F. N. Beg
University of California, San Diego
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Featured researches published by F. N. Beg.
Physics of Plasmas | 1997
F. N. Beg; A. R. Bell; A. E. Dangor; C. Danson; Ap Fews; M. E. Glinsky; B. A. Hammel; P. Lee; P. A. Norreys; M. Tatarakis
The interaction of a 1053 nm picosecond laser pulse with a solid target has been studied for focused intensities of up to 1019 W cm−2. The maximum ion energy cutoff Emax (which is related to the hot electron temperature) is in the range 1.0–12.0 MeV and is shown to scale as Emax≈I1/3. The hot electron temperatures were in the range 70–400 keV for intensities up to 5×1018 W cm−2 with an indication of a high absorption of laser energy. Measurements of x-ray/γ-ray bremsstrahlung emission suggest the existence of at least two electron temperatures. Collimation of the plasma flow has been observed by optical probing techniques.
Physics of Plasmas | 2001
S. V. Lebedev; F. N. Beg; S. N. Bland; J. P. Chittenden; A. E. Dangor; M. G. Haines; K. H. Kwek; S. A. Pikuz; T. A. Shelkovenko
A phenomenological model of wire array Z-pinch implosions, based on the analysis of experimental data obtained on the mega-ampere generator for plasma implosion experiments (MAGPIE) generator [I. H. Mitchell et al., Rev. Sci. Instrum. 67, 1533 (1996)], is described. The data show that during the first ∼80% of the implosion the wire cores remain stationary in their initial positions, while the coronal plasma is continuously jetting from the wire cores to the array axis. This phase ends by the formation of gaps in the wire cores, which occurs due to the nonuniformity of the ablation rate along the wires. The final phase of the implosion starting at this time occurs as a rapid snowplow-like implosion of the radially distributed precursor plasma, previously injected in the interior of the array. The density distribution of the precursor plasma, being peaked on the array axis, could be a key factor providing stability of the wire array implosions operating in the regime of discrete wires. The modified “initial...
The Astrophysical Journal | 2002
S. V. Lebedev; J. P. Chittenden; F. N. Beg; S. N. Bland; A. Ciardi; D. J. Ampleford; S. Hughes; M. G. Haines; Adam Frank; Eric G. Blackman; Thomas Anthony Gardiner
We present the first results of astrophysically relevant experiments where highly supersonic plasma jets are generated via conically convergent flows. The convergent flows are created by electrodynamic acceleration of plasma in a conical array of fine metallic wires (a modification of the wire array Z-pinch). Stagnation of plasma flow on the axis of symmetry forms a standing conical shock effectively collimating the flow in the axial direction. This scenario is essentially similar to that discussed by Canto and collaborators as a purely hydrodynamic mechanism for jet formation in astrophysical systems. Experiments using different materials (Al, Fe, and W) show that a highly supersonic (M ~ 20), well-collimated jet is generated when the radiative cooling rate of the plasma is significant. We discuss scaling issues for the experiments and their potential use for numerical code verification. The experiments also may allow direct exploration of astrophysically relevant issues such as collimation, stability, and jet-cloud interactions.
Physics of Plasmas | 1999
P.A. Norreys; M. I. K. Santala; E.L. Clark; Matthew Zepf; I. Watts; F. N. Beg; K. Krushelnick; M. Tatarakis; A. E. Dangor; X. Fang; Paul Graham; T. McCanny; R. P. Singhal; K.W.D. Ledingham; Alan Creswell; D.C.W. Sanderson; Joseph Magill; A. Machacek; J. S. Wark; R. Allott; B. Kennedy; D. Neely
Novel measurements of electromagnetic radiation above 10 MeV are presented for ultra intense laser pulse interactions with solids. A bright, highly directional source of γ rays was observed directly behind the target. The γ rays were produced by bremsstrahlung radiation from energetic electrons generated during the interaction. They were measured using the photoneutron reaction [63Cu(γ,n)62Cu] in copper. The resulting activity was measured by coincidence counting the positron annihilation γ rays which were produced from the decay of 62Cu. New measurements of the bremsstrahlung radiation at 1019 W cm−2 are also presented.
Applied Physics Letters | 2001
M. I. K. Santala; Matthew Zepf; F. N. Beg; E.L. Clark; A. E. Dangor; K. Krushelnick; M. Tatarakis; I. Watts; K.W.D. Ledingham; T. McCanny; I. Spencer; A. Machacek; R. Allott; Robert J. Clarke; P.A. Norreys
Nuclear activation has been observed in materials exposed to the ablated plasma generated from high intensity laser–solid interactions (at focused intensities up to 2×1019 W/cm2) and is produced by protons having energies up to 30 MeV. The energy spectrum of the protons is determined from these activation measurements and is found to be consistent with other ion diagnostics. The possible development of this technique for “table-top” production of radionuclides for medical applications is also discussed.
Physics of Plasmas | 2002
S. V. Lebedev; F. N. Beg; S. N. Bland; J. P. Chittenden; A. E. Dangor; M. G. Haines
The effect of discrete wires on the implosion dynamics of wire array Z-pinch experiments at ∼1 MA current level is discussed. The data show that the formation of a core–corona structure leads to gradual radial redistribution of mass by precursor plasma flow from the stationary wire cores during the first ∼80% of the implosion time. This phase ends with the formation of gaps in the wire cores, which occurs due to the nonuniformity of ablation rate along the wires. The final phase of the implosion starting at this time occurs as a rapid snowplow-like implosion of the plasma, previously injected into the interior of the array. The density distribution of the precursor plasma being peaked on the array axis could be a key factor providing stability of the wire array implosions operating in the regime of discrete wires. The implications of this implosion scenario to the operation of nested wire arrays and foam targets on the array axis are also discussed.
Physics of Plasmas | 2000
K. Krushelnick; E.L. Clark; Matthew Zepf; J.R. Davies; F. N. Beg; A. Machacek; M. I. K. Santala; M. Tatarakis; I. Watts; P.A. Norreys; A. E. Dangor
Energetic protons up to 30 MeV have been measured from high intensity laser interactions (⩽5×1019 W/cm2) with solid density plasmas. Up to 1012 protons (> 2 MeV) were observed at the rear of thin aluminum foil targets and measurements of their angular deflection were made. Similar energies were measured from ions produced from the front of the foils. Nuclear activation and track detector measurements suggest that the protons measured at the rear originate from the front surface of the target and are bent by large magnetic fields that exist in the plasma interior, which are likely generated by a laser-produced beam of fast electrons.
Journal of Applied Physics | 2000
F. N. Beg; I. Ross; A. Lorenz; J. F. Worley; A. E. Dangor; M. G. Haines
A study of a 2 kJ, 200 kA, table top plasma focus device as an intense x-ray source is reported. The x-ray yield from a number of gases, (deuterium, nitrogen, neon, argon, and xenon) is measured as a function of filling pressure and in neon as a function of anode length. In gases with Z<18, the plasma implodes to form a uniform cylindrical column, whereas for Z⩾18, the plasma consists of a number of hot spots. A maximum x-ray yield of 16.6 J and pulse length of 10–15 ns was obtained in neon. The x-ray emission was established to be due to H- and He-like line radiation. The temperature estimated from spectroscopic observations was about 300–400 eV at an electron density of (3–5)×1020 cm−3 in neon. At low pressures in neon, hard x-ray radiation, presumably due to electron beams was dominant. Mesh images of different wire materials were recorded at the optimum pressure in neon as a proof of principle for x-ray backlighting.
Plasma Physics and Controlled Fusion | 1998
P. A. Norreys; Ap Fews; F. N. Beg; A. R. Bell; A. E. Dangor; P. Lee; M B Nelson; H. Schmidt; Michael Tatarakis; M. D. Cable
Neutron fluxes of up to were measured when planar deuterated targets were irradiated with 1.3 ps FWHM (full width at half maximum) laser pulses at a wavelength of 1054 nm and focused intensities up to . The neutron energy spectra are consistent with an angularly dispersed beam target interaction, whereas a thermonuclear source is considered unlikely.
Review of Scientific Instruments | 2001
S. V. Lebedev; F. N. Beg; S. N. Bland; J. P. Chittenden; A. E. Dangor; M. G. Haines; M. Zakaullah; S. A. Pikuz; T. A. Shelkovenko; David A. Hammer
The dynamics of wire arrays have been studied using a point-projection X-pinch x-ray backlighter installed in one of the return posts of the MAGPIE generator. Variations of diameter (15–50 μm aluminum) and number of wires (two or four) in the X-pinch enabled backlit images in the range of 140–200 ns after the current start. A temporal and spatial resolution of <1 ns and 5 μm is achieved. The radiographic images of aluminum wire array show that the wire cores are present at the original position until 80% of the implosion time and the size of the wire cores is 0.25 mm for aluminum and 0.1 mm for tungsten. A very fine structure of the order of 10 μm has been observed in titanium wire arrays.