NIST Physics Laboratory National Institute of Standards and Technology NIST Physics Laboratory NIST Atomic Spectroscopic Database - Manganese Holdings

Choose a stage of ionization from the column on the left and a data type from the row on top. The numbers in the table indicate database holdings. Warning: Choosing a stage of ionization with many holdings (e.g., thousands) may cause your browser to time out.

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Spectrum          Energy    Wavelengths       Transition
                  Levels                   Probabilities
 All              2251           1310             1934
 Mn I              526              0              512
 Mn II             512              0               17
 Mn III            393              0                0
 Mn IV             104              0                0
 Mn V               85              0              112
 Mn VI             116              0               99
 Mn VII             43             57               35
 Mn VIII            32             49                3
 Mn IX              26             42               23
 Mn X               28             53               20
 Mn XI              44             74               58
 Mn XII             29             52               64
 Mn XIII            18             92               96
 Mn XIV             51            104               40
 Mn XV              43            171              229
 Mn XVI             16             74               21
 Mn XVII            24             32               25
 Mn XVIII           17             47               74
 Mn XIX             16             76               88
 Mn XX              21            102              113
 Mn XXI             16             49               57
 Mn XXII            28             79               96
 Mn XXIII           11             62               70
 Mn XXIV            26             74               82
 Mn XXV             26             21                0


Wavelength:  to  Ångströms (for wavelengths and transition probabilities data only)



 



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