Abstract
X-ray spectra produced when 8.5 MeV amu-1 Fe, Kr and Nb ions are excited in collisions with a graphite target are reported. X-ray transitions originating in one-, two- and three-electron ions are observed and used to test the accuracy of the theoretical X-ray energy calculations. The production probabilities for Li-, He- and H-like ions were determined from the relative gamma -ray line strengths and centroid line energies.
| Original language | English (US) |
|---|---|
| Article number | 008 |
| Pages (from-to) | 3545-3549 |
| Number of pages | 5 |
| Journal | Journal of Physics B: Atomic and Molecular Physics |
| Volume | 13 |
| Issue number | 18 |
| DOIs | |
| State | Published - 1980 |
| Externally published | Yes |
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ASJC Scopus subject areas
- Atomic and Molecular Physics, and Optics
Cite this
Fe, Kr and Nb X-ray spectra produced in 8.5 MeV amu-1 ion-solid collisions. / Fortner, R. J.; Howell, R. H.; Matthews, Dennis L.
In: Journal of Physics B: Atomic and Molecular Physics, Vol. 13, No. 18, 008, 1980, p. 3545-3549.Research output: Contribution to journal › Article
}
TY - JOUR
T1 - Fe, Kr and Nb X-ray spectra produced in 8.5 MeV amu-1 ion-solid collisions
AU - Fortner, R. J.
AU - Howell, R. H.
AU - Matthews, Dennis L
PY - 1980
Y1 - 1980
N2 - X-ray spectra produced when 8.5 MeV amu-1 Fe, Kr and Nb ions are excited in collisions with a graphite target are reported. X-ray transitions originating in one-, two- and three-electron ions are observed and used to test the accuracy of the theoretical X-ray energy calculations. The production probabilities for Li-, He- and H-like ions were determined from the relative gamma -ray line strengths and centroid line energies.
AB - X-ray spectra produced when 8.5 MeV amu-1 Fe, Kr and Nb ions are excited in collisions with a graphite target are reported. X-ray transitions originating in one-, two- and three-electron ions are observed and used to test the accuracy of the theoretical X-ray energy calculations. The production probabilities for Li-, He- and H-like ions were determined from the relative gamma -ray line strengths and centroid line energies.
UR - http://www.scopus.com/inward/record.url?scp=36149048320&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=36149048320&partnerID=8YFLogxK
U2 - 10.1088/0022-3700/13/18/008
DO - 10.1088/0022-3700/13/18/008
M3 - Article
AN - SCOPUS:36149048320
VL - 13
SP - 3545
EP - 3549
JO - Journal of the Physics B: Atomic and Molecular Physics
JF - Journal of the Physics B: Atomic and Molecular Physics
SN - 0022-3700
IS - 18
M1 - 008
ER -