High Energy Density Laboratory Astrophysics 2008 2009
DOI: 10.1007/978-90-481-9999-0_27
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Collisionless interaction of an energetic laser produced plasma with a large magnetoplasma

Abstract: We have commissioned a high-energy glass-laser at the Large Plasma Device (LAPD) to study the interaction of a dense laser-produced plasma with a large (17 m) magnetized plasma. First experiments with an energy of the laser blow-off an order of magnitude higher than previous work (Gekelman et al. in J. Geophys. Res. 108(A7):1281, 2003) produced large amplitude Alfvén waves (δB ⊥ /B 0 ≈ 15%). We will discuss the potential of this facility for collisionless laboratory astrophysics experiments.

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Cited by 4 publications
(5 citation statements)
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“…The large spatial and temporal scales probed here are of further interest for astrophysicallyrelevant, laboratory-simulated collisionless shocks, where large spatial (several ion gyro-radii) and temporal (several ion gyro-periods) scales are required to form and propagate the shock [31,22]. This study presents the first step in measuring the temperature and density evolutions of these phenomena.…”
Section: Discussionmentioning
confidence: 83%
“…The large spatial and temporal scales probed here are of further interest for astrophysicallyrelevant, laboratory-simulated collisionless shocks, where large spatial (several ion gyro-radii) and temporal (several ion gyro-periods) scales are required to form and propagate the shock [31,22]. This study presents the first step in measuring the temperature and density evolutions of these phenomena.…”
Section: Discussionmentioning
confidence: 83%
“…Laboratory experiments of relevance to heliospheric magnetosonic shocks must fulfill a number of conditions, expressed in terms of dimensionless scaling parameters [ Drake , ; Constantin et al , ]. The piston must drive a magnetic pulse at supermagnetosonic speed ( M A = v shock / v A > 1) through the magnetized plasma long enough for coupling to occur ( τ Ω c i >1, where τ = L / v shock is the shock transit time, L is the ambient plasma size along the blow‐off axis, and Ω c i is the ambient ion cyclotron frequency).…”
Section: Methodsmentioning
confidence: 99%
“…Experiments in a quasi-parallel geometry will take advantage of the unsurpassed length of the ambient plasma column (D = 18 m). Previous experiments at lower power and sub-Alfvénic velocity [53,54] have shown that the blow-off from a solid target propagates as a high-density plasma-cloud over distances of several meters through the ambient plasma, when directed along the field lines. In H + at n i = 2 × 10 13 cm −3 and 350 G, the piston can then propagate over more than 300 c/ω pi .…”
Section: Collisionless Shocks In the Lapdmentioning
confidence: 99%
“…A new kilojoule-class laser system (Raptor) has been commissioned at the Phoenix laser-facility one floor above the LAPD for a new class of integrated experiments on exploding plasmas in the presence of a large magnetoplasma. The laser facility also includes a 35 J (5 ns at 1064 nm) Nd:silicate rod laser system (Phoenix) [53], and a 25 J / 6 Hz high-average-power slab laser [57]. Like similar high-energy lasers elsewhere [58][59][60][61][62] the new kilojoule-system includes recycled components from the decommissioned NOVA laser of Lawrence Livermore National Laboratory [63].…”
Section: High-energy Laser Systemmentioning
confidence: 99%