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Formation of interstellar clouds: Parker instability with phase transitions
Telemachos Ch Mouschovias
, Matthew W. Kunz
, Duncan A. Christie
Astronomy
Physics
Research output
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peer-review
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Dive into the research topics of 'Formation of interstellar clouds: Parker instability with phase transitions'. Together they form a unique fingerprint.
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Keyphrases
Phase Transition
100%
Galactic Plane
100%
Interstellar Clouds
100%
Parker Instability
100%
Cm(III)
66%
Magnetic Field Lines
66%
Magnetic Field Strength
66%
Nonlinear Evolution
66%
Physical Properties
33%
Two Dimensional
33%
Shock Waves
33%
Mean Density
33%
Flux Ratio
33%
Field Strength
33%
Spatial Dimension
33%
Density Field
33%
Maximum Density
33%
Nonlinear Phase
33%
Interstellar Medium
33%
Mean Magnetic Field
33%
Turbulent Velocity
33%
Sheet-like
33%
Nonlinear Perturbation
33%
Velocity Dispersion
33%
Almost Everywhere
33%
Cloudlet
33%
Cold Neutral Medium
33%
Warm Neutral Medium
33%
Physics
Interstellar Clouds
100%
Magnetic Field
100%
Field Strength
75%
Shock Wave
25%
Critical Temperature
25%
Interstellar Matter
25%
Mean Matter Density
25%
Cold Neutral Medium
25%
Warm Neutral Medium
25%