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Article (PDF, 280 KB).pdf

angeo-37-971-2019.pdf

🔗 Source: angeo.copernicus.org

📊 Size: 280 KB

📄 Pages: 18 pages

⬇️ Downloads: 63

Summary

The mirror mode in collisionless magnetized high-temperature plasmas develops an interesting macro-state, starting as a classical zero-frequency ion fluid instability that saturates quasi-linearly at a low magnetic level, forming elongated magnetic bubbles that trap the electron component. The trapped electrons interact with thermal ion sound waves, generating attractive wake potentials that lead to the formation of electron pairs in the lowest-energy singlet state. These pairs become spatially locked near the bounce-mirror points, contributing to a large anisotropy that breaks the quasi-linear stability and causes further growth of the mirror mode. The growth is compensated by either dissipation of the pairs and their anisotropy or inflow of plasma from the environment, potentially leading to localized diamagnetism.

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Description

The mirror mode in collisionless magnetized high-temperature plasmas develops an interesting macro-state, starting as a classical zero-frequency ion fluid...

Technical Information

File Format: PDF
File Size: 280 KB
Pages: 18
Language: EN
Total Downloads: 63
Last Updated: 3 weeks ago

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