cop98#10_ls#ne0.dat

Resolved Specific Ion Data Collections

Ion
Ne0+
Temperature Range
0.043 eV → 43.08 eV

ADF04

Filename
cop98#10_ls#ne0.dat
Full Path
adf04/adas#10/cop98#10_ls#ne0.dat
Download data
  • Spontaneous Emission: Ne+0(i) → Ne+0(j) + hv
  • Electron Impact Excitation: Ne+0(i) + e → Ne+0(j) + e
  • Free Electron Recombination: Ne+1(i) + e → Ne+0(j)
2s2 2p6 1S0.0 0.0 cm-1
2s2 2p5 3s1 3P4.0 134269.0 cm-1
2s2 2p5 3s1 1P1.0 135891.0 cm-1
2s2 2p5 3p1 3S1.0 148260.0 cm-1
2s2 2p5 3p1 3D7.0 149808.0 cm-1
2s2 2p5 3p1 1P1.0 150774.0 cm-1
2s2 2p5 3p1 3P4.0 150854.0 cm-1
2s2 2p5 3p1 1D2.0 150860.0 cm-1
2s2 2p5 3p1 1S0.0 150919.0 cm-1
2s2 2p5 3d1 3P4.0 161571.0 cm-1
2s2 2p5 3d1 1F3.0 161594.0 cm-1
2s2 2p5 3d1 1P1.0 161639.0 cm-1
2s2 2p5 3d1 1D2.0 161702.0 cm-1
2s2 2p5 3d1 3F10.0 162060.0 cm-1
2s2 2p5 3d1 3D7.0 162090.0 cm-1
-------------------------------------------------------------------------------

  File generated by compression of a J-resolved file

  Program: ADAS209

  Source file: /home/adas/adas/adf04/adas#10/cop98#10_ic#ne0.dat

  Original level indexing:
     1    2    3    4    5    6    7    8    9   10
    11   12   13   14   15   16   17   18   19   20
    21   22   23   24   25   26   27
  Selection Vector:
     1    2    2    2    3    4    5    5    5    6
     7    8    9    6    6   10   10   14   11   10
    12   13   15   14   14   15   15

  Original parent metastables:
    (1S)
  Parent bundling vector:
     0


  Date     :  11-Dec-2000
  Producer :  Martin O'Mullane

-------------------------------------------------------------------------------

 Comments from unbundled file:
--------------------------------------------------------------------------------

             Configuration
       Eissner            == Standard             Parentage

   1   22563              == 2S2 2P6              1 1S  1S/
   2   22553514           == 2S2 2P5 3S1          1 2P  2P/ 1 2S  3P/
   3   22553514           == 2S2 2P5 3S1          1 2P  2P/ 1 2S  3P/
   4   22553514           == 2S2 2P5 3S1          1 2P  2P/ 1 2S  3P/
   5   22553514           == 2S2 2P5 3S1          1 2P  2P/ 1 2S  1P/
   6   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3S/
   7   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3D/
   8   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3D/
   9   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3D/
  10   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3P/
  11   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  1P/
  12   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  1D/
  13   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3P/
  14   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  3P/
  15   22553515           == 2S2 2P5 3P1          1 2P  2P/ 1 2P  1S/
  16   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3P/
  17   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3P/
  18   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3F/
  19   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  1F/
  20   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3P/
  21   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  1P/
  22   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  1D/
  23   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3D/
  24   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3F/
  25   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3F/
  26   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3D/
  27   22553516           == 2S2 2P5 3D1          1 2P  2P/ 1 2D  3D/

--------------------------------------------------------------------------------

   Generated from Cowan Atomic Structure Program

   From IFG file : /work/work_remote/mog/cowan_work/ifg#ne0.dat

   Options in effect

   Coupling    Avalue   numtemps   Lweight   Isonuclear   Comment Level
   IC          YES      14         NO        NO           2


   Cowan code options
   ------------------

         SCF method used                      :  HR

         Scale factors for Slater Parameters  :  75 99 75 75 70

         Optically allowed transitions        :  Yes

         Optically forbidden transitions (M1) :  None

         Optically forbidden transitions (E2) :  Both Parities

         Born Collision-Strength  - forbidden :  0 ->  2

         Born Collision-Strength  - allowed   :  1 ->  1


   Parity 1    Parity 2    Allowed
         39          83        111     initially
         39          83        111     reduced

   Note: The Born method does NOT calculate spin changing transitions
   correctly. Supplement for important transitions of this type.


   Producer : Martin O'Mullane
   Date     : 06/03/00

--------------------------------------------------------------------------------

  The level list has been changed to reflect the jl nature of coupling
  in NeI. The transformation is from the LS to LSJLSJ in the RCG
  output of the Cowan code. In the proper notation we have


     1  2S2 2P6                 (1)0( 0.0)
     2  2p5(2P<1.5>) 3s <1.5>   (3)1( 2.0)
     3  2p5(2P<1.5>) 3s <1.5>   (3)1( 1.0)
     4  2p5(2P<0.5>) 3s <0.5>   (3)1( 0.0)
     5  2p5(2P<0.5>) 3s <0.5>   (1)1( 1.0)
     6  2p5(2P<1.5>) 3p <0.5>   (3)0( 1.0)
     7  2p5(2P<1.5>) 3p <2.5>   (3)2( 3.0)
     8  2p5(2P<1.5>) 3p <2.5>   (3)2( 2.0)
     9  2p5(2P<1.5>) 3p <1.5>   (3)2( 1.0)
    10  2p5(2P<1.5>) 3p <1.5>   (3)1( 2.0)
    11  2p5(2P<0.5>) 3p <1.5>   (1)1( 1.0)
    12  2p5(2P<0.5>) 3p <1.5>   (1)2( 2.0)
    13  2p5(2P<0.5>) 3p <0.5>   (3)1( 0.0)
    14  2p5(2P<0.5>) 3p <0.5>   (3)1( 1.0)
    15  2p5(2P<1.5>) 3p <0.5>   (1)0( 0.0)
    16  2p5(2P<1.5>) 3d <0.5>   (3)1( 0.0)
    17  2p5(2P<1.5>) 3d <0.5>   (3)1( 1.0)
    18  2p5(2P<1.5>) 3d <3.5>   (3)3( 4.0)
    19  2p5(2P<1.5>) 3d <3.5>   (1)3( 3.0)
    20  2p5(2P<1.5>) 3d <1.5>   (3)1( 2.0)
    21  2p5(2P<1.5>) 3d <1.5>   (1)1( 1.0)
    22  2p5(2P<1.5>) 3d <2.5>   (1)2( 2.0)
    23  2p5(2P<1.5>) 3d <2.5>   (3)2( 3.0)
    24  2p5(2P<0.5>) 3d <2.5>   (3)3( 2.0)
    25  2p5(2P<0.5>) 3d <2.5>   (3)3( 3.0)
    26  2p5(2P<0.5>) 3d <1.5>   (3)2( 2.0)
    27  2p5(2P<0.5>) 3d <1.5>   (3)2( 1.0)


  The energy levels have been replaced by those of C E Moore (Atomic
  Energy Levels, National Bureau of Standards Circular 467, 1949)

   Producer : Martin O'Mullane
   Date     : 06/03/00

--------------------------------------------------------------------------------

 Filtered adf04 file to
  - sort energy levels
  - remove non physical A values from
    energy level reversals
  - remove energies above ionisation potential
  - remove duplicate transitions

 Code : /home/omullane/adf04_utils/filter_adf04.x


 Level list :

      1   2   3   4   5   6   7   8   9  10
     11  12  13  14  15  16  17  18  19  20
     21  22  23  24  25  26  27

 Original level order :

      1   2   3   4   5   6   7   8   9  10
     11  12  15  14  13  16  17  18  19  20
     21  22  23  24  25  26  27

 Date     :  06/03/00
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

 Effective collision strengths from the ground 2p6 1S state to the 2p5 3s
 and 2p53p levels have been taken variously from:
    Zeman & Bartschat, J. Phys. B 30, p4609, (1997)
    Tsurubuchi et al., J. Phys. B, 33, p3713, (2000)
    Machado et al, Phys. Rev. A, 29, p1811, (1984)
    Chilton et al, Phys. Rev. A, 61, 052708, (2000)

 Preferred curves have been prepared on a spreadsheet and converted to
 effective collison strengths by the neutqd2.f program. Full details
 are available in ADAS Technical Note ATN(2000)01.

 A-values from NIST tables for these transitions.

 Date     :  27/11/2000
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

 A-values from J A del Val et al,, Astron. Astrophys., 357, p1137-1142, (2000)
 for transitions 12-2, 14-3, 13-3, 12-3, 10-2, 14-4, 9-2, 11-4, 10-3, 9-3,
 8-3, 14-5, 11-5, 9-5, 6-2, 27-6, 8-5, 6-3, 6-4, 21-6, 20-6, 17-6, 16-6.
 These lie between 593 and 814A.

 Date     :  11/12/2000
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

 Filtered adf04 file to
  - sort energy levels
  - remove non physical A values from
    energy level reversals
  - remove energies above ionisation potential
  - remove duplicate transitions

 Code : /home/omullane/adf04_utils/filter_adf04.x


 Level list :

      1   2   3   4   5   6   7   8   9  10
     11  12  13  14  15

 Original level order :

      1   2   3   4   5   7   6   8   9  10
     12  13  14  11  15

  Unphysical A values. Set A=1.0E-30 for following transitions :

      7     6    A =   2.93D-05


 The following duplicate transitions were found

       6    7
       8    7
       9    7
      15   14
      14   13


 Date     :  11-Dec-2000
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

   RADIATIVE RECOMBINATION DATA ADDED

   PROCESSED BY ADAS211 ON :
   /home/adas/adas/adf08/rrc98#f/rrc98#f_ne1ls.dat

 Date     :  20-Dec-2000
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

     Dielectronic data is post-processed from Badnell files as follows:

      /home/adas/adas/adf09/mom93#f/mom93#f_ne1ls22.dat

     The cross-referencing file is as follows:

      /home/adas/adas/adf18/a09_a04/drm96#ne/drm96#ne_ls#ne0.dat

     The parent metastable indices are as follows:

     1.    2S2 2P5             (2)1( 2.5)

     Dielectronic data added to  15 existing rad. recom. level sets


 Date     :  20-Dec-2000
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

  Added ionisation rates (S-lines) from :
      /home/adas/adas/adf07/szd96#ne/szd96#ne_ne.dat

    S  1  +1   ISEL =    2   Energy =    173929.00
    S  2  +1   ISEL =    4   Energy =     39659.80
    S  2  +2   ISEL =    5   Energy =    258839.10

  Set first point to 9.99+9 to exclude it from interpolation.

  Code     : ADAS807
  Producer : Martin O'Mullane
  Date     : 20/12/00

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 Ionisation pathways of level 2 should be split into parent 1 and 2, not
 parent 1 and 3.

 Date     :  20-Dec-2000
 Producer :  Martin O'Mullane

--------------------------------------------------------------------------------

   Add the orbital energies.

   Martin O'Mullane
   12-12-2019

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  • Processes
  • States
  • Comments
  • Origins

Data Classes

Fundamental

ADF01ADF04ADF07ADF08ADF09ADF38ADF39ADF48

Derived

ADF11ADF12ADF13ADF15ADF21ADF22