Anode plasma dynamics in the self-magnetic-pinch diode
The self-magnetic-pinch diode is being developed as an intense electron beam source for pulsed-power-driven x-ray radiography. In high-power operation, the beam electrons desorb contaminants from the anode surface from which positive ions are drawn to the cathode. The counterstreaming electrons and...
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Published in: | Physical review special topics. PRST-AB. Accelerators and beams Vol. 14; no. 2; p. 024401 |
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American Physical Society
02-02-2011
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Abstract | The self-magnetic-pinch diode is being developed as an intense electron beam source for pulsed-power-driven x-ray radiography. In high-power operation, the beam electrons desorb contaminants from the anode surface from which positive ions are drawn to the cathode. The counterstreaming electrons and ions establish an equilibrium current. It has long been recognized, however, that expanding electrode plasmas can disrupt this equilibrium and cause rapid reduction of the diode impedance and the radiation pulse. Recently developed numerical techniques, which enable simultaneous modeling of particle currents with 10^{13} cm^{-3} densities to plasmas of near solid density, are applied to a model of the self-magnetic-pinch diode which includes the formation and evolution of anode surface plasmas. Two mechanisms are shown to cause rapid impedance loss, anode plasma expansion into the anode-cathode (A-K) gap, and increased ion space-charge near the cathode surface. The former mechanism dominates for shorter A-K gaps, while the latter dominates for longer gaps. Model results qualitatively reproduce the time-dependent impedances measured for this diode. |
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AbstractList | The self-magnetic-pinch diode is being developed as an intense electron beam source for pulsed-power-driven x-ray radiography. In high-power operation, the beam electrons desorb contaminants from the anode surface from which positive ions are drawn to the cathode. The counterstreaming electrons and ions establish an equilibrium current. It has long been recognized, however, that expanding electrode plasmas can disrupt this equilibrium and cause rapid reduction of the diode impedance and the radiation pulse. Recently developed numerical techniques, which enable simultaneous modeling of particle currents with 10^{13} cm^{-3} densities to plasmas of near solid density, are applied to a model of the self-magnetic-pinch diode which includes the formation and evolution of anode surface plasmas. Two mechanisms are shown to cause rapid impedance loss, anode plasma expansion into the anode-cathode (A-K) gap, and increased ion space-charge near the cathode surface. The former mechanism dominates for shorter A-K gaps, while the latter dominates for longer gaps. Model results qualitatively reproduce the time-dependent impedances measured for this diode. |
ArticleNumber | 024401 |
Author | Bruner, Nichelle Hahn, Kelly D. Oliver, Bryan V. Welch, Dale R. |
Author_xml | – sequence: 1 givenname: Nichelle surname: Bruner fullname: Bruner, Nichelle – sequence: 2 givenname: Dale R. surname: Welch fullname: Welch, Dale R. – sequence: 3 givenname: Kelly D. surname: Hahn fullname: Hahn, Kelly D. – sequence: 4 givenname: Bryan V. surname: Oliver fullname: Oliver, Bryan V. |
BackLink | https://www.osti.gov/biblio/1178289$$D View this record in Osti.gov |
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CitedBy_id | crossref_primary_10_1063_1_4916062 crossref_primary_10_1109_TPS_2021_3095221 crossref_primary_10_1109_TPS_2013_2275646 crossref_primary_10_1063_1_5013240 crossref_primary_10_1103_PhysRevAccelBeams_24_120401 crossref_primary_10_1103_PhysRevAccelBeams_22_120401 crossref_primary_10_1063_5_0089904 crossref_primary_10_1063_1_4794955 crossref_primary_10_1063_1_4978231 crossref_primary_10_1063_1_5109430 crossref_primary_10_1103_PhysRevAccelBeams_22_050401 crossref_primary_10_1063_1_5009014 crossref_primary_10_1063_1_5115800 crossref_primary_10_1063_5_0073971 crossref_primary_10_1103_PhysRevSTAB_17_050401 crossref_primary_10_1103_PhysRevAccelBeams_24_020402 crossref_primary_10_1063_1_5085507 crossref_primary_10_1063_1_4926580 crossref_primary_10_1063_1_5046945 crossref_primary_10_1103_PhysRevAccelBeams_24_060401 |
Cites_doi | 10.1103/PhysRevE.58.1163 10.1109/27.602496 10.1109/TPS.2008.917169 10.1063/1.3270471 10.1088/0022-3727/40/6/020 10.1063/1.2980418 10.1109/TPS.2010.2049128 10.1017/S0263034600011617 10.1109/JPROC.2004.829056 10.1109/TPS.2007.895227 10.12693/APhysPolA.115.1044 10.1109/TPS.2004.835956 10.1109/TPS.2005.845305 10.1116/1.1315200 10.1063/1.2207587 10.1103/PhysRev.22.347 10.1063/1.1592802 10.1016/0039-6028(79)90705-2 |
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References | PhysRevSTAB.14.024401Cc3R1 PhysRevSTAB.14.024401Cc2R1 B. Oliver (PhysRevSTAB.14.024401Cc6R1) 2009; 115 PhysRevSTAB.14.024401Cc14R1 PhysRevSTAB.14.024401Cc13R1 PhysRevSTAB.14.024401Cc16R1 PhysRevSTAB.14.024401Cc15R1 PhysRevSTAB.14.024401Cc21R1 PhysRevSTAB.14.024401Cc20R1 PhysRevSTAB.14.024401Cc12R1 PhysRevSTAB.14.024401Cc23R1 PhysRevSTAB.14.024401Cc11R1 D. R. Welch (PhysRevSTAB.14.024401Cc17R1) 1998; 16 PhysRevSTAB.14.024401Cc7R1 P. Redhead (PhysRevSTAB.14.024401Cc19R1) 1968 D. Johnson (PhysRevSTAB.14.024401Cc10R1) 2005 J. Threadgold (PhysRevSTAB.14.024401Cc1R1) 2003 PhysRevSTAB.14.024401Cc5R1 PhysRevSTAB.14.024401Cc4R1 PhysRevSTAB.14.024401Cc18R1 C. Vermare (PhysRevSTAB.14.024401Cc22R1) 1999; 27 PhysRevSTAB.14.024401Cc9R1 |
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