Astrophysical plasma, a highly ionized gas found throughout the universe, is fundamental to the study of cosmic phenomena as it constitutes over 99% of the visible matter in the universe. Its behavior is governed by complex interactions between magnetic fields and charged particles, influencing phenomena from solar flares to the dynamics of galaxies and galaxy clusters.

Astrophysical Plasma

Highly ionized gas

Cosmic Phenomena

Visible matter in the universe

Magnetic fields are invisible forces generated by electric currents and magnetic materials, influencing the behavior of charged particles in their vicinity. They play a crucial role in various natural phenomena and technological applications, from Earth's magnetosphere to electromagnetic devices.

Magnetic Fields

Charged particles are fundamental components of matter that carry an electric charge, either positive or negative, and are influenced by electromagnetic fields. They play a crucial role in various physical phenomena, including electricity, magnetism, and the behavior of atoms and molecules.

Charged Particles

Solar flares are sudden and intense bursts of radiation from the sun's atmosphere, caused by the release of magnetic energy stored in the sun's atmosphere. These flares can affect space weather, disrupt communication systems on Earth, and pose risks to astronauts and satellites in space.

Solar Flares

Dynamics of galaxies

Galaxy clusters are the largest gravitationally bound structures in the universe, consisting of hundreds to thousands of galaxies along with dark matter and hot gas. They are crucial for understanding the large-scale structure of the cosmos and provide insights into the distribution and behavior of dark matter and the evolution of galaxies.

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