Latest Plasma Stories
Cottonwood #13-6 goes from 5 BOPD to 57 BOPD an Increase of 1040% in oil production Houston, TX (PRWEB) October 01, 2013 Propell Technologies Group,
With its proprietary cold-plasma technology, IonField Systems will develop an automated instrument to clean plastic microtiter plates and reduce microtiter plate cost by 98%.
Scientists from the Heidelberg Max Planck Institute for Nuclear Physics (MPIK) in cooperation with DESY (Hamburg) at the synchrotron PETRA III have investigated for the first time X-ray absorption of highly charged iron ions.
One of the most frequently-used physics laboratories on the International Space Station recently completed its final set of experiments.
Recently, ArcBro.com, a well-known manufacturer of CNC cutting machine and plasma cutting equipment, has announced its special offer on CNC plasma cutters, up to 30% off. (PRWEB)
Recently, ArcBro.com, the well established manufacturer of CNC cutting machine and plasma cutting equipment, has released its new CNC pipe cutting equipment. (PRWEB)
A study published in the journal Annales Geophysicae provides the first conclusive proof of the existence of plasmaspheric wind.
Hannes Olof GÃ¶sta AlfvÃ©n (May 30, 1908 - April 2, 1995) was a Swedish plasma physicist born in NorrkÃ¶ping, Sweden. AlfvÃ©n received his PhD from the University of Uppsala in 1934. His thesis was titled "Investigations of the Ultra-short Electromagnetic Waves." He was originally trained as an electrical power engineer and later moved on to research and teaching in the fields of plasma physics. AlfvÃ©n made many contributions to plasma physics, including theories describing the...
Heliopause -- The heliopause is the boundary where our Sun's solar wind is stopped by the interstellar medium. The solar wind blows a "bubble" in the interstellar medium (the rareified hydrogen and helium gas that permeates the galaxy). The point where the solar wind's strength is no longer great enough to push back the interstellar medium is known as the heliopause, and is often considered to be the outer "border" of the solar system. The distance to the heliopause is not precisely...
Solar Prominence -- Solar prominences are large arch-shaped structures observable in the solar corona. These often have a twist and occasionally become unstable, ejecting plasma and magnetic flux out from the sun. The physics of solar prominence instability is believed to be governed by magnetic forces and magnetic helicity issues. It is thought that instability occurs when a magnetic flux tube becomes excessively twisted. ----- Click here to learn more on this topic from eLibrary:
- Withering but not falling off, as a blossom that persists on a twig after flowering.
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