The quasi-steady states of collisionless plasmas in space (e.g., in the solar wind and planetary environments) are governed by the interactions of charged particles with wave fluctuations. These interactions are responsible not only for the dissipation of plasma waves but also for their excitation. The present analysis focuses on two instabilities, mirror and electromagnetic ion cyclotron instabilities, associated with the same proton temperature anisotropy
- Award ID(s):
- 1842643
- NSF-PAR ID:
- 10325729
- Date Published:
- Journal Name:
- Physics
- Volume:
- 3
- ISSN:
- 2624-8174
- Page Range / eLocation ID:
- 1175–1189
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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- Free Publicly Accessible Full Text
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Accepted Manuscript1.0
- Journal Article:
- https://doi.org/10.3390/ physics3040075
