destruction of a magnetic mirror trapped hot electron
play

Destruction of a Magnetic Mirror-Trapped Hot Electron Ring by a - PowerPoint PPT Presentation

Destruction of a Magnetic Mirror-Trapped Hot Electron Ring by a shear Alfven Wave Y. Wang 1 , W. Gekelman 1 , P. Pribyl 1 , D. Papadopoulos 2 1 University of California, Los Angeles 2 University of Maryland, College Park Work supported by ONR MURI


  1. Destruction of a Magnetic Mirror-Trapped Hot Electron Ring by a shear Alfven Wave Y. Wang 1 , W. Gekelman 1 , P. Pribyl 1 , D. Papadopoulos 2 1 University of California, Los Angeles 2 University of Maryland, College Park Work supported by ONR MURI award ( Fundamental Physics Issues on Radiation Belt Dynamics and } Remediation ), performed at the Basic Plasma Science Facility which is supported by DOE and NSF

  2. Motivations and Background } Radiation Belt Remediation – Artificial method to control and drain the energetic particles trapped by the Earth’s magnetic field, which can be fed by natural source or human activities (such as High-altitude nuclear explosions) and pose hazards to space satellites. � } Rotating Magnetic Field (RMF) source -- * Image from NASA website The RMF source is an innovative method to efficiently launch waves in space plasmas. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 2

  3. Schematics of the experiment Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 3

  4. Hot electron ring generation Fast electrons are generated by Electron Cyclotron Resonant Heating (ECRH) at } f microwave = 2f ce. ( Peak Power = 15 kW, pulse duration = 30 ~ 50 ms) X-rays are measured outside the 3/8’’ stainless steel vacuum chamber, which cut off } x-ray transmission below 100keV. The perpendicular E field generates a hot electron population with large } perpendicular energies, which grad-B and curvature drift in the θ -direction and form a hot electron ring in the magnetic mirror. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 4

  5. Measurement of the ring size } The size and position of the hot electron } The axial extension of the ring is ring is measured by inserting a measured to be Δ z = 211 cm, which “luminator probe” along the positive x- corresponds to a minimum hot axis. The thickness of the ring is ~10cm electron pitch angle of 56 o (loss cone = 47 o ) B ( z ) & # 1 = 47 tan 1 max 1 56 − $ ! θ ° θ = − = ° min loss cone $ ! B % " min Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 5

  6. Rotating Magnetic Field (RMF) antenna Measured B Alfven vectors 2 m away from antenna } The RMF antenna is composed of 2 orthogonal coils, placed in x-z and y-z planes, with diameters of 8 cm and 9 cm. } Driven by 2 independent RF drivers, capable of launching waves with arbitrary polarity. } The shear Alfvén wave dispersion relation has been verified. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 6

  7. Disruption of the hot electron ring } The shear Alfvén wave significantly enhances hot electron loss, as evidenced by a burst of x-rays. } The x-ray signal is modulated at the Alfvén wave frequency. Signal averaged over 1200 shots Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 7

  8. } A population of fast electrons persists after the shut-off of the ECRH, and can be de-trapped by application of the shear Alfvén wave to produce X-ray bursts. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 8

  9. Electrons lost axially travel ~ 11m along the Electrons lost radially are most likely to strike } } magnetic field line to the anode. X-rays are the waveguide, which is the closest metallic generated on the mesh anode. object to the magnetic mirror. * Graph normalization: Parallel loss is about 2% of radial loss Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 9

  10. Alfvén ghost } The fast electrons loss is observed to continue even after the termination of the Alfvén wave. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 10

  11. Deformation of the hot electron ring } The ring becomes asymmetric in the Alfvén wave field. } The deformation of the ring gives rise to the oscillations in the x-ray signal at f=f Alfvén . Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 11

  12. Deformation of the hot electron ring } The ring becomes asymmetric in the Alfvén wave field. } The deformation of the ring gives rise to the oscillations in the x-ray signal at f=f Alfvén . Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 12

  13. Deformation of the hot electron ring } The ring becomes asymmetric in the Alfvén wave field. } The deformation of the ring gives rise to the oscillations in the x-ray signal at f=f Alfvén . Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 13

  14. Role of Alfvén wave polarization } LH and RH waves of same amplitude } LH and RH waves of arbitrary and arbitrary phases are mixed. amplitudes are mixed together to scatter the hot electrons. } The x-ray oscillation is phase locked to the RH component. } The x-ray intensity is only related to the amplitude of the RH component. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 14

  15. X-ray spectrum } X-ray spectrum is measured by analyzing pulse heights from the NaI(Tl) scintillator x-ray detector. The Alfvén wave de-trapping effect is observed for electrons with a broad range of energy. Radial loss Axial loss Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 15

  16. Proposed de-trapping mechanism } The hot electron ring is deformed in the non-uniform Alfvén wave field, most likely by the E wave × B 0 drift. It is proposed that the deformation accumulates if the ring azimuthal drift speed matches that of the rotation of the Alfvén wave pattern. } Collective modes of the ring, with three dimensional spatial distortion, can affect its confinement and lead to losses. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 16

  17. Summary The enhanced loss of fast electrons trapped in a magnetic mirror geometry irradiated } by shear Alfvén waves is studied by laboratory experiments. Magnetic mirror trapped fast electrons with energies up to 3 MeV are generated by 2 nd harmonic Electron } Cyclotron Resonance Heating Shear Alfvén waves are launched by a Rotating Magnetic Field antenna with arbitrary polarity } Irradiated by a right-handed circularly polarized shear Alfvén wave, the electrons are lost in both the radial and } axial direction with a modulated at f Alfvén . The loss continues even after the termination the wave. Test particle simulation confirms that the single particle motion of the trapped fast } electrons in presence of a shear Alfvén wave is not adequate to explain the experimental observation. No axial loss is observed in the test particle simulation with a wave amplitude measured in the } experiment It is proposed that the deformation of the hot electron ring drives a collective mode of } the ring that leads to electron losses from the magnetic mirror. Experimental evidence indicates deformation of the hot electron ring, most likely due to the E wave × B 0 } drift in the Alfvén wave field. The deformation grows when the electron azimuthal (grad-B and curvature) drift matches the rotation of the RH shear Alfvén wave. The non-uniform 3D charge distribution in the deformation builds up a large scale global electric field and leads to electron loss. Destruction of a magnetic mirror-trapped hot electron ring by a shear Alfvén wave � 17

  18. Planning next experiment… • Frequency 8.5-9.6 GHz • peak power 225 kW maximum • pulse width 0.5 us (or 2.4 us) • 0.1% duty cycle maximum � 18

  19. � 19

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend