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The 2p-3d Electron Transition Multiplet of Ar +13 : A Stellar Density Diagnostic. Laura Heeter Kristina Naranjo-Rivera 2003-04. Introduction. Applications Density and temperature diagnostic for astrophysics Stellar corona, solar flairs Naturally occurring thermal plasma
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The 2p-3d Electron Transition Multiplet of Ar+13: A Stellar Density Diagnostic Laura Heeter Kristina Naranjo-Rivera 2003-04
Introduction Applications • Density and temperature diagnostic for astrophysics • Stellar corona, solar flairs • Naturally occurring thermal plasma • Chandra Observatory x-ray data
L-shell spectral peaks • Simple Structure • Density sensitivity (Å)
3d15/2 3d13/2 2p23/2 Metastable State 2p13/2 Forbidden Transition Ground State 2p11/2 Trabert et al. Study • Metastable level- 9.7 ms atomic lifetime
3d15/2 3d13/2 2p23/2 Metastable State 2p13/2 Forbidden Transition Ground State 2p11/2 Theory • Dr. Ming Feng-Gu • Peak intensities will invert with increased beam current density • Increased excitation to metastable state 2p13/2 Wavelength (Å)
Hypothesis • Sensitivity to beam current density • Increased electron excitation to metastable level
Objective Density EBIT Ar+13 Emission Spectra Electon Beam Ion Trap Stellar Object Ar+13 Emission Spectra Density?
Collector Liquid Helium Reservoir Liquid Nitrogen Reservoir Trapping Region Superconducting Helmholtz Magnet Electron Gun EBIT http://www-phys.llnl.gov/Research/EBIT/
Prepare EBIT Excite Ar to Ar+13 • Determine Constant Beam Energy Collect & Analyze Spectral Images Calculate Intensity Ratios Compare Experimental and Theoretical Data Methods
Results • Inverse relationship: beam current and intensity ratio
Results vs. Theory Wavelength (Å)
Comparison to Theoretical Models Ar+13 experimental data Monoenergetic beam Maxwellian plasma model Density (cm –3)
Discussion • Increased population of metastable state occurred as beam current density increased • Accuracy promises Ar+13 as a useful density diagnostic
Further Studies • Broader density range • Use other more abundant elements • Mg, Fe, Ni, and more • Currently Fe+21 is being tested
Acknowledgements • The EBIT Team • Dr. Peter Beiersdorfer • Edward Magee • Dr. Hui Chen • Dr. Elmar Träbert • Ming Feng-Gu • Ms. Fruen and the Research Class
The 2p-3d Electron Transition Multiplet of Ar+13: A Stellar Density Diagnostic Laura Heeter Kristina Naranjo-Rivera 2003-04
Elaboration of Methods: Analyze Ar+13 Spectra • Igor Pro • N+5 calibration • Sum like data
Calculate Intensity Ratios R = (I (3d5/2→2p3/2) + I (3d3/2→2p3/2)) / I(3d3/2→2p1/2)