astrophysical plasma

This is usually not the case in fusion, space and astrophysical plasmas.

RFPs are also used in the study of astrophysical plasmas as they share many features.

He is a specialist on Space and Astrophysical Plasmas.

She has published papers on astrophysical plasma spectroscopy and structure and energy balance in cool star coronae.

It should be noted by the readers that most of the non-dark-matter universe is plasma and such plasma-processes are common in astrophysical plasma.

The well-known MHD with high magnetic Reynolds number, as the astrophysical plasma inside a star for example.

His research interests include plasma electrodynamics, with application to space and astrophysical plasmas, especially in the context of auroral and magnetospheric physics.

AstroGK: A code based on GS2 (above) for studying turbulence in astrophysical plasmas.

It is designed to gather information about the microphysics of magnetic reconnection, energetic particle acceleration, and turbulence, processes that occur in many astrophysical plasmas.

In astrophysical plasmas such as the solar corona, current sheets may have an aspect ratio (breadth divided by thickness) as high as 100,000:1.

He is the author of several papers on astrophysical plasmas, from the formation of stars, double layers, the Bennett Pinch, to interstellar helical filaments.

Many astrophysical systems are not in local thermal equilibrium, and therefore require an additional kinematic treatment to describe all the phenomena within the system (see Astrophysical plasma).

In astrophysical plasmas, Debye screening prevents electric fields from directly affecting the plasma over large distances, i.e., greater than the Debye length.

Their suitability to prepare and reproduce in a microscopic volume the conditions of high temperature astrophysical plasmas and magnetic confinement fusion plasmas make them very appropriate research tools.

MHD waves and oscillations are a popular tool for the remote diagnostics of laboratory and astrophysical plasmas, e.g. the corona of the Sun (Coronal seismology).

In 1958, Woltjer, working on astrophysical plasmas, noted that is conserved, which implies that a twisty field will attempt to maintain its twistyness even with external forces being applied to it.

With these properties, the primary scientific purpose of ASCA is the X-ray spectroscopy of astrophysical plasmas; especially the analysis of discrete features such as emission lines and absorption edges.

He concluded his lectured and later discloses that he worked as part of the team at Institute of Space and Planetary Astrophysics that worked on the astronomical objects, astrophysical plasma, and physical cosmology.

The Madison Symmetric Torus (MST) is a reversed field pinch (RFP) physics experiment with applications to both fusion energy research and astrophysical plasmas located at University of Wisconsin-Madison.

Both plasma physicists and astrophysicists are interested in active galactic nuclei, because they are the astrophysical plasmas most directly related to the plasmas studied in the laboratory, and those studied in fusion power experiments.

Compared to the sizes of the plasmas which contain them, double layers are very thin (typically ten Debye lengths), with widths ranging from a few millimeters for laboratory plasmas to thousands of kilometres for astrophysical plasmas.

It is one of the few observatories to utilize relatively low frequencies (10-88 MHz), and is used to study relativistic particles, cosmic evolution, astrophysical plasma, decametric radio emissions from Jupiter-like extrasolar planets, and giant flares from magnetars.

High velocity jets of controllable density and temperature allow astrophysical phenomena such as solar wind, galactic jets, solar events and astrophysical plasma to be partially simulated in the laboratory and measured directly, in addition to astronomic and satellite observations.

As a staff scientist his research interests include studying plasma kinetic physics and magnetohydrodynamics of the solar wind, heliosphere, shock waves, MHD and kinetic simulation of plasma instabilities, and turbulent processes associated with space, solar and astrophysical plasmas.

Besides theoretical and computer-simulated astrophysics and nuclear astrophysics (including important nuclear reactions and properties of unstable stellar cores, equations of state of quark-matter and core matter of higher density), he worked on the modeling of astrophysical plasmas for important subatomic processes.