Oscar Buneman

This article is about the British physicist. For his son, the British computer scientist, see Peter Buneman.
Oscar Buneman
Born (1913-09-28)28 September 1913
Died 24 January 1993(1993-01-24) (aged 79)
Institutions Stanford University[1]
Alma mater University of Manchester[2]
Doctoral advisor Douglas Hartree[2]
Doctoral students
Children Peter Buneman

Oscar Buneman (28 September 1913 – 24 January 1993) made advances in science, engineering, and mathematics. Buneman was a pioneer of computational plasma physics and plasma simulation.[1][4]

Career

In 1940 upon completion of his PhD with Douglas Hartree,[2] Buneman joined Hartree's magnetron research group assisting the development of radar during World War II. They discovered the Buneman–Hartree criterion for the voltage threshold of a magnetron operation. After the war, Buneman developed theories and simulations of collision-less dissipation of currents[5] called the Buneman instability. This is an example of anomalous resistivity or absorption. It is anomalous because the phenomenon does not depend on collisions. Buneman advanced elliptic equation solver methods and their associated applications (as well as for the fast Fourier transforms).

Personal life

On January 24, 1993, Oscar Buneman at the age of 79 died near Stanford University. The computer scientist Peter Buneman is his son.

Publications

References

  1. 1 2 Buneman, R.; Barker, R. J.; Peratt, A. L.; Brecht, S. H.; Langdon, A. B.; Lewis, H. R. (1994). "A tribute to Oscar Buneman - pioneer of plasma simulation". IEEE Transactions on Plasma Science. 22: 22. doi:10.1109/27.281546.
  2. 1 2 3 4 Oscar Buneman at the Mathematics Genealogy Project
  3. Holdren, John Paul (1970). Collisionless Stability of an Inhomogeneous, Confied, Planar Plasma (PhD thesis). Stanford University.
  4. Oscar Buneman's publications indexed by the Scopus bibliographic database, a service provided by Elsevier. (subscription required)
  5. Buneman, O. (1959). "Dissipation of Currents in Ionized Media". Physical Review. 115 (3): 503. doi:10.1103/PhysRev.115.503.


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