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Compressible magnetohydrodynamic turbulence in interstellar plasmas
Yoram Lithwick
*
, Peter Goldreich
*
Corresponding author for this work
Physics and Astronomy
Research output
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Contribution to journal
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Article
›
peer-review
274
Scopus citations
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Dive into the research topics of 'Compressible magnetohydrodynamic turbulence in interstellar plasmas'. Together they form a unique fingerprint.
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INIS
plasma
100%
density
100%
turbulence
100%
magnetohydrodynamics
100%
fluctuations
72%
length
63%
spectra
45%
protons
36%
entropy
36%
magnetic fields
27%
gases
18%
cooling
18%
shear
18%
damping
18%
mean free path
18%
constraints
9%
particles
9%
transport
9%
power
9%
ionization
9%
amplitudes
9%
radiowave radiation
9%
scintillations
9%
compressibility
9%
Physics
Magnetohydrodynamic Turbulence
100%
Interstellar Plasma
100%
Variations
100%
Spectra
62%
Protons
50%
Entropy
50%
Eddy
50%
Magnetic Fields
37%
Pressure
37%
Interstellar Matter
25%
Cooling
25%
Mean Free Path
25%
Gas Pressure
25%
Turbulence
25%
Region
25%
Shears
25%
Amplitudes
12%
Compressibility
12%
Ionization
12%
Scintillation
12%
Particle
12%