2006
DOI: 10.1016/j.radphyschem.2006.09.002
|View full text |Cite
|
Sign up to set email alerts
|

Kα3,4 satellites in Mg–Cl elements

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
5
0

Year Published

2010
2010
2022
2022

Publication Types

Select...
5
1

Relationship

0
6

Authors

Journals

citations
Cited by 6 publications
(6 citation statements)
references
References 11 publications
1
5
0
Order By: Relevance
“…This fact explains the dependence of the intensity of KαL 1 satellite lines with the excitation source. Indeed, for the transition probability of the whole KαL 1 group relative to the Kα spectrum, values between 0.013 [63] and 0.044 [64] have been reported for photons, between 0.050 (present results) and 0.068 [62] for electrons, and the value 0.081 [44] for protons. Nevertheless, the behaviour of the Kα 3 /Kα 4 ratio with the oxidation state for the different excitation sources cannot be inferred from the double ionization probabilities.…”
Section: Kα Groupsupporting
confidence: 52%
“…This fact explains the dependence of the intensity of KαL 1 satellite lines with the excitation source. Indeed, for the transition probability of the whole KαL 1 group relative to the Kα spectrum, values between 0.013 [63] and 0.044 [64] have been reported for photons, between 0.050 (present results) and 0.068 [62] for electrons, and the value 0.081 [44] for protons. Nevertheless, the behaviour of the Kα 3 /Kα 4 ratio with the oxidation state for the different excitation sources cannot be inferred from the double ionization probabilities.…”
Section: Kα Groupsupporting
confidence: 52%
“…(b) Intensity relative to the Kα group. Filled circles: present results; open circles: [24]; crossed circles: [25]; half-filled circles: [54]; filled up triangles: [9]; half-filled up triangles: [4]; filled down triangles: [10]; crossed triangles: [1]; open up triangles: [14]; open down triangles: [2]; filled squares: [17]; open squares: [21]; half-filled squares: [18]. The solid line is a linear fit to the data obtained by electron and photon incidence; whereas the dashed line is a linear fit to the data obtained by proton incidence.…”
Section: K α 3 and K α 4 Linesmentioning
confidence: 88%
“…Regarding Kα transitions, several works were carried out to investigate satellite emissions induced by photon [1][2][3][4][5][6][7][8][9][10][11][12][13][14][15][16], proton [17][18][19][20], heavy-ion [17,21,22], and electron [13,[23][24][25][26][27][28][29] impact, although most of them were focused on a few particular elements or transitions. Some theoretical studies related to Kα satellite transitions were also performed [13,[30][31][32][33][34][35][36].…”
Section: Introductionmentioning
confidence: 99%
“…Several works were carried out to investigate the K satellite transitions induced by photon [1][2][3][4][5][6][7][8][9][10][11][12][13][14], proton [15][16][17][18], heavy-ion [15,[19][20][21][22], and electron [23][24][25][26][27][28][29][30][31][32][33] impact, although most of them are focused on a few particular elements or transitions. Theoretical calculations were performed by several authors [25,26,29,[34][35][36][37][38][39][40].…”
Section: Introductionmentioning
confidence: 99%