chan_1992_neon#

W. F. Chan, G. Cooper, X. Guo, and C. E. Brion, Phys. Rev. A 45, 1420 (1992)

Source record · Catalogue · Review register

Source kind: measurement

Recorded technique: Dipole (e,e) spectroscopy (part II of the series whose part III is chan_1992). Low resolution (about 1 eV FWHM, 8 keV impact energy, zero scattering angle): electron-energy-loss spectra 15.7-250 eV (steps 0.1, 0.5, 1 and 2 eV in 15.7-25, 25-50, 50-120, 120-250 eV) converted to relative optical oscillator strengths with the spectrometer’s Bethe-Born factor; the part above 250 eV from a fit A E^-B to 120-250 eV (B = 1.959; 17.6 % of the valence-shell total); the absolute scale by Thomas-Reiche-Kuhn normalisation of the whole area to 8.34 (eight valence electrons plus 0.34 for Pauli-excluded transitions), independent of any optical measurement (pp. 3, 6). High resolution (0.048 eV FWHM, 3 keV; also 0.072 and 0.098 eV): spectra 16-26 eV converted with the averaged Bethe-Born factor B_HR and normalised at 25 eV to the low-resolution data; peaks above 19 eV deconvoluted, nd[1/2] and nd[3/2] of the 2P_3/2 series fitted as one peak (p. 10). Energy scale: the 3s’ peak at 16.850 eV (Moore) at low resolution, the He 21.218 eV line admitted with the sample at high resolution (p. 6). Matheson neon, 99.99 %.

Materials in structured entries: Ne

Dataset quantities: differential_oscillator_strength, oscillator_strength

Contents: 44 datasets; 0 formulas.

Curation notes#

Part II of the series (neon); part III (argon, krypton, xenon) is chan_1992, part I (helium) chan_1991. Values per atom; no density or state involved. Page numbers are the library pdf pages (journal page = pdf page + 1419).

Continuum (Table I): df/dE in 10^-2 eV^-1 at photon energy E (eV), 21.6-250 eV, from the low-resolution spectrometer. The paper states no uncertainty for these values. The 45.0 eV point (7.45) sits on the 2s -> 3p autoionising resonance (maximum at 45.550 eV, p. 12). The high-resolution 40-55 eV autoionising spectrum (Fig. 3) and the 16-26 eV discrete spectrum (Fig. 2) are figures only and not extracted; the text gives the resonance energies 44.999 (2p^-2 3s3p), 45.550, 47.127, 47.677, 47.975 eV (2s -> np, n = 3-6) and a peak X at 43.735 eV (p. 12), not extracted.

Discrete lines (Tables II-IV): the present oscillator strengths with their estimated uncertainties in parentheses (‘~5% for the lower energy resolved transitions and <= 10% for those such as 6s, 6s’, 5d, and 5d’’, p. 10), and the literature values the tables compare, one dataset per source (and variant) as in chan_1992. The column headers name the transitions but, unlike part III, print no energies; the text gives only the resonance lines: ‘the 16.671 eV (f_1) and 16.848 eV (f_2) resonance lines’ (p. 2). The low-resolution calibration quotes the 3s’ state at 16.850 eV (Moore, p. 6): 2 meV from the 16.848 eV of p. 2; the p. 2 values are used. So each source has up to three datasets: ‘<source>_Ne’ (the resonance lines, eV), ‘<source>_higher_Ne’ (Tables III, IV, rows by transition label, index abscissa 1 = 4s, 2 = 4s’, 3 = 3d, 4 = 3d’, 5 = 5s, 6 = 5s’, 7 = 4d, 8 = 4d’, 9 = 6s, 10 = 6s’, 11 = 5d, 12 = 5d’) and ‘<source>_sum_Ne’ (the summed nl + nl’ values of note a, rows by pair, 1 = 3s+3s’, 2 = 4s+4s’, 3 = 3d+3d’, 4 = 5s+5s’, 5 = 4d+4d’, 6 = 6s+6s’, 7 = 5d+5d’). FORMAT NEED: the higher lines need their transition energies (Moore’s tables, Ref. [66], not in the library) before they can be used as lines; until then the index datasets hold the values and labels only.

Text values not extracted: the present summed f_1 + f_2 = 0.171 (p. 11; 0.0118 + 0.159); the dipole-forbidden 3p and 4p peaks at 18.96 and 20.38 eV, ‘all less than 0.3% of the f_2 peak’ (p. 10); West and Marr’s total discrete sum 0.4 (p. 12, ‘would seem to be too high’). Table labels printed differently from the reference list (the data are not affected): ‘Amusy’ya’ (Table III), ‘Bhaskar and Luiro’ (Ref. [37]: Lurio), ‘Lawrence and Liszt (1960)’ (Table III; Ref. [33] is 1969), ‘Klose (1970) [34]’ (Ref. [34] is Phys. Rev. 188, 45 (1969)), ‘Jongh and Eck’ (De Jongh and Van Eck). The uncertainty Lewis prints for f_2, (0.002) on 0.168 (1.2 %), is small beside his (0.002) on 0.012 for f_1; kept as printed (as for his argon value in chan_1992).

S(k): the paper prints no Cauchy moments or dipole sums (only the TRK normalisation to 8.34). Lesiuk et al. (2020, Table XI, lesiuk_2020/chan_1992_Ne) quote S(-4) = 2.938 and S(-6) = 5.137 as ‘Chan et al.’, citing this paper; those numbers are not in it, and Lesiuk et al. do not say how they were obtained.

Recorded bibliographic identity status: VALIDATED_WITH_WARNINGS. This concerns identification of the source; it does not establish the scientific correctness of its contents.

Datasets#

chan_1992_neon/continuum_Ne#

{
  "id": "continuum_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__continuum_Ne.csv",
  "table": "tbl_66ad40730b41, tbl_b252935d2cb5",
  "quantity": "differential_oscillator_strength",
  "unit": "1/eV",
  "scale": 0.01,
  "abscissa_unit": "eV",
  "use": "primary"
}

Table I and its continuation: df/dE (10^-2 eV^-1) at 21.6-250 eV, 220 points, rows by photon energy in reading order (column by column). Low-resolution dipole (e,e), TRK-normalised to 8.34. No uncertainty stated.

chan_1992_neon/albat_1974_Ne#

{
  "id": "albat_1974_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__albat_1974_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "R. Albat and N. Gruen, J. Phys. B 7, L9 (1974)"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, configuration interaction.

chan_1992_neon/aleksandrov_1983_Ne#

{
  "id": "aleksandrov_1983_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__aleksandrov_1983_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "Y. M. Aleksandrov, P. F. Gruzdev, M. G. Kozlov, A. V. Loginov, V. N. Makhov, R. V. Fedorchuk, and M. N. Yakimenko, Opt. Spektrosk. 54, 7 (1983) [Opt. Spectrosc. (USSR) 54, 4 (1983)]"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); total absorption.

chan_1992_neon/aleksandrov_1983_higher_Ne#

{
  "id": "aleksandrov_1983_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__aleksandrov_1983_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149, tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "Y. M. Aleksandrov, P. F. Gruzdev, M. G. Kozlov, A. V. Loginov, V. N. Makhov, R. V. Fedorchuk, and M. N. Yakimenko, Opt. Spektrosk. 54, 7 (1983) [Opt. Spectrosc. (USSR) 54, 4 (1983)]"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

chan_1992_neon/aleksandrov_1983_theory_Ne#

{
  "id": "aleksandrov_1983_theory_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__aleksandrov_1983_theory_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "Y. M. Aleksandrov, P. F. Gruzdev, M. G. Kozlov, A. V. Loginov, V. N. Makhov, R. V. Fedorchuk, and M. N. Yakimenko, Opt. Spektrosk. 54, 7 (1983) [Opt. Spectrosc. (USSR) 54, 4 (1983)]"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, intermediate coupling.

chan_1992_neon/aleksandrov_1983_theory_higher_Ne#

{
  "id": "aleksandrov_1983_theory_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__aleksandrov_1983_theory_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149, tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "Y. M. Aleksandrov, P. F. Gruzdev, M. G. Kozlov, A. V. Loginov, V. N. Makhov, R. V. Fedorchuk, and M. N. Yakimenko, Opt. Spektrosk. 54, 7 (1983) [Opt. Spectrosc. (USSR) 54, 4 (1983)]"
  ]
}

chan_1992_neon/amusya_1990_sum_Ne#

{
  "id": "amusya_1990_sum_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__amusya_1990_sum_Ne.csv",
  "table": "tbl_3545e6ef35ab, tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "M. Ya. Amus'ya, Atomic Photoeffect (Plenum, New York, 1990), p. 170"
  ]
}

Summed oscillator strengths of the pairs nl + nl’ (note a; printed centred between the two columns), rows by pair, index abscissa (1 = 3s+3s’ ... 7 = 5d+5d’); theory, RPAE.

chan_1992_neon/aymar_1970_length_Ne#

{
  "id": "aymar_1970_length_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__aymar_1970_length_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "M. Aymar, S. Feneuille, and M. Klapisch, Nucl. Instrum. Methods 90, 137 (1970)"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, dipole length.

chan_1992_neon/aymar_1970_velocity_Ne#

{
  "id": "aymar_1970_velocity_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__aymar_1970_velocity_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "M. Aymar, S. Feneuille, and M. Klapisch, Nucl. Instrum. Methods 90, 137 (1970)"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, dipole velocity.

chan_1992_neon/bhaskar_1976_Ne#

{
  "id": "bhaskar_1976_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__bhaskar_1976_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "N. D. Bhaskar and A. Lurio, Phys. Rev. A 13, 1484 (1976)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); lifetime, Hanle effect.

chan_1992_neon/cooper_1962_sum_Ne#

{
  "id": "cooper_1962_sum_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__cooper_1962_sum_Ne.csv",
  "table": "tbl_3545e6ef35ab, tbl_bbf7e53a7149, tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "J. W. Cooper, Phys. Rev. 128, 681 (1962)"
  ]
}

Summed oscillator strengths of the pairs nl + nl’ (note a; printed centred between the two columns), rows by pair, index abscissa (1 = 3s+3s’ ... 7 = 5d+5d’); theory, one-electron central potential.

chan_1992_neon/de_jongh_1971_Ne#

{
  "id": "de_jongh_1971_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__de_jongh_1971_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "J. P. De Jongh and J. Van Eck, Physica 51, 104 (1971)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); relative self-absorption.

chan_1992_neon/decomps_1968_higher_Ne#

{
  "id": "decomps_1968_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__decomps_1968_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "B. Decomps and M. Dumont, IEEE J. Quantum Electron. QE-4, 916 (1968)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

chan_1992_neon/ducloy_1973_higher_Ne#

{
  "id": "ducloy_1973_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__ducloy_1973_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "M. Ducloy, Ann. Phys. (Paris) 8, 403 (1973)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

chan_1992_neon/geiger_1970_Ne#

{
  "id": "geiger_1970_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__geiger_1970_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "J. Geiger, Z. Phys. 177, 138 (1964); J. Geiger, Phys. Lett. 33A, 351 (1970)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); electron impact.

chan_1992_neon/gold_1959_semiempirical_Ne#

{
  "id": "gold_1959_semiempirical_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__gold_1959_semiempirical_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "A. Gold and R. S. Knox, Phys. Rev. 113, 834 (1959)"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, semiempirical.

chan_1992_neon/gold_1959_wave_function_Ne#

{
  "id": "gold_1959_wave_function_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__gold_1959_wave_function_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "A. Gold and R. S. Knox, Phys. Rev. 113, 834 (1959)"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, wave function.

chan_1992_neon/gruzdev_1967_Ne#

{
  "id": "gruzdev_1967_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__gruzdev_1967_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "P. F. Gruzdev, Opt. Spektrosk. 22, 313 (1967) [Opt. Spectrosc. (USSR) 22, 170 (1967)]"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, intermediate coupling, Coulomb approximation.

chan_1992_neon/gruzdev_loginov_1973_Ne#

{
  "id": "gruzdev_loginov_1973_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__gruzdev_loginov_1973_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "P. F. Gruzdev and A. V. Loginov, Opt. Spektrosk. 35, 3 (1973) [Opt. Spectrosc. (USSR) 35, 1 (1973)]"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, intermediate coupling with Hartree-Fock wave functions.

chan_1992_neon/gruzdev_loginov_1973_higher_Ne#

{
  "id": "gruzdev_loginov_1973_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__gruzdev_loginov_1973_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "P. F. Gruzdev and A. V. Loginov, Opt. Spektrosk. 35, 3 (1973) [Opt. Spectrosc. (USSR) 35, 1 (1973)]"
  ]
}

Table III: oscillator strengths of the lines above the resonance lines, rows by transition label, index abscissa (1 = 4s ... 12 = 5d’, the tables’ column order): the paper does not print their energies; theory, intermediate coupling with Hartree-Fock wave functions. Note b: ‘Lifetime data converted by Westerveld, Mulder, and Van Eck [43] to oscillator strengths using transition probabilities reported in Refs. [73] and [74]’.

chan_1992_neon/irwin_1973_Ne#

{
  "id": "irwin_1973_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__irwin_1973_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "D. J. G. Irwin, A. E. Livingston, and J. A. Kernahan, Can. J. Phys. 51, 1948 (1973)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); lifetime, beam foil.

chan_1992_neon/kazantsev_1971_Ne#

{
  "id": "kazantsev_1971_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__kazantsev_1971_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "S. Kazantsev and M. Chaika, Opt. Spektrosk. 3, 510 (1971) [Opt. Spectrosc. (USSR) 3, 273 (1971)]"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); lifetime, hidden alignment.

chan_1992_neon/kelly_1964_sum_Ne#

{
  "id": "kelly_1964_sum_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__kelly_1964_sum_Ne.csv",
  "table": "tbl_3545e6ef35ab, tbl_bbf7e53a7149, tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "P. S. Kelly, J. Quant. Spectrosc. Radiat. Transfer 4, 117 (1964)"
  ]
}

Summed oscillator strengths of the pairs nl + nl’ (note a; printed centred between the two columns), rows by pair, index abscissa (1 = 3s+3s’ ... 7 = 5d+5d’); theory, Slater approximation to Hartree-Fock.

chan_1992_neon/klose_1969_ic_cf_higher_Ne#

{
  "id": "klose_1969_ic_cf_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__klose_1969_ic_cf_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "J. Z. Klose, Phys. Rev. 188, 45 (1969)"
  ]
}

chan_1992_neon/klose_1969_ic_hfs_higher_Ne#

{
  "id": "klose_1969_ic_hfs_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__klose_1969_ic_hfs_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "J. Z. Klose, Phys. Rev. 188, 45 (1969)"
  ]
}

chan_1992_neon/klose_1969_lifetime_higher_Ne#

{
  "id": "klose_1969_lifetime_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__klose_1969_lifetime_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "J. Z. Klose, Phys. Rev. 188, 45 (1969)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table III: oscillator strengths of the lines above the resonance lines, rows by transition label, index abscissa (1 = 4s ... 12 = 5d’, the tables’ column order): the paper does not print their energies; lifetime, delayed coincidence (the table labels it ‘Klose (1970) [34]’; Ref. [34] is the 1969 paper).

chan_1992_neon/klose_1969b_ic_hfs_higher_Ne#

{
  "id": "klose_1969b_ic_hfs_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__klose_1969b_ic_hfs_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "J. Z. Klose, J. Quant. Spectrosc. Radiat. Transfer 9, 881 (1969)"
  ]
}

chan_1992_neon/knystautas_1974_Ne#

{
  "id": "knystautas_1974_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__knystautas_1974_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "E. J. Knystautas and R. Drouin, Astron. Astrophys. 37, 145 (1974)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); lifetime, beam foil.

chan_1992_neon/korolev_1964_Ne#

{
  "id": "korolev_1964_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__korolev_1964_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "F. A. Korolev, V. I. Odintsov, and E. V. Fursova, Opt. Spektrosk. 16, 555 (1964) [Opt. Spectrosc. (USSR) 16, 304 (1964)]"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); natural-broadening profile.

chan_1992_neon/lawrence_1969_Ne#

{
  "id": "lawrence_1969_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__lawrence_1969_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "G. M. Lawrence and H. S. Liszt, Phys. Rev. 178, 178 (1969)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); lifetime, delayed coincidence.

chan_1992_neon/lawrence_1969_higher_Ne#

{
  "id": "lawrence_1969_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__lawrence_1969_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "G. M. Lawrence and H. S. Liszt, Phys. Rev. 178, 178 (1969)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

chan_1992_neon/lawrence_1969_westerveld_higher_Ne#

{
  "id": "lawrence_1969_westerveld_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__lawrence_1969_westerveld_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "G. M. Lawrence and H. S. Liszt, Phys. Rev. 178, 178 (1969), recalculated in W. B. Westerveld, Th. F. A. Mulder, and J. Van Eck, J. Quant. Spectrosc. Radiat. Transfer 21, 533 (1979)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table III: oscillator strengths of the lines above the resonance lines, rows by transition label, index abscissa (1 = 4s ... 12 = 5d’, the tables’ column order): the paper does not print their energies; lifetime, delayed coincidence, recalculated by Westerveld et al. with the branching ratios of Refs. [53], [73], [74] (note c).

chan_1992_neon/lewis_1967_Ne#

{
  "id": "lewis_1967_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__lewis_1967_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "E. L. Lewis, Proc. Phys. Soc. 92, 817 (1967)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); pressure-broadening profile.

chan_1992_neon/natali_unpublished_Ne#

{
  "id": "natali_unpublished_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__natali_unpublished_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "S. Natali, C. E. Kuyatt, and S. R. Mielczarek, unpublished observations as quoted in W. B. Westerveld et al. (1979) and J. Berkowitz, Photoabsorption, Photoionization and Photoelectron Spectroscopy (Academic, New York, 1979), p. 80"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); electron impact.

chan_1992_neon/natali_unpublished_higher_Ne#

{
  "id": "natali_unpublished_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__natali_unpublished_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "S. Natali, C. E. Kuyatt, and S. R. Mielczarek, unpublished observations as quoted in W. B. Westerveld et al. (1979) and J. Berkowitz, Photoabsorption, Photoionization and Photoelectron Spectroscopy (Academic, New York, 1979), p. 80"
  ]
}

chan_1992_neon/natali_unpublished_total_Ne#

{
  "id": "natali_unpublished_total_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__natali_unpublished_total_Ne.csv",
  "table": "tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "S. Natali, C. E. Kuyatt, and S. R. Mielczarek, unpublished observations as quoted in W. B. Westerveld et al. (1979) and J. Berkowitz, Photoabsorption, Photoionization and Photoelectron Spectroscopy (Academic, New York, 1979), p. 80"
  ]
}

Table IV ‘Total to ionization’: the discrete oscillator-strength sum up to 21.616 eV (the midpoint of the 2P_3/2 and 2P_1/2 thresholds, p. 11), index abscissa; electron impact.

chan_1992_neon/present_Ne#

{
  "id": "present_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__present_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "primary",
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); the present high-resolution dipole (e,e) measurement (0.048 eV FWHM), normalised at 25 eV to Table I. Estimated uncertainty ~5 % (p. 10).

chan_1992_neon/present_higher_Ne#

{
  "id": "present_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__present_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149, tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "primary",
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table III and Table IV: oscillator strengths of the lines above the resonance lines, rows by transition label, index abscissa (1 = 4s ... 12 = 5d’, the tables’ column order): the paper does not print their energies; the present high-resolution dipole (e,e) measurement (0.048 eV FWHM), deconvoluted peak areas, normalised at 25 eV to Table I. Estimated uncertainty ~5 %, <= 10 % for 6s, 6s’, 5d, 5d’ (p. 10). nd[1/2] and nd[3/2] of the 2P_3/2 series are one peak in the deconvolution (p. 10): ‘3d’, ‘4d’, ‘5d’ are their sums.

chan_1992_neon/present_total_Ne#

{
  "id": "present_total_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__present_total_Ne.csv",
  "table": "tbl_f0fb0b7927fd",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "check",
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table IV ‘Total to ionization’: the discrete oscillator-strength sum up to 21.616 eV (the midpoint of the 2P_3/2 and 2P_1/2 thresholds, p. 11), index abscissa. A sum over the present-work lines and the unlisted higher members: a check, not fitted beside them. The text compares 0.277 (Natali et al.) and West and Marr’s 0.4, ‘too high’ (p. 12).

chan_1992_neon/stewart_1975_Ne#

{
  "id": "stewart_1975_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__stewart_1975_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "R. F. Stewart, Mol. Phys. 29, 1577 (1975)"
  ]
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); theory, time-dependent Hartree-Fock.

chan_1992_neon/stewart_1975_higher_Ne#

{
  "id": "stewart_1975_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__stewart_1975_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "R. F. Stewart, Mol. Phys. 29, 1577 (1975)"
  ]
}

chan_1992_neon/tsurubuchi_1990_Ne#

{
  "id": "tsurubuchi_1990_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__tsurubuchi_1990_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "S. Tsurubuchi, K. Watanabe, and T. Arikawa, J. Phys. Soc. Jpn. 59, 497 (1990)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); absolute self-absorption.

chan_1992_neon/westerveld_1979_Ne#

{
  "id": "westerveld_1979_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__westerveld_1979_Ne.csv",
  "table": "tbl_3545e6ef35ab",
  "quantity": "oscillator_strength",
  "abscissa_unit": "eV",
  "use": "reproduced",
  "reproduced_from": [
    "W. B. Westerveld, Th. F. A. Mulder, and J. Van Eck, J. Quant. Spectrosc. Radiat. Transfer 21, 533 (1979)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Table II: oscillator strengths of the resonance lines 3s (f_1, 16.671 eV) and 3s’ (f_2, 16.848 eV), energies from the text (p. 2); absolute self-absorption.

chan_1992_neon/westerveld_1979_higher_Ne#

{
  "id": "westerveld_1979_higher_Ne",
  "material": "Ne",
  "file": "Ne/chan_1992_neon__westerveld_1979_higher_Ne.csv",
  "table": "tbl_bbf7e53a7149",
  "quantity": "oscillator_strength",
  "abscissa": "label",
  "use": "reproduced",
  "reproduced_from": [
    "W. B. Westerveld, Th. F. A. Mulder, and J. Van Eck, J. Quant. Spectrosc. Radiat. Transfer 21, 533 (1979)"
  ],
  "uncertainty": {
    "column": true,
    "level": "not stated"
  }
}

Formulas#

No formulas are recorded.

Corrections#

No dataset errata are recorded in this source record.

Formula corrections, where recorded, appear with their formulas above. Curation notes may also discuss corrections or unresolved interpretation. Consult the review register for the checks and decisions.