75 research outputs found
Curved Herbig-Haro Jets: Simulations and Experiments
Herbig-Haro jets often show some degree of curvature along their path, in
many cases produced by the ram pressure of a side-wind. We present simulations
of both laboratory and astrophysical curved jets and experimental results from
laboratory experiments. We discuss the properties and similarities of the
laboratory and astrophysical flow, which show the formation of internal shocks
and working surfaces. In particular the results illustrate how the break-up of
the bow-shock and clumps in the flow are produced without invoking jet
variability; we also discuss how jet rotation reduces the growth of the
Rayleigh-Taylor instability in curved jets.Comment: 15 pages, 5 figure, accepted to be published in The Astrophysical
Journa
Jet Deflection via Cross winds: Laboratory Astrophysical Studies
We present new data from High Energy Density (HED) laboratory experiments
designed to explore the interaction of a heavy hypersonic radiative jet with a
cross wind. The jets are generated with the MAGPIE pulsed power machine where
converging conical plasma flows are produced from a cylindrically symmetric
array of inclined wires. Radiative hypersonic jets emerge from the convergence
point. The cross wind is generated by ablation of a plastic foil via
soft-X-rays from the plasma convergence region. Our experiments show that the
jets are deflected by the action of the cross wind with the angle of deflection
dependent on the proximity of the foil. Shocks within the jet beam are apparent
in the data. Analysis of the data shows that the interaction of the jet and
cross wind is collisional and therefore in the hydro-dynamic regime. MHD plasma
code simulations of the experiments are able to recover the deflection
behaviour seen in the experiments. We consider the astrophysical relevance of
these experiments applying published models of jet deflection developed for AGN
and YSOs. Fitting the observed jet deflections to quadratic trajectories
predicted by these models allows us to recover a set of plasma parameters
consistent with the data. We also present results of 3-D numerical simulations
of jet deflection using a new astrophysical Adaptive Mesh Refinement code.
These simulations show highly structured shocks occurring within the beam
similar to what was observed in the experimentsComment: Submitted to ApJ. For a version with figures go to
http://web.pas.rochester.edu/~afrank/labastro/CW/Jet-Wind-Frank.pd
Magnetic Tower Outflows from a Radial Wire Array Z-pinch
We present the first results of high energy density laboratory astrophysics
experiments which explore the evolution of collimated outflows and jets driven
by a toroidal magnetic field. The experiments are scalable to astrophysical
flows in that critical dimensionless numbers such as the Mach number, the
plasma beta and the magnetic Reynolds number are all in the astrophysically
appropriate ranges. Our experiments use the MAGPIE pulsed power machine and
allow us to explore the role of magnetic pressure in creating and collimating
the outflow as well as showing the creation of a central jet within the broader
outflow cavity. We show that currents flow along this jet and we observe its
collimation to be enhanced by the additional hoop stresses associated with the
generated toroidal field. Although at later times the jet column is observed to
go unstable, the jet retains its collimation. We also present simulations of
the magnetic jet evolution using our two-dimensional resistive
magneto-hydrodynamic (MHD) laboratory code. We conclude with a discussion of
the astrophysical relevance of the experiments and of the stability properties
of the jet.Comment: Accepted by MNRAS. 17 pages without figures. Full version with
figures can be found at
http://www.pas.rochester.edu/~afrank/labastro/MF230rv.pd
Exploring the parameter space of MagLIF implosions using similarity scaling. II. Current scaling
Magnetized Liner Inertial Fusion (MagLIF) is a magneto-inertial-fusion (MIF)
concept, which is presently being studied on the Z Pulsed Power Facility. The
MagLIF platform has achieved interesting plasma conditions at stagnation and
produced significant fusion yields in the laboratory. Given the relative
success of MagLIF, there is a strong interest to scale the platform to higher
peak currents. However, scaling MagLIF is not entirely straightforward due to
the large dimensionality of the experimental input parameter space and the
large number of distinct physical processes involved in MIF implosions. In this
work, we propose a novel method to scale MagLIF loads to higher currents. Our
method is based on similarity (or similitude) scaling and attempts to preserve
much of the physics regimes already known or being studied on today's Z
pulsed-power driver. By avoiding significant deviations into unexplored and/or
less well-understood regimes, the risk of unexpected outcomes on future
scaled-up experiments is reduced. Using arguments based on similarity scaling,
we derive the scaling rules for the experimental input parameters
characterizing a MagLIF load (as functions of the characteristic current
driving the implosion). We then test the estimated scaling laws for various
metrics measuring performance against results of 2D
radiation--magneto-hydrodynamic HYDRA simulations. Agreement is found between
the scaling theory and the simulation results.Comment: 19 pages, submitted to Physics of Plasma
Supersonic radiatively cooled rotating flows and jets in the laboratory
The first laboratory astrophysics experiments to produce a radiatively cooled
plasma jet with dynamically significant angular momentum are discussed. A new
configuration of wire array z-pinch, the twisted conical wire array, is used to
produce convergent plasma flows each rotating about the central axis. Collision
of the flows produces a standing shock and jet that each have supersonic
azimuthal velocities. By varying the twist angle of the array, the rotation
velocity of the system can be controlled, with jet rotation velocities reaching
~20% of the propagation velocity.Comment: Accepted for publication in Physical Review Letters (16 pages, 5
figures
The evolution of magnetic tower jets in the laboratory
The evolution of laboratory produced magnetic jets is followed numerically through three-dimensional, non-ideal magnetohydrodynamic simulations. The experiments are designed to study the interaction of a purely toroidal field with an extended plasma background medium. The system is observed to evolve into a structure consisting of an approximately cylindrical magnetic cavity with an embedded magnetically confined jet on its axis. The supersonic expansion produces a shell of swept-up shocked plasma which surrounds and partially confines the magnetic tower. Currents initially flow along the walls of the cavity and in the jet but the development of current-driven instabilities leads to the disruption of the jet and a re-arrangement of the field and currents. The top of the cavity breaks-up and a well collimated, radiatively cooled, 'clumpy' jet emerges from the system
Association of polymorphisms in CASP10 and CASP8 with FEV 1 /FVC and bronchial hyperresponsiveness in ethnically diverse asthmatics
Several chromosomal regions have been identified using family-based linkage analysis to contain genes contributing to the development of asthma and allergic disorders. One of these regions, chromosome 2q32-q33, contains a gene cluster containing CFLAR, CASP10 and CASP8. These genes regulate the extrinsic apoptosis pathway utilized by several types of immune and structural cells that have been implicated in the pathogenesis of asthma
Laboratory Studies of Astrophysical Jets
Jets and outflows produced during star-formation are observed on many scales:
from the "micro-jets" extending a few hundred Astronomical Units to the
"super-jets" propagating to parsecs distances. Recently, a new "class" of
short-lived (hundreds of nano-seconds) centimetre-long jets has emerged in the
laboratory as a complementary tool to study these complex astrophysical flows.
Here I will discuss and review the recent work done on "simulating"
protostellar jets in the laboratory using z-pinch machines.Comment: 25 Pages, 11 Figures to appear in Lecture Notes in Physics. Series
Title: Jets from young stars IV: From models to observations and experiments
Editors: P. J. V. Garcia and J. M. T. Ferreira. Publisher: Springe
Laboratory Astrophysics and Collimated Stellar Outflows: The Production of Radiatively Cooled Hypersonic Plasma Jets
We present 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 (), 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.Comment: 13 Pages, (inc 4 figs), LaTex, Submitted to ApJ Let
3D MHD Simulations of Laboratory Plasma Jets
Jets and outflows are thought to be an integral part of accretion phenomena
and are associated with a large variety of objects. In these systems, the
interaction of magnetic fields with an accretion disk and/or a magnetized
central object is thought to be responsible for the acceleration and
collimation of plasma into jets and wider angle flows. In this paper we present
three-dimensional MHD simulations of magnetically driven, radiatively cooled
laboratory jets that are produced on the MAGPIE experimental facility. The
general outflow structure comprises an expanding magnetic cavity which is
collimated by the pressure of an extended plasma background medium, and a
magnetically confined jet which develops within the magnetic cavity. Although
this structure is intrinsically transient and instabilities in the jet and
disruption of the magnetic cavity ultimately lead to its break-up, a well
collimated, knotty jet still emerges from the system; such clumpy morphology is
reminiscent of that observed in many astrophysical jets. The possible
introduction in the experiments of angular momentum and axial magnetic field
will also be discussed.Comment: 15 pages, 4 figures, accepted by Astrophysics and Space Science for
Special Issue High Energy Density Laboratory Astrophysics Conferenc
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