dc.contributor.author |
Greenwood, J. B. |
en_US |
dc.contributor.author |
Williams, I. D. |
en_US |
dc.contributor.author |
Smith, S. J. |
en_US |
dc.contributor.author |
Chutjian, A. |
en_US |
dc.date.accessioned |
2004-09-23T22:08:24Z |
|
dc.date.available |
2004-09-23T22:08:24Z |
|
dc.date.issued |
2000-11-27 |
en_US |
dc.identifier.citation |
Physica scripta |
en_US |
dc.identifier.clearanceno |
00-2538 |
en_US |
dc.identifier.uri |
http://hdl.handle.net/2014/16480 |
|
dc.description.abstract |
Charge exchange followed by radiative stabilization are the main processes responsible for the recent observations of X-ray emission from comets in their approach to the Sun. A new apparatus was constructed to measure, in collisions of HCIs with atoms and molecules, (a) absolute cross sections for single and multiple charge exchange, and (b) normalized X-ray emission cross sections. |
en_US |
dc.format.extent |
347942 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en_US |
|
dc.subject.other |
charge exchange x-ray highly-charged ions comets |
en_US |
dc.title |
X-ray emission from charge exchange of highly-charged ions in atoms and molecules |
en_US |