresponding to the solar rotation, solar mass flow and solar magnetic field...
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Charge Exchange in X-Ray Astrophysics
Charge exchange is an atomic process that primarily occurs at interfaces between the neutral and ionized gas. The study of the process has been...
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The Solar Wind Speed Expansion Factor [\({v}\)–\(f _{\text{s}}\)] Relationship at the Inner Boundary (18 \(\text{R}_{\odot }\)) of the Heliosphere
The accuracy of data-driven magnetohydrodynamics (MHD) models depends on accurate boundary conditions specified at the inner heliosphere. However,...
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Kappa Distributions: Concluding Remarks and Perspectives
This last chapter provides a brief summary of the main results and conclusions, which can be drawn from the topical analyzes of this book. Without...
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Precursory Signals of Forbush Decreases Not Connected with Shock Waves
Forbush decreases (FDs) are sharp reductions of the cosmic-ray (CR) intensity, following intense solar activity such as coronal mass ejections (CMEs)...
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Aspects of the Influence of the Global Heliospheric Current Sheet on GCR Propagation
AbstractThe influence of the global heliospheric current sheet on the heliospheric characteristics important for GCR propagation is considered,...
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SMILE: A Novel Way to Explore Solar-Terrestrial Interactions
This chapter describes the scientific motivations that led to the development of the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE)...
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Three-Dimensional Simulations of Solar Wind Preconditioning and the 23 July 2012 Interplanetary Coronal Mass Ejection
Predicting the large-scale eruptions from the solar corona and their propagation through interplanetary space remains an outstanding challenge in...
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Earth’s Exospheric X-Ray Emissions
In this chapter we explore solar wind charge exchange X-ray emission emitted from the Earth’s exosphere, following an interaction between heavy ions...
