Latest Plasma Stories
Our Sun erupted on June 7, 2011, sending tons of hot plasma blasting into space. Some of the plasma fell back to the surface of the Sun, sparking bright flashes of ultraviolet light. A new study examines the dramatic event to provide new insights into how young stars grow by consuming nearby gas.
A new plasma cutter allows Bluff Manufacturing to perform all cutting in-house with increased accuracy and speed Fort Worth, Texas (PRWEB) May 13, 2013
Longevity Global Inc., renowned industrial equipment provider, is offering FORCECUT 42i plasma cutter at affordable price.
Researchers wrote in the journal Physics of Plasmas about experiments that helped reveal details of a cooling process that could potentially bring practical fusion closer.
Scientists at the University of Missouri have devised a new way to create and control plasma that could transform American energy generation and storage.
Together with NASA, University of Washington researchers believe it may be possible to use nuclear fusion to power a trip to Mars that is safe, inexpensive and only takes about a month.
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:
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