THE STUDY OF COLD PLASMA GENERATION AT ATMOSPHERIC PRESSURE IN VARIOUS WORKING MEDIA

Veenu Goyal

Research Scholar CMJ, University, Shillong

Dr. Rajeev Kumar Pandey

Department of Physics, Approved Guide of CMJ University, Shillong, Meghalaya

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Abstract

References

1. Sturrock, Peter A. (1994). Plasma Physics: An Introduction to the Theory ofAstrophysical, Geophysical & Laboratory Plasmas. Cambridge University Press. ISBN 0521448107.
2. It is often stated that more than 99% of the material in the visible universe is plasma. See, for example, D. A. Gurnett, A. Bhattacharjee (2005). Introduction to PlasmaPhysics: With Space and Laboratory Applications. Cambridge, UK: Cambridge University Press. p. 2. ISBN 0521364833. andK Scherer, H Fichtner, B Heber (2005). Space Weather: The Physics behind a Slogan. Berlin: Springer. p. 138. ISBN 3540229078. Essentially, all of the visible light from space comes from stars, which are plasmas with a temperature such that they radiate strongly at visible wavelengths. Most of the ordinary (or baryonic) matter in the universe, however, is foundin the intergalactic medium, which is also a plasma, but much hotter, so that it radiates primarily as X-rays. The current scientific consensus is that about 96% of the total energydensity in the universe is not plasma or any other form of ordinary matter, but a combination of cold dark matter and dark energy
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