We are particularly interested in interstellar medium (ISM) phenomena which can be described by the laws of plasma physics. This is appropriate since nearly all of the ISM phases possess sufficient ionization for plasma behavior.
It is entirely possible that the most important discovery in astronomy of the next decade will not come from an astronomical telescope, but from a physics laboratory experiment.
The coming years will be a golden era for interstellar magnetism studies, due to recent advances in radioastronomical techniques such as rotation measure synthesis...as well as the prospect of major new radio telescopes which are being planned or are under construction.
...turbulence almost certainly plays an important role in the astrophysics of the ISM. Turbulence-associated magnetic field fluctuations govern the diffusion and propagation of charged particles in the galaxy...interstellar turbulence is almost certainly responsible for determining fundamental transport coefficients such as viscosity, resistivity, and thermal conductivity. Knowledge of the values of these transport coefficients is crucial for developing credible mathematical
models of the ISM.
To understand the evolutionary processes which govern the interstellar medium, it is necessary to know its basic physical properties, and the variation in these properties from one place to another. These basic properties consist of the fundamental “plasma parameters” such as electron density, elemental composition, ionization fraction, magnetic field strength, electron temperature, ion temperature, and (if possible) the functional form of the electron and ion distribution...
Magnetic field reconnection is one of the foremost topics in basic plasma physics and astrophysical plasma physics. The importance of reconnection in astrophysics is that the considerable energy in magnetic fields can be released, plasma flows generated, and perhaps particles accelerated in electric fields generated in the reconnection regions...It seems that magnetic reconnection and its associated current sheets must arise in the interstellar medium. Faraday rotation measurements of extragalactic radio sources show random variations from one line of sight to another...
Observational research could consist of additional, higher spatial-density Faraday rotation measurements of extragalactic radio sources to identify regions of high magnetic shear...These regions could then be inspected for other anomalies, such as enhanced heating or plasma flows
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The Interstellar Medium in a Can: Laboratory Experiments of Relevance to ISM Astrophysics