Laboratory simulation of charge exchange - Produced x-ray emission from comets

P. Beiersdorfer, K. R. Boyce, G. V. Brown, H. Chen, S. M. Kahn, R. L. Kelley, M. May, R. E. Olson, F. S. Porter, C. K. Stahle, W. A. Tillotson

Research output: Contribution to journalArticle

Abstract

In laboratory experiments using the engineering spare microcalorimeter detector from the ASTRO-E satellite mission, we recorded the x-ray emission of highly charged ions of carbon, nitrogen, and oxygen, which simulates charge exchange reactions between heavy ions in the solar wind and neutral gases in cometary comae. The spectra are complex and do not readily match predictions. We developed a charge exchange emission model that successfully reproduces the soft x-ray spectrum of comet Linear C/1999 S4, observed with the Chandra X-ray Observatory.

Original languageEnglish (US)
Pages (from-to)1558-1559
Number of pages2
JournalScience
Volume300
Issue number5625
DOIs
StatePublished - Jun 6 2003

ASJC Scopus subject areas

  • General

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    Beiersdorfer, P., Boyce, K. R., Brown, G. V., Chen, H., Kahn, S. M., Kelley, R. L., May, M., Olson, R. E., Porter, F. S., Stahle, C. K., & Tillotson, W. A. (2003). Laboratory simulation of charge exchange - Produced x-ray emission from comets. Science, 300(5625), 1558-1559. https://doi.org/10.1126/science.1084373