Soft X-ray emissions related to the solar wind charge exchange observed by the X-ray satellite observatories

T. Ishida*, T. Kanda, H. Akamatsu, T. Enoki, K. Henmi, Y. Ishisaki, Y. Ezoe, T. Ohashi, K. Shinozaki, K. Mitsuda, H. Ohashi, L. Liu, J. Wang, H. Tanuma

*Corresponding author for this work

Research output: Contribution to journalConference articlepeer-review

1 Scopus citations

Abstract

We have observed the emission spectra in collisions of bare and hydrogen-like C and O ions with helium atoms and hydrogen molecules as target gases in the soft X-ray region using a window-less Si(Li) detector at collision energies around 100 keV. Because it is found that the 1s-2p emission is dominant in each spectrum, we indicate that the cascade from the upper states give the large population of the 2p state after the consideration using state-selective capture cross sections calculated by the TC-AOCC method.

Original languageEnglish
Article number082021
JournalJournal of Physics: Conference Series
Volume388
Issue numberPART 8
DOIs
StatePublished - 2012
Event27th International Conference on Photonic, Electronic and Atomic Collisions, ICPEAC 2011 - Belfast, United Kingdom
Duration: 2011/07/272011/08/02

ASJC Scopus subject areas

  • General Physics and Astronomy

Fingerprint

Dive into the research topics of 'Soft X-ray emissions related to the solar wind charge exchange observed by the X-ray satellite observatories'. Together they form a unique fingerprint.

Cite this