1 / 25

Costello/Kennedy/Mosnier/van Kampen National Centre for Plasma Science & Technology (NCPST) and School of Physical S

CLPR Research in Laser Plasmas. Costello/Kennedy/Mosnier/van Kampen National Centre for Plasma Science & Technology (NCPST) and School of Physical Sciences, Dublin City University. Outline. The ‘Centre for Laser Plasma Research’ (CLPR)-NCPST- Who are we & what do we do ?

hue
Download Presentation

Costello/Kennedy/Mosnier/van Kampen National Centre for Plasma Science & Technology (NCPST) and School of Physical S

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. CLPRResearch in Laser Plasmas Costello/Kennedy/Mosnier/van Kampen National Centre for Plasma Science & Technology (NCPST) and School of Physical Sciences, Dublin City University

  2. Outline • The ‘Centre for Laser Plasma Research’ (CLPR)-NCPST-Who are we & what do we do ? • Table Top’ Laser Generated Plasma Basics • Projects

  3. NCPST/CLPRWho are we ? What do we do ?

  4. NCPST/ CLPR - Who are we ? • NCPST established with Irish Government funding (Euro 8M) in 1999. Now EU Training Site. • Consortium of new and existing laboratories in plasma physics, chemistry and engineering • Fundamental and Applied Scientific Goals • CLPR node is divided into 4(6) laboratories focussed on PLD and photoabsorption spectroscopy/ imaging (especially in UV - X-ray)

  5. The CLPR node comprises 6 laboratory areas focussed on pulsed laser matter interactions (spectroscopy/ imaging) Academic Staff (4):John T. Costello, Eugene T. Kennedy, Jean-Paul Mosnier and Paul van Kampen Post Doctoral Fesearchers (5): Dr. Deirdre Kilbane (PVK/JC) Dr. Hugo de Luna (JC) Dr. Jean-Rene Duclere (JPM) Dr. Pat Yeates (ETK) Dr. Mark Stapleton (JC) PhD students (8): Caroline Banahan (PVK/JC)Kevin Kavanagh (JC) Adrian Murphy (JC) John Dardis (JC) Jonathan Mullen (PVK) Rick O'Hare (JPM) Eoin O’Leary (ETK) Rebecca Treacy (PVK) Visiting PhD student (2):Michael Novotny (JPM) and Philip Orr (JC) Funded by: SFI - Frontiers and Investigator HEA - PRTLI and North-South IRCSET - Embark& BRGS Enterprise Ireland - BRGS EU - Marie Curie and RTD

  6. Research Theme Probing matter with fast and ultrafast UV, extreme-UV and X-ray pulses (Imaging/Spectroscopy in the UV - Soft X-Ray) Figure from lectures notes of David Attwood, U Calif.-Berkeley

  7. NCPST/ CLPR - What do we do ? DCU Pico/Nanosecond Laser Plasma Light Sources VUV, XUV & X-rayAtomic Absorption Spectroscopy VUV Photoabsorpion Imaging VUV LIPS for Analytical Purposes Pulsed Laser Deposition (PLD)/ICCD Imaging and Spectroscopy of PLD Plumes Aarhus/Berkeley Synchrotrons Photoion and Photoelectron Spectroscopy Hamburg - FEL Femtosecond IR+XUV Facility Development

  8. Part I - Table Top Laser-Plasma Basics

  9. Plasma & The 4 Phases of Matter Greek Philosophers Physicists Earth Solid Water Liquid Wind Gas FirePlasma Plasma: Fluid (gas) of electrons and ions

  10. How do you make a laser plasma ? Vacuum or Background Gas Target Plasma Assisted Chemistry Laser Pulse- 1 J/ 10 ns Lens Spot Size = 100 mm (typ. Diam.) F > 1011 W.cm-2 Te = 100 eV (~106 K) Ne = 1021 cm-3 Vexpansion 106 cm.s-1 Emitted - Atoms, Ions, Electrons, Clusters, IR - X-ray Radiation

  11. Intense Laser Plasma Interaction S Elizer, “The Interaction of High Power Lasers with Plasmas”, IOP Series in Plasma Physics (2002)

  12. In summary we know that:Laser Produced Fireballs are-Hot: Te = 105 - 108 KelvinDense: ne= 1021 e/cm3Transient: ps - msRapid: 106 - 107 cm/secDublin to Cork in 3 seconds !!!

  13. Laser - Astrophysical Plasmas - Solar Interior So now we know that laser plasmas are hot & dense ! We can tune temperature, density etc. so that they produce spectra to be compared with spectra from other laboratory and astrophysical sources !! Figure - David Attwood, U C Berkeley

  14. Laser Plasmas as VUV to X-ray Sources Since a laser plasma is HOT - (Te= 10 - 1000 eV) and (say) you consider it to be a black (or grey) body, then most emission should be at photon energies also in the 10 - 1000 eV range, i.e.,at Vacuum Ultraviolet (VUV),Extreme-Ultraviolet (EUV)and Soft X-ray (SXR) wavelengths !! Figure from lectures notes of David Attwood, U Calif.-Berkeley

  15. Generally Extreme-UV Science & Technology is Growing Rapidly Industry: Lithography Bio-Medical: Microscopy Basic Research: Astronomy

  16. Our Themes Laser Plasma Light Sources (dev & appls) Instrumentation and techniques Imaging and Spectroscopy in the UV, VUV, EUV and X-ray regions Physics of 1. 'Colliding Plasma Systems' 2. Structure and dynamics of atoms and ions

  17. DUAL LASER PLASMA (DLP) EXPERIMENTS UV - Xray Source Absorbing Sample

  18. Dual Laser Plasma (DLP) Photoabsorption J T Costello et al., Phys.Scr. T34, 77 (1991), E T Kennedy et al., Opt.Eng 33, 3984 (1994) No tuning required No vapour required Flexible Neutral/Multiplycharged/ Refractory Elements Dx, DT, I(W/cm2)  Species choice Backlighting Plasma Io Both Plasmas I = Ioe-snL Backlighter Relative Absorption Cross Section sNL =Ln(Io/I)

  19. TOF Oven Synchrotron - Photoion Results- BW3 Undulator XUV Radiation Li Vapour

  20. Photoionization as a plasma diagnostic VUV Photoabsorption Imaging VUV CCD Sample Io(x,y,t) I(x,y,t) Pass a collimated VUV beam through the plasma sample and measure the spatial distribution of the absorption. J Hirsch et al., J.Appl.Phys 88, 4953 (2000), Rev.Sci.Instrum (in press 2003)

  21. ULtrafast Emission and Absorption Photography Laser Beam Wedge Lens Target I-CCD Andor - Belfast <2 ns shutter time

  22. Colliding Plasmas Generate a Secondary Plasma !

  23. ‘Colliding Stars Model System' - 'Colliding Plasmas' Is that what's happening here ? NGC 2346

  24. Some Other Current Projects • Photoionization of ions with DLP setup in DCU, e.g. Mn2+, JPB Vol 38, L1 (2005) accessed > 500 times in <50 days! • First two-colourDLP (LP Continuum + Panther OPA) photoabsorption expts on ions - tests for FEL+OPA ? • Negative ion beams in intense 800 nm fields (QUB/MPI/ DCU) Phys. Rev. Lett 93, Art. No. 223001 (2004) • Photoionization of ions in merged synchrotron-ion beam experiments (Aarhus - Orsay/DCU/John West) • 'Clean'/ UHV laser plasma (dilute) ion source under development at DCU - possible source for synchrotron/ FEL expts ? • Laser plasma X-ray spectroscopy now available at DCU - Experience at 6 - 15 Angstrom (XFEL expt'l tests ?)

  25. Conclusions Lots happening and projects in: • UV - X-ray Sources - Lasers, Laser plasmas, Synchrotron & FEL - JC/ETK • Plasma probing with UV to X-ray radiation - spectroscopy & imaging - JC/ETK/PVK • Pulsed Laser Deposition & Diagnostics (with SSL) - JPM/EMG/MOH Lots of Int'l collaborations and opportunities to travel Come and talk with us if you are interested in lasers, plasmas, optics and atomic physics

More Related