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What is Solar Wind

Handbook of Research on AI Methods and Applications in Computer Engineering
“Not uniform” stream of charged participles, that flows from the Sun in all possible directions.
Published in Chapter:
The Application of Machine Learning for Predicting Global Seismicity
Viacheslav Shkuratskyy (York St. John University, UK), Aminu Bello Usman (York St. John University, UK), and Michael S. O'Dea (York St. John University, UK)
DOI: 10.4018/978-1-6684-6937-8.ch011
Abstract
An earthquake is one of the deadliest natural disasters. Forecasting an earthquake is a challenging task since natural causes such as rainfall or volcanic eruptions disrupt data. Earthquakes can also be caused by human beings, such as mining or dams. Solar activity has also been suggested as a possible cause of earthquakes. Solar activity and earthquakes occur in different parts of the solar system, separated by a huge distance. However, scientists have been trying to figure out if there are any links between these two seemingly unrelated occurrences since the 19th century. In this chapter, the authors explored the methods of how machine learning algorithms including k-nearest neighbour, support vector regression, random forest regression, and long short-term memory neural networks can be applied to predict earthquakes and to understand if there is a relationship between solar activity and earthquakes. The authors investigated three types of solar activity: sunspots number, solar wind, and solar flares, as well as worldwide earthquake frequencies that ranged in magnitude and depth.
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Space Weather and Link to Climate Change
A flow of charged particles released from the upper atmosphere of the Sun, called the corona. This plasma consists of mostly electrons, protons and alpha particles with kinetic energy between 0.5 and 10 keV . Embedded within the solar-wind plasma is the interplanetary magnetic field. The solar wind varies in density, temperature and speed over time and over solar latitude and longitude. Its particles can escape the Sun's gravity because of their high energy resulting from the high temperature of the corona, which in turn is a result of the coronal magnetic field.
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Advances in Electromagnetic Environmental Shielding for Aeronautics and Space Applications
Steam of charged particles or plasma based on electrons, protons, and alpha particles with kinetic energy between 0.5 and 10 keV released from the upper atmosphere of the sun.
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