Hall-magnetohydrodynamic waves in flowing ideal incompressible solar-wind plasmas: reconsidered
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s10509-020-3741-7.pdf
Reference30 articles.
1. Ballai, I., Thelen, J.C., Roberts, B.: Solitary waves in a Hall solar wind plasma. Astron. Astrophys. 404, 701 (2003). https://doi.org/10.1051/0004-6361:20030580
2. Birn, J., Galsgaard, K., Hesse, M., et al.: Forced magnetic reconnection. Geophys. Res. Lett. 32, L06105 (2005). https://doi.org/10.1029/2004GL022058
3. Cally, P.S., Khomenko, E.: Fast-to-Alfvén mode conversion mediated by the hall current. I. Cold plasma model. Astrophys. J. 814, 106 (2005). https://doi.org/10.1088/0004-637X/814/2/106
4. Chandrasekhar, S.: Hydrodynamic and Hydromagnetic Stability. Clarendon, Oxford (1961), Chap. 11
5. Edwin, P.M., Roberts, B.: Wave propagation in a magnetically structured atmosphere. III: The slab in a magnetic environment. Sol. Phys. 76, 239 (1982). https://doi.org/10.1007/BF00170986
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