Applying Nyquist's method for stability determination to solar wind observations
The role instabilities play in governing the evolution of solar and astrophysical plasmas is a matter of considerable scientific interest. The large number of sources of free energy accessible to such nearly collisionless plasmas makes general modeling of unstable behavior, accounting for the temper...
| Main Authors: | , , , |
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| Other Authors: | |
| Language: | en |
| Published: |
AMER GEOPHYSICAL UNION
2017
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| Online Access: | http://hdl.handle.net/10150/626568 http://arizona.openrepository.com/arizona/handle/10150/626568 |