ls#kr8.dat

Resolved Specific Ion Data Collections

Ion
Kr8+
Temperature Range
6.980 eV → 1396 eV

ADF04

Filename
ls#kr8.dat
Full Path
adf04/copmm#36/ls#kr8.dat
Download data
  • Spontaneous Emission: Kr+8(i) → Kr+8(j) + hv
  • Electron Impact Excitation: Kr+8(i) + e → Kr+8(j) + e
606 1S0.0 0.0 cm-1
65596517 3D7.0 689271.0 cm-1
65596517 1D2.0 699801.0 cm-1
65596518 3P4.0 840861.0 cm-1
65596518 3F10.0 845041.0 cm-1
65596518 1D2.0 854721.0 cm-1
65596518 1P1.0 858541.0 cm-1
65596518 1F3.0 860781.0 cm-1
65596518 3D7.0 860801.0 cm-1
65596519 3S1.0 1078130.0 cm-1
65596519 1P1.0 1087430.0 cm-1
65596519 3G13.0 1089430.0 cm-1
65596519 3P4.0 1090430.0 cm-1
65596519 1F3.0 1091630.0 cm-1
65596519 3D7.0 1092630.0 cm-1
65596519 3F10.0 1099230.0 cm-1
65596519 1G4.0 1099530.0 cm-1
65596519 1D2.0 1101930.0 cm-1
65596519 1S0.0 1186630.0 cm-1
6559651a 3P4.0 1296630.0 cm-1
6559651a 1D2.0 1300630.0 cm-1
6559651a 3H16.0 1301530.0 cm-1
6559651a 1G4.0 1302130.0 cm-1
6559651a 1F3.0 1302830.0 cm-1
6559651a 3D7.0 1303830.0 cm-1
6559651a 3F10.0 1307430.0 cm-1
6559651a 3G13.0 1308830.0 cm-1
6559651a 1H5.0 1309930.0 cm-1
6559651a 1P1.0 1320830.0 cm-1
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     Generated from Cowan Atomic Structure Program

     M O'Mullane        16:40  19/10/1994



     SCF method used                      : HR

     Scale factors for Slater Parameters  : 95 99 85 85 60

     Optically allowed transitions        : yes

     Optically forbidden transitions M1   : both

     Optically forbidden transitions E2   : both

     Born Collision-Strength  - print     :  9

                              - forbidden :  0 -> 2

                              - allowed   :  1 -> 1

                              - included  :  3,all

     Parity 1    Parity 2    Allowed
            0           0        378     initially
            0           0        154     reduced

---------------------------------------------------------------------------------
    Level 1 had incorrect Eissner notation.
    Martin O'Mullane
    30-11-2011 
---------------------------------------------------------------------------------

Contributors

  • Martin O'Mullane
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