Presentation is loading. Please wait.

Presentation is loading. Please wait.

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

Similar presentations


Presentation on theme: "1 Magnetized Laboratory Plasmas and Astrophysical Jets …And Space Physics Dr. Robert Sheldon October 10, 2003."— Presentation transcript:

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

2 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 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 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 Feel free to correct my outdated or misinformed data.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 5/27 I. Astrophysical Jets

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

7 7/27 The Crab

8 8/27 Some jet theories…

9 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 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 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 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 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 14 II. Space Plasma Linacs

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

16 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 17/27 Nature abhors charge separation: Parallel Electric Field Theory Whipple, JGR 1977. 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 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 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 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 21/27 Quadrupole Electric Field: 1st Excited State of a Dipole B-field + + + + - - - -

22 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 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 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 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 26 III. Lab Plasma Accelerators

27 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 10-400 mTorr Simple Cheap

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

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

30 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 31/27 3 rd Lab Setup w/ Pyrex Bell Jar Laser Plasma

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

33 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 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 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 36/27

37 37/27

38 38/27

39 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 40/27 Some References Sheldon & Spurrier, "The Spinning Terrella Experiment", Phys. Plasmas, 8, 1111-1118, 2001. Sheldon, "The Bimodal Magnetosphere", Adv. Sp. Res., 25, 2347-2356, 2000. Sheldon, Spence & Fennel, "Observation of 40keV field-aligned beams", Geophys. Res. Lett. 25, 1617-1620, 1998. Several PowerPoint presentations All at: http://bex.nsstc.uah.edu/RbS/http://bex.nsstc.uah.edu/RbS/

41 41/27 The Magnetosphere in 1990

42 42/27 Better than Carnot


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

Similar presentations


Ads by Google