Show simple item record

Experimental Investigation of a High‐Energy Density, High‐Pressure Arc Plasma

dc.contributor.authorMartin, Edward Anthonyen_US
dc.date.accessioned2010-05-06T21:37:15Z
dc.date.available2010-05-06T21:37:15Z
dc.date.issued1960-02en_US
dc.identifier.citationMartin, Edward A. (1960). "Experimental Investigation of a High‐Energy Density, High‐Pressure Arc Plasma." Journal of Applied Physics 31(2): 255-267. <http://hdl.handle.net/2027.42/70092>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/70092
dc.description.abstractThe underwater spark is utilized to study the fundamental parameters of a plasma at 30 000°K and 10 000 atmos pressure. The 25‐kv spark is obtained by underwater discharge of capacitors having a stored energy of 1800 joules, the inertia of the water providing the confinement necessary to develop high pressures. Phenomena relating to the initiating wire (exploded wire) are discussed. Kerr cell photographs show that spherical structures are formed around both electrodes under certain conditions. A possible explanation is postulated. A detailed energy balance and particle balance are carried out. The results show that the plasma has great capability to store energy in dissociation, excitation, and ionization without a corresponding increase in temperature. The plasma is 30% ionized and the total particle density is about 2×1027 per cubic meter. At this density the plasma radiates a blackbody spectrum. Pressures are obtained by calculation based on the rate of spark channel expansion and the shock properties of water. The plasma is found to have an internal pressure of the same order of magnitude as the external pressure because of interparticle Coulomb forces. Plasma conductivity calculated from equations of Gvosdover and Spitzer and Harm agree very well with the experimental value. The study is basically experimental, with the emphasis in interpretation being placed on reliability of the conclusions rather than on refined accuracy.en_US
dc.format.extent3102 bytes
dc.format.extent1357157 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleExperimental Investigation of a High‐Energy Density, High‐Pressure Arc Plasmaen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumThe University of Michigan, Ann Arbor, Michiganen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/70092/2/JAPIAU-31-2-255-1.pdf
dc.identifier.doi10.1063/1.1735555en_US
dc.identifier.sourceJournal of Applied Physicsen_US
dc.identifier.citedreferenceH. C. Early and E. A. Martin, Communication and Electronics (American Institute of Electrical Engineers, New York, 1956), Vol. 22, p. 788.en_US
dc.identifier.citedreferenceH. H. Rust and H. Drubba, Z. angew. Phys. 5, 251 (1953).en_US
dc.identifier.citedreferenceLord Rayleigh, Proc. London Math. Soc. 10, 4 (1878).en_US
dc.identifier.citedreferenceW. Kleen, Ann. Physik 403, 579 (1931).en_US
dc.identifier.citedreferenceA star at 29 000 °K should have a greater absorption coefficient for red light than for blue light. See L. H. Aller, Astrophysics, the Atmospheres of the Sun and Stars (Ronald Press Company, New York, 1953), p. 186.en_US
dc.identifier.citedreferenceG. E. Gibson and W. Heitler, Z. Physik 49, 465 (1928).en_US
dc.identifier.citedreferenceR. H. Fowler, Statistical Mechanics (Cambridge University Press, Cambridge, 1936), second edition.en_US
dc.identifier.citedreferenceH. Maecker, Ergeb. exakt. Naturw. 25, 310 (1951).en_US
dc.identifier.citedreferenceL. Spitzer and R. Harm, Phys. Rev. 89, 977 (1953).en_US
dc.owningcollnamePhysics, Department of


Files in this item

Show simple item record

Remediation of Harmful Language

The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.

Accessibility

If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.