X-Ray Spectroscopy of Highly Charged Ions in Laboratory and Astrophysical Plasmas

Published

September 1, 2010

Author(s)

E. H. Silver, N Brickhouse, T. Lin, G X. Chen, K. Kirby, John D. Gillaspy, Joseph N. Tan, J M. Laming

Abstract

This paper presents (1) new laboratory data on the x-ray spectra of He-like Ar XVII over a broad spectral range (300-3500 eV) at high resolution (2) the results of new measurements of K-shell x- ray reference lines in carbon, oxygen, iron, copper, and aluminum which were then used to obtain an absolute calibration of our x-ray microcalorimeter efficiency function, and (3) a review of our laboratory astrophysics research program. The data will be used to improve our laboratory measurements of Ne-like Fe XVII which, together with the new argon data presented here are useful for interpreting observations from NASA's orbiting Chandra X-ray Observatory.

Proceedings Title

Proceedings of the International Conference on Recent Advances in Spectroscopy: Theoretical, Astrophysical, and Experimental Perspectives

Conference Dates

January 28-31, 2009

Conference Location

Kodaikanal, IN

Pub Type

Conferences

Keywords

K-shell X rays, atomic spectroscopy, microcalorimeter, heliumlike argon XVII, neonlike iron XVII, efficiency calibration, electron beam ion trap (EBIT)

Citation

Silver, E. , Brickhouse, N. , Lin, T. , Chen, G. , Kirby, K. , Gillaspy, J. , Tan, J. and Laming, J. (2010), X-Ray Spectroscopy of Highly Charged Ions in Laboratory and Astrophysical Plasmas, Proceedings of the International Conference on Recent Advances in Spectroscopy: Theoretical, Astrophysical, and Experimental Perspectives, Kodaikanal, IN (Accessed April 16, 2024)