1 Magnetized Laboratory Plasmas and Astrophysical Jets …And Space Physics Dr. Robert Sheldon October 10, 2003.

Slides:



Advertisements
Similar presentations
Stellar Structure Section 6: Introduction to Stellar Evolution Lecture 18 – Mass-radius relation for black dwarfs Chandrasekhar limiting mass Comparison.
Advertisements

AGN Feedback at the Parsec Scale Feng Yuan Shanghai Astronomical Observatory, CAS with: F. G. Xie (SHAO) J. P. Ostriker (Princeton University) M. Li (SHAO)
UAH The Spinning Terrella Experiment: Lab Analog for Earth's Magnetosphere Robert Sheldon 1, Eric Reynolds 2 1 National Space Science and Technology Center,
Physics of fusion power
X X X X X10 14.
Star Birth How do stars form? What is the maximum mass of a new star? What is the minimum mass of a new star?
Who are the usual suspects? Type I Supernovae No fusion in white dwarf, star is supported only by electron degeneracy pressure. This sets max mass for.
Particle acceleration in plasma By Prof. C. S. Liu Department of Physics, University of Maryland in collaboration with V. K. Tripathi, S. H. Chen, Y. Kuramitsu,
Radio and X-ray emission in radio-quiet quasars Katrien C. Steenbrugge, Katherine M. Blundell and Zdenka Kuncic Instituto de Astronomía, UCN Department.
Accretion Processes in GRBs Andrew King Theoretical Astrophysics Group, University of Leicester, UK Venice 2006.
Neutron Stars and Black Holes Please press “1” to test your transmitter.
The Solar Corona and Solar Wind Steven R. Cranmer Harvard-Smithsonian Center for Astrophysics.
Neutron Stars and Black Holes
X-ray polarisation: Science
1 Galactic Groupings and Active Galactic Nuclei Topics Clusters and superclusters; Giant Elliptical Formation Starburst and other explosive galaxies; Seyferts,
Physics of fusion power Lecture 6: Conserved quantities / Mirror device / tokamak.
INTRODUCTION OF WAVE-PARTICLE RESONANCE IN TOKAMAKS J.Q. Dong Southwestern Institute of Physics Chengdu, China International School on Plasma Turbulence.
The Acceleration of Anomalous Cosmic Rays by the Heliospheric Termination Shock J. A. le Roux, V. Florinski, N. V. Pogorelov, & G. P. Zank Dept. of Physics.
Fusion Physics - Energy Boon or Nuclear Gloom? David Schilter and Shivani Sharma.
Coronal radiation belts? H. S. Hudson Space Sciences Lab, UC Berkeley.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
Physics of fusion power Lecture 8: Conserved quantities / mirror / tokamak.
Neutron Stars and Black Holes PHYS390: Astrophysics Professor Lee Carkner Lecture 18.
Finite Temperature Effects on VLF-Induced Precipitation Praj Kulkarni, U.S. Inan and T. F. Bell MURI Review February 18, 2009.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections
Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15 “How will we see when the sun goes dark?” “We will be forced to grope and feel our way.”
A Critical Role for Viscosity in the Radio Mode AGN Feedback Cycle Paul Nulsen Harvard-Smithsonian Center for Astrophysics 2014 July 9X-ray View of Galaxy.
F. Cheung, A. Samarian, W. Tsang, B. James School of Physics, University of Sydney, NSW 2006, Australia.
MMFW Madison, Wisconsin 6 May 2011 D.J. Den Hartog, R. M. Magee, S.T.A. Kumar, V.V. Mirnov (University of Wisconsin–Madison) D. Craig (Wheaton College)
Physics of fusion power Lecture 7: particle motion.
Quasars and Other Active Galaxies
Tuija I. Pulkkinen Finnish Meteorological Institute Helsinki, Finland
F.M.H. Cheung School of Physics, University of Sydney, NSW 2006, Australia.
Active Galaxy Jets – An exhausting business Diana Worrall University of Bristol.
1 Rockets, Stars & Jars Hot on the trail of cosmic plasma accelerators Dr. Robert Sheldon February 19, 2003.
Kinetic Effects on the Linear and Nonlinear Stability Properties of Field- Reversed Configurations E. V. Belova PPPL 2003 APS DPP Meeting, October 2003.
1 Mirror Mode Storms in Solar Wind and ULF Waves in the Solar Wind C.T. Russell, L.K. Jian, X. Blanco-Cano and J.G. Luhmann 18 th STEREO Science Working.
Electromagnetically Trapped Dusty Plasma Ring R. Sheldon, E. Thomas Jr, D. Gallagher, M. Adrian, M. Abbas, P. Craven & E. Reynolds Wheaton College / National.
Comparisons of Inner Radiation Belt Formation in Planetary Magnetospheres Richard B Horne British Antarctic Survey Cambridge Invited.
Basic Electronics By Asst Professor : Dhruba Shankar Ray For B.Sc. Electronics Ist Year 1.
High energy Astrophysics Mat Page Mullard Space Science Lab, UCL 6. Jets and radio emission.
Plasma universe Fluctuations in the primordial plasma are observed in the cosmic microwave background ESA Planck satellite to be launched in 2007 Data.
Computational Model of Energetic Particle Fluxes in the Magnetosphere Computer Systems Yu (Evans) Xiang Mentor: Dr. John Guillory, George Mason.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
The Last Epoch Sections Reminders Don’t forget about weekly reflections… Should I drop the 2 lowest weekly reflections? Should I drop the 3.
Space Science MO&DA Programs - September Page 1 SS It is known that the aurora is created by intense electron beams which impact the upper atmosphere.
In Situ Measurements of Auroral Acceleration Regions Wu Tong
The X-ray Universe Sarah Bank Presented July 22, 2004.
Field-Aligned Potentials Robert Sheldon 1, Dennis Gallagher 1, Mian Abbas 1, Mark Adrian 1, Paul Craven 1, Edward Thomas, Jr 2 1 NASA/Marshall Space Flight.
High gradient acceleration Kyrre N. Sjøbæk * FYS 4550 / FYS 9550 – Experimental high energy physics University of Oslo, 26/9/2013 *k.n.sjobak(at)fys.uio.no.
1 The Spinning Magnet Accelerator Cosmic CERNs and SLACs Robert Sheldon April 12, 2001.
Death of Stars II Physics 113 Goderya Chapter(s): 14
Quasars and Other Active Galaxies
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
Super Massive Black Holes The Unknown Astrophysics of their initial formation.
Magnetic Reconnection in Plasmas; a Celestial Phenomenon in the Laboratory J Egedal, W Fox, N Katz, A Le, M Porkolab, MIT, PSFC, Cambridge, MA.
GR/MHD SIMULATIONS OF JET-LAUNCHING Collaborators: J.P. De Villiers, J.F. Hawley, S. Hirose.
Ion effects in low emittance rings Giovanni Rumolo Thanks to R. Nagaoka, A. Oeftiger In CLIC Workshop 3-8 February, 2014, CERN.
UAH Ionospheric Sources of Storm-time RC and Plasmasheet Populations R. B. Sheldon The University of Alabama in Huntsville.
Chapter 21 Galaxy Evolution Looking Back Through Time Our goals for learning How do we observe the life histories of galaxies? How did galaxies.
Helically Symmetry Configuration Evidence for Alfvénic Fluctuations in Quasi-Helically Symmetric HSX Plasmas C. Deng and D.L. Brower, University of California,
Introduction to Space Weather Jie Zhang CSI 662 / PHYS 660 Spring, 2012 Copyright © The Sun: Magnetic Structure Feb. 16, 2012.
= Boozer g= 2*1e -7 *48*14*5361 =.7205 =0 in net current free stellarator, but not a tokamak. QHS Mirror Predicted Separatrix Position Measurements and.
What is the Origin of the Frequently Observed v -5 Suprathermal Charged-Particle Spectrum? J. R. Jokipii University of Arizona Presented at SHINE, Zermatt,
High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.
NIMROD Simulations of a DIII-D Plasma Disruption S. Kruger, D. Schnack (SAIC) April 27, 2004 Sherwood Fusion Theory Meeting, Missoula, MT.
Pulsars: the Magnetosphere and the γ-ray emission
Wakefield Accelerator
Fermi Bubble Z.G.,Xiong.
AGN: Quasars By: Jay Hooper.
Presentation transcript:

1 Magnetized Laboratory Plasmas and Astrophysical Jets …And Space Physics Dr. Robert Sheldon October 10, 2003

2/27 Abstract Despite the high conductivity of laboratory and space plasmas, which cause most theorists to treat them as quasi-neutral fluids, inhomogeneous magnetic fields can produce and support quite large potential differences, even along field lines. The theory of field-aligned potentials is several decades old, but remains a neglected part of plasma theory and experiment. We present some in situ spacecraft measurements and laboratory results suggesting the presence of these parallel electric fields. Should these fields scale to stellar sizes, they could easily exceed the 1.1MV threshold for pair production, and generate positron jets. We model the astrophysical system with a laboratory angular magnet, and demonstrate the dual jet-like features of this steady state system. We argue that this electric quadrupole, far from being a peculiar laboratory curiosity, is the energetically favored, first excited state of a magnetic dipole+plasma. If so, it may explain the ubiquity of non-thermal, energetic jets in astrophysical plasmas.

3/27 Talk Outline I.Astrophysical Jets A.Apologies B.Characteristics of Astrophysical Jets II.Space Plasma LINACs A.Resonant vs Non-resonant B.The spinning magnet linac III.Laboratory Plasma Physics A.Field-aligned voltages B.Dusty plasmas

4/27 Apologies I’m a space plasma guy, so please excuse my astrophysical chutzpah as enthusiasm for cross-disciplinary studies. Much of the jet research reflects a research proposal compiled 6 years ago. Feel free to correct my outdated or misinformed data. This presentation falls between disciplines—it has too much data & not enough theory for an astrophysicist, too little data & too much theory for space plasma physics.

5/27 I. Astrophysical Jets

6/27 Herbig-Haro Objects: YSO Stars with Accretion Disks HH30

7/27 The Crab

8/27 Some jet theories…

9/27 Necessary Conditions for Jets (Proceedings of 1993 Astrophysical Jets Symposium, ed. J.Pringle) Strong Magnetic field Determined by synchrotron radiation Accretion disk Large angular momentum Central attractor—BH, neutron star star Compact (esp. compared to jets) 15 minute variation in AGN variability Spinning? Hot? (nonthermal emission)

10/27 Why would I study jets? The usual suspects: cool, mystery, funding… Cool: It sure beats space physics in photogenicity. Mystery: No accepted explanation in 40 years. Funding: n/a Some unusual aspects of jets: Practicality. Its huge cosmic scaling (km  parsecs) suggests a robust mechanism that has wide application. It may solve the energy problem here on Earth. I may be able to make a cheap ion source for my lab.

11/27 Jets, Entropy, and Heat Engines X-rays are usually non-thermal. if thermal they would cool too fast Synchrotron is by definition non-thermal Non-thermal=low entropy (S) =acceleration Acceleration is either 1-step, multi-step Multistep is either resonant or stochastic Most efficient is 1-step, but with smallest entropy Ultimate energy source that drives jet is either nuclear (stars) or gravitational (BH) = high-S High-S Heat  Low-S Acceleration = Heat Engine. (think: jet engine)

12/27 Deep field image taken by HST, showing galaxies as far as the eye can see. Some percentage of these are x-ray emitters. This suggests that the Xray continuum is really discrete Xray objects in the sky. Visible vs Xray: HST deep field

13/27 God’s Heat Engine If all those discrete x-ray sources are associated with jets, then it makes this jet mechanism the most ubiquitous heat engine in the universe. In some sense then, it is the most efficient heat engine possible, or else it wouldn’t be so common. We might be able to domesticate it for terrestrial use—e.g. better than Carnot

14 II. Space Plasma Linacs

15/27 B-field aligned “beams” Trapped H+ 43keV O+ Beams!

16/27 Beams as 1-step accelerators Are the beams stochastically accelerated? No. Little evidence of pitch-angle scattering O+ dominates BELOW H+ in the ionosphere. In order to produce O+, it must be rapidly extracted from D-region without equilibriating with H+. Are the beams multi-step (Fermi) accelerated? Fermi acceleration aka ionospheric pressure cooker, needs a parallel E-field too. In which case, 1-step is faster than multi-step. 1-step=40kV E // is simplest theory

17/27 Nature abhors charge separation: Parallel Electric Field Theory Whipple, JGR Ne = Ni, quasi-neutrality (Wheaton grad 1953?) Different pitchangles for Ions and electrons  n kT e || E Wouldn’t E-field bring ions back to electrons?

18/27 Heuristics for Parallel-E Formation: Bouncing keeps H + & e - apart. E-field Bouncing motion of ion in a magnetic mirror B-field (dipole) looks like marble rolling in a bowl.

19/27 Necessary Conditions for E || in Space Inhomogeneous strong B-field such that grad-B drifts dominate over ExB. (Dipole field) Source of hot plasma Injected directly (accretion disks) Convected from elsewhere (plasmasheet) Spinning central magnet? Result: Rim feed, axial exit accelerator. Efficient Hot, non-thermal Xray source. This matches all the criteria for AP jets!

20/27 Rough Theory of the Mechanism Hot plasma trapped in an inhomogeneous field will produce E //, i.e. quadrupolar space charge. Size of E // depends on several factors: Driving plasma source rate—accretion rate Temperature of the source Loss rate due to scattering, radiation, etc. Strength of the inhomogeneous B-field gradient When the E-field > 1.11 MeV, pair- production begins, and positrons are accelerated into a beam. (YSO’s may be accelerating H+)

21/27 Quadrupole Electric Field: 1st Excited State of a Dipole B-field

22/27 Some thoughts on the driver In our Earth observations, the driver was ExB drift of warm (10keV) plasmasheet plasma, which sets up an instability with the ionosphere. In astrophysical jets, much hotter plasma from an accretion disk is available. See, for example, Jovian plasma torus. In this case, synchrotron cooling of hot electrons leads to the quadrupolar space charge distribution. Thus, multiple drivers cause an energy density increase, expressed as quadrupolar E-field.

23/27 Why is the jet so collimated? 1)It comes from a very small source 2)Global magnetic fields further collimate it upon exiting the core dipole 3)Current carried by the jet (it’s non- neutral after all) does some self- collimation, and may balance self- repulsion. 4)We really need some relativistic MHD simulations to do this self- consistently….

24/27 Can plasma power blazar jets? (not to mention stars, neutron stars, quasars…) The maximum E // of a plasma is limited by 2nd order forces ((F x B) x B) that short out E. Using typical numbers for YSO fields, we get limiting energies of keV - MeV.(Rothwell97) Applying same formula to blazar jets, we get ~1 GeV. Precisely the value that explains observations! Objection: black holes power blazars. How does plasma affect BH gravitational equilibrium? Theorists don’t know yet. GR +E&M = ad hoc. A single plasma mechanism may explain all AP jets.

25/27 Jet Scaling If Blazars have 2AU sized dipoles, and microquasars are 10’s of km, then this mechanism scales by factors of 10 million. Can we build one in the laboratory? High strength, inhomogeneous magnet Hot plasma source at equator Spinning? The Spinning Terrella Experiment

26 III. Lab Plasma Accelerators

27/27 1 st Experimental Setup w/electrode Bell jar, oil roughing pump, HV power supply, Nd-B ceramic magnet (low Curie temp!) Needle valve used to control the pressure from mTorr Simple Cheap

28/27 Arcs and Sparks=> Equator Potential 40s exposure Arcs follow B-field lines Arc completely around! Electrode spinningstationary

29/27 2 nd Lab Setup w/Biassed Magnet 1) N & e 2) Saturated 3)-400VDC 4) 0.5Tesla 5)10-200mT

30/27 Characteristics of Discharge KeV of Voltage Discharge lasts 30 microseconds Calculated milliCoulombs of charge Estimated nF capacitance of magnetic field In better vacuum (or collisionless plasma) potentials are limited by 2 nd order plasma drifts Result: Space charge accelerator (How do I know for sure? Dust tracer...)

31/27 3 rd Lab Setup w/ Pyrex Bell Jar Laser Plasma

32/27 Saturn’s Rings in the Lab 3  SiO 2 dust Dust Ring

33/27 Model for Jets So far, we have modelled the dipole field, but our “central attractor” is very space- filling. In astrophysical jets, the central attractor is much smaller than the accretion ring. Thus trapped plasma does not precipitate on the central attractor—the loss cone is small. We repeat the above experiments with an annular magnet, which simulates the astrophysical system. Same magnetic field polarity, same –400VDC applied voltage.

34/27 The 4 th Wheaton Bell Jar Setup Built in Experimental Physics class by Geoff Poore & Ben Noonan [2002] Moderate vacuum (10mTorr) oil- roughing pumped Pyrex bell jar Exploring toroidal magnetized DC glow discharge plasma geometry

35/27 Toroidal DC-glow discharge 2/17/03 Annular disk forming at dipole minimum Central jet forming at toroidal minimum Density contours perpendicular to B Asymmetric jet possibly due to spontaneous symmetry breaking

36/27

37/27

38/27

39/27 Conclusions We have some pretty pictures that look remarkably like astrophysical jets We have demonstrated a novel space- charge plasma configuration which is not very well described by current plasma theory We have an experimental system which we are still exploring with novel plasma diagnostics (dust tracers) We have interested several amateurs in building it—high school, undergrads…

40/27 Some References Sheldon & Spurrier, "The Spinning Terrella Experiment", Phys. Plasmas, 8, , Sheldon, "The Bimodal Magnetosphere", Adv. Sp. Res., 25, , Sheldon, Spence & Fennel, "Observation of 40keV field-aligned beams", Geophys. Res. Lett. 25, , Several PowerPoint presentations All at:

41/27 The Magnetosphere in 1990

42/27 Better than Carnot