1 / 13

John J. Curry Atomic Spectroscopy Group National Institute of Standards and Technology physics.nist.gov/Divisions/Div84

John J. Curry Atomic Spectroscopy Group National Institute of Standards and Technology physics.nist.gov/Divisions/Div842/Gp1/index.html. What are the highest priority atomic data needs emerging from High-Energy Density Laboratory Plasma research?. jjcurry@nist.gov. Atomic Spectra Database

zariel
Download Presentation

John J. Curry Atomic Spectroscopy Group National Institute of Standards and Technology physics.nist.gov/Divisions/Div84

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. John J. Curry Atomic Spectroscopy Group National Institute of Standards and Technology physics.nist.gov/Divisions/Div842/Gp1/index.html

  2. What are the highest priority atomic data needs emerging from High-Energy Density Laboratory Plasma research? jjcurry@nist.gov

  3. Atomic Spectra Database • Measurements of highly-charged ions in EBIT • Non-LTE plasma modeling

  4. Contributors: Yuri Ralchenko John Gillaspy Joseph Tan Joe Reader ASD Contributors Alexander Kramida Much of the work described here has received long-term support from The Department of Energy, Office of Fusion Energy Sciences

  5. http://physics.nist.gov/PhysRefData/ASD

  6. http://physics.nist.gov/PhysRefData/ASD

  7. Different ions

  8. W57+ W55+ W56+ W58+ W61+ W60+ W59+ W54+ W62+ EBIT spectra of W (Ebeam = 8.8 keV) EXP IONS: W54+ - W63+ Modeling: 6600 levels > 1 million transitions THEORY All strong lines were identified as the n=3-n=3 transitions (E1 and M1)

  9. Non-LTE Databases http://nlte.nist.gov/NLTE4 http://nlte.nist.gov/SAHA

  10. Xe: level populations Ar: mean ion charge Au: ionization distribution

  11. FLYCHK at NIST:a complete time-dependent collisional-radiative code for online calculations http://nlte.nist.gov/FLY

More Related