Spectral Lines

This section starts with the description of the input parameters of the Lines Search Form. For the description of the output, either in tabular or graphical form, see the Lines Output section.

 Lines Search Form

When loaded in the browser, the Lines Search Form displays only the Main search parameters block. At the bottom of this block, there are buttons "Reset Input," "Retrieve Data," "Show Graphical Options," and "Show Advanced Settings." When the "Show ..." buttons are clicked, the corresponding blocks of input options appear on the screen, and the buttons change their names to "Hide ..."

• Main search parameters
  • Spectra of interest (e.g., Na I, Na II, Mg I-III, Mn-Co Ar-like).
  • Primary quantity of interest: wavelength (default), wavenumber, photon energy, or frequency; selected from a pulldown menu in the Lines Form.
  • Lower and upper limits of the range of the primary quantity
  • Units for the quantity of interest: angstroms (Å), nanometers (nm; default for wavelengths), micrometers (μm); cm⁻¹ (the only choice for wavenumbers); eV (default for photon energies), Ry, Hartree; GHz (the only choice for frequencies). The units are selected from a pulldown menu in the Lines Form. The same units apply both to the output quantity and to the lower/upper limits of the quantity range.
• Graphical Output Options
  • Dynamic Plot options
    • No plots (used to reset the plotting options)
    • Line Identification Plot
    • Spectrum Image Plot
    • Saha-LTE Spectrum Plot
  • Grotrian Diagram options
• Advanced Settings
  • Output options
  • Optional search criteria
  • Additional search criteria

 Main Search Parameters

  Selecting Spectra for Line Searches

If the user has not provided enough information to specify spectra, an error message will be displayed.

Examples of Spectral Notation (Case Insensitive)

  Lower and upper limits of the wavelength/wavenumber/photon energy/frequency range

Note that the units set in the drop-down menu in the Main Parameters section apply not only to the limits of the promary quantity search range, but also to the output. By default, the wavelengths are included in the output. The user can change the choice of the columns displayed in the output and set a number of other options (e.g., whether the wavelengths are in standard air or in vacuum) in the Advanced Settings section of the Search Form. These settings will be displayed if the user clicks on the "Show Advanced Settings" button.

  Graphical Output Options

• Dynamic Plots: Line Identification, Spectrum Image, and Saha/LTE spectrum plots;
• Grotrian Diagrams

 Dynamic Plot Options

• Line Identification Plot
  
  Selecting this option would produce a PDF file showing positions of all spectral lines of the chosen Spectra within the chosen wavelength/wavenumber/photon energy/frequency range.
  
  The contents and use of the Line Identification Plots are explained in the corresponding Output section.
  
  
• Spectrum Image Plot
  
  This is an experimental feature introduced in ASD v.5.11 in 2023, and its operation has a limited flexibility. For example, it presently works only if the search is restricted to a single atom or ion, and only if the search is made for wavelengths in the units of nm, within the range between 380 nm and 780 nm. The purpose of the plot is to simulate an appearance of the spectrum produced by a slit spectrograph in a visible range, so that the color of each spectral line roughly corresponds to human percention of light at the line's wavelength, and its intensity roughly corresponds to intensities listed in the tabular output of ASD. The lines listed in ASD without numerical intensity values are assigned small non-zero intensities to make them visible in the image. The plot is displayed as an image at the bottom of the lines tabular output.
  
  
• Saha-LTE Spectrum
  
  Selecting this option would produce a PDF file with a plot showing line emission from an optically thin plasma having the chosen values of electron temperature and electron density. For this plot, both the lower and upper limits of the wavelength/wavenumber/photon energy/frequency range are mandatory parameters.
  
  The plasma emission intensities are calculated in arbitrary units. These units can be chosen from one of the two options: 1) energy flux units (the default choice) or 2) photon count units. If only one ion/atom is chosen for plot generation, then the populations of the energy levels are calculated according to the Boltzmann formula N_k = N₀/g₀·g_k·exp(−E_k/T_e) where N_k is the level population, N₀ is the population of the ground state level, g_k and g₀ are the statistical weights of the levels, E_k is the energy of the level with respect to the ground state in eV, and T_e is the electron temperature in eV to be entered in the text field. In this case the electron density N_e is not required to be entered.
  
  If several ions/atoms are chosen for plot generation (e.g., "C I-V" is entered in the Spectra input box), then first the ionization distribution between different ions is calculated according to the Saha formula (see, e.g., H.R. Griem, Principles of Plasma Spectroscopy, 1997), and then within each ion, the populations are calculated using the Boltzmann distribution formula. In this case both the electron temperature and electron density are mandatory parameters.
  
  The total number of photons emitted per second per unit volume of plasma in each radiative transition is calculated by multiplying the population density of the upper level, N_k, by the rate of spontaneous radiative decay, A_ki (a.k.a. transition probability or Einstein A-coefficient), from the upper level k to the lower level i of the transition. If the user requested the intensity scale to be in terms of energy flux, the photon emission rate is multiplied by the photon energy, E_k − E_i (in units of cm⁻¹ to calculate the emitted energy flux per unit plasma volume.
  
  The spectrum may be convoluted with the Doppler (Gaussian) line profile for each of the spectral lines. To do that, the user must check the Doppler-broadened spectrum box in the Lines Search Form and (optionally) specify the Ion Temperature (in eV) corresponding to the desired broadening. In practice, experimental spectra are broadened by many different mechanisms, e.g., instrumental broadening. To produce a synthetic spectrum resembling experimental ones, the user may need to specify an unphysically large Ion Temperature. The only meaning of this parameter is the broadening it produces.
  
  By default (if no Ion Temperature was specified), the entered electron temperature T_e is used for calculation of the line width parameter. An ion temperature T_i may be entered if T_i ≠ T_e.
  
  If a Doppler-broadened spectrum is requested by the user, the spectrum will be calculated on a grid with the step size defined by the total number of spectral lines of the selected spectra in the requested range and by the broadening of each spectral line (i.e., Ion Temperature). The greater the number of lines, the greater is the number of grid points required. The greater is the Ion Temperature, the lesser grid points are required. To reduce the load on our database servers, we are limiting the total number of data points in the spectrum grid. If the user's selection requires too many grid points, the ASD codes will choose a greater Ion Temperature corresponding to the maximum allowed grid points, and a warning about it will be displayed in the output.
  
  If several chemical elements are involved in the string entered in the Spectra input box, an additional form will appear, requesting the user to enter the percentage abundances of each element in the mixture.
  
  Such an additional form will also appear if the requested Spectra contain hydrogen or deuterium. For these spectra, the user must specify whether the resolved fine structure or configuration-average wavelengths should be used for their lines. This is due to the special character of hydrogen and deuterium spectra. In these spectra, the widths of the fine structure of energy levels are exceptionally small and thus, the fine structure is usually unresolved in experimental spectra recorded with low or moderate resolution. However, due to the fundamental importance of these spectra in physics, many studies of them are made with exceptionaly high resolution. To accommodate the needs of both low- and high-resolution spectroscopy, ASD contains two overlapping subsets of energy level and spectral line data for both H and D in the same data sets. For calculation of simulated spectra of H and D, only one subset of these data, either low- or high-resolution, must be selected (otherwise, the partition functions would be doubled, and the calculated intensities would be too large). For other elements, ASD does not have both these types of energy levels and wavelengths mixed in the tables, so a prompt for this choice will not appear.
  
  The contents of the output Saha-LTE plots and tables accompanying them are explained in the corresponding Output section.

 Java Grotrian Diagrams

  Advanced Settings

• Output Options controlling the general layout of the output,
• Optional Search Criteria controlling the range of selected data, and
• Additional Search Criteria controlling the scope and type of the selected and displayed data.

Output Options

The following options apply to all lines and levels searches and are collectively referred to as output options.

• Choice of display using an HTML table, an ASCII fixed-column-width table, a CSV or tab-delimted data file.
• Choice of removing Javascript tags in the output (convenient for an ASCII table when saving the output into a file)
• Energy level units. The user may choose between cm⁻¹ (default), eV, Rydberg, Hartree (=2×Rydberg), or GHz.
• Choice of viewing the (scrollable) data all at once, or one page at a time.
• Choice of page size. The number of lines displayed on each page of the output may be modified so that they would fit the user's screen size.
• Output ordering. The output can be sorted according to either wavelength or multiplet order. The multiplet order is available if only one ion or atom is specified in the Spectra box.
  

  Wavelength ordering

  All spectra are intermingled according to wavelength ordering. A spectrum must be provided if no wavelength range is indicated.
  

  Multiplet ordering

  Multiplets are transitions that share the same term and configuration. Multiplets have been ordered in the transition probability compilations according to energies and g values of the lower and upper levels, and have been assigned arbitrary multiplet numbers that reflect this order.

  To view multiplet-ordered data, the user must select the "Multiplet ordering" radio box.

  In some cases, a multiplet is missing from the numbered list. In general, this is because some property of a compiled wavelength or level involved is consistent with other more recent compilations, such as the NIST energy level data.

  Only the lines with energy level classification are displayed in the multiplet-ordered output, and therefore the total number of lines shown at the top of the page may be different for wavelength and multiplet orderings.

The default is to display output in its entirety as an HTML formatted table. By default, the levels are displayed in cm⁻¹.

For instructions on how to modify options associated with viewing data, refer to the section options for viewing data.

  Optional Search Criteria

The following search criteria may be specified:

• Maximum lower level energy.
• Maximum upper level energy.
• Preference of whether the transition strength bounds will apply to A_ki (default), f_ik, S, or log(gf) values.
• Minimum and/or maximum transition strength.
• Accuracy minimum for A_ki, f_ik, S, or log(gf).
• Relative intensity minimum.

  Additional Search Criteria

The following options apply to all line searches and are collectively referred to as additional search criteria options.

• Line selection options:
  • All lines of data meeting the search criteria,
  • Only lines with transition probability data,
  • Only lines with energy level classifications, or
  • Only lines with observed wavelengths.
  • Only lines with plasma-diagnostics data.

  The default is to display all lines of data meeting the search criteria, regardless of whether the lines contain transition probability data, energy level classifications, or plasma-diagnostics data.

• Choice of display of the plasma-diagnostics data:

  Plasma diagnostics data were added to ASD when version 5.3 was released. For the list of spectra that include these data, refer to the Version History (search for the word "diagnostics"). To include the diagnostics data in the Lines output, check the corresponding checkbox.

• Choice of bibliographic information output:

  If the corresponding checkbox is checked, the bibliographic references for transition probabilities (TP) and spectral lines will be shown in two separate columns.

• Choice of display of wavelength data:
  • Observed wavelength
  • Ritz wavelength
  • The default is to suppress the display of the "observed-Ritz" column of data. Checking the "observed-Ritz" option will cause that column of data to be generated in the output.
    
    
• Choice of wavelength type:

  The default is to display wavelengths in:
     Vacuum (< 200 nm), Air (200 nm to 2,000 nm), Vacuum (> 2,000 nm).

  For wavelength ordered output, the table headings for the wavelength columns change as needed to reflect the change in wavelength type.

  For multiplet ordered output, the type of the output value (wavelength in air or vacuum or wavenumber, which is always in vacuum) and the measurement units are specified in a separate column next to the values.

  Alternative choices are:
  • Vacuum (< 200 nm), Air (200 nm to 1,000 nm), Wavenumber (> 1,000 nm)
  • Vacuum (< 1,000 nm), Wavenumber (> 1,000 nm)
  • Vacuum (< 200 nm), Air (200 nm to 2,000 nm), Vacuum (> 2,000 nm)
  • Vacuum (all wavelengths)
  • Vacuum (< 185 nm), Air ( (> 185 nm))
  • Wavenumber (all wavelengths)

  Note that the formula we use for the refractive index of air was experimentally verified in the wavelength range between 185 nm and 1690 nm. The refractive index of air is not known for wavelengths outside of this range, where air strongly absorbs all radiation. For this reason, wavelengths shorter than 185 nm and 1690 nm cannot be displayed in air. For wavelengths >1690 nm, output of wavelengths in air is allowed, because the formula for the refractive index of air behaves smoothly in this range. However, the users should be cautious when using such wavelengths, as their validity is uncertain.

To change the default, the user simply needs to click on one of the radio buttons. The user will also need to check appropriate checkboxes if individual columns of wavelength information are desired:

• Choice of display of transition strength information. The default is to display the following columns of data:
  • A_ki,
  • Accuracy,
  • Relative intensity.

  By default, the A_ki (or g_kA_ki) are displayed in units of s⁻¹. They can be displayed in units of 10⁸ s⁻¹ if a proper checkbox is checked.
  
  To suppress display of the Relative Intensity data column, the corresponding checkbox can be unchecked.

  Although the f_ik, S, and log(gf) values are not displayed by default, if the corresponding checkboxes are clicked, then those data values will be displayed.

• Choice of transition type:
  
  By default, both electric dipole-allowed (E1) and forbidden (M1, E2, M2,...) transitions are displayed in the output. To display only allowed or only forbidden transitions, a user must uncheck the checkbox corresponding to the unwanted type of transitions.
  
  
• Choice of level information: For lines output, the default is to display:
  • Configurations,
  • Terms,
  • Energies, and
  • J values.

  To suppress display of the information listed above, the corresponding checkbox can be unchecked.

 Lines Output

• Tabular Output
• Graphical Output
  • Dynamic Plots:
    • Line Identification Plots
    • Saha-LTE Spectrum Plots
  • Grotrian Diagrams

 Output Line Tables

The output on the screen is HTML-formatted by default, but a significantly faster ASCII format may also be selected. The output will be even faster and more suitable for saving and viewing in other software, such as Excel or other spreadsheet viewers, if the No Javascript box is checked in the Optional Search Criteria section in the Advanced Settings block of the Lines Input Form. This box is automatically checked when the user selects the ASCII format. However, it can be unchecked if the output is intended solely for browsing purposes. The links to the online content of the bibliographic references are included in the output only if the No Javascript box is not checked.

Help popup windows

The output may contain some symbols or combinations thereof colored in red. This means that moving a mouse over such symbols would result in appearance of a small popup window showing some explanatory text provided the Javascript language is enabled in the browser options or preferences. Moving the mouse out would remove the popup window unless a user clicked on the red symbols. In that case, the popup window remains visible until the next mouse click on the same symbols. For the Ritz wavelengths, such popup windows appear also for the brown asterisk and pink plus symbols after the Ritz wavelengths (see below).

 Explanation of the Lines Tables

• Ion
• Observed Wavelength, Ritz Wavelength, and Obs.-Ritz Wavelength
• Wavelength Uncertainties
• Wavenumbers
• Rel. Int: Relative Intensity
• Transition Strengths, Accuracy
• E_i-E_k: Lower level and upper level energies
• Configurations: Configurations of the lower and upper levels
• Terms : Terms of the lower and upper levels
• J-values: the total electronic angular momenta of the lower and upper levels
• g_i-g_k: Lower level statistical weight (g_i=2J_i+1) - upper level statistical weight (g_k=2J_k+1)
• Type: Transition type and multipolarity: electric dipole, magnetic quadrupole, etc.
• TP Ref.
• Line Ref.
• Plasma diagnostics data
• Line Identification Plots
• Saha-LTE plots

 Ion

Observed Wavelength, Ritz Wavelength, and Obs.-Ritz Wavelength

The user may choose to display both Ritz and observed wavelengths. The Obs-Ritz value may also be displayed. By default, wavelengths are given for vacuum wavelengths below 200 nm and above 2000 nm, with standard-air wavelengths in between. Conversion between the air and vacuum wavelengths used in ASD is explained here.

 Uncertainties of Observed and Ritz Wavelengths

All uncertainties given in ASD are meant to be on the level of one standard deviation.

Wavenumbers

• The "Wavenumber (all wavelengths)" radio button can be selected in the Additional Criteria section of the Advanced Settings block of the Lines Search Form.
  
  In this case, instead of the observed and Ritz wavelengths and their uncertainties, the wavenumbers and their uncertainties will be displayed, and the "Obs-Ritz" column will contain the differences between the observed and Ritz wavenumbers.
  
  
• The "Wavenumber" box can be checked in the Additional Criteria section of the Advanced Settings block of the Lines Search Form.
  
  This option will have an effect only if the "Wavenumber (all wavelengths)" was not selected (see above). An additional column containing the wavenumbers will be included in the output table to provide a quick reference to the wavenumber scale corresponding to the observed and Ritz wavelengths. For lines that have an observed wavelength, the value given in this column is the observed wavenumber as it is stored in ASD. In some spectra, these values are directly quoted from the literature sources for the corresponding lines, and their precision may be greater than that of the observed wavelengths. However, in most cases they were calculated from the observed wavelengths (using the standard air to vacuum conversion where appropriate) and rounded according to the "rule of 25."
  
  For lines that do not have an observed wavelength, the value given is the Ritz wavenumber, and it is shown in italics.

 Significant Figures

• Uncertainty of the value should be no less than 2.5 units of the least significant figure of the value. This is dictated by statistical properties of rounded decimal numbers. All uncertainties given in ASD are meant to be on the level of one standard deviation.
• The given energy levels and wavelengths should be internally consistent.

• Legacy data.
  
  Some early researchers rounded their measured data too harshly with the intention of giving the data thought to be valid to the last given figure. Besides the fact that it is impossible in principle (there is always a finite probability that the rounded value contains an incorrect last digit), such rounding precludes the use of the results in rigorous statistical analyses.
  
  
• Systematic errors in measurements.
  
  In some cases, absolute positions of measured wavelengths contain poorly known systematic shifts and thus are of poor accuracy, but separations between them could be measured much more accurately. This requires giving additional figures in the wavelength values to avoid loss of accuracy.
  
  
• Theoretical data.
  
  It is especially difficult to estimate uncertainties of purely theoretical data. Systematic errors caused by approximations used in the calculation may lead to poor absolute accuracy, but the intervals between the calculated energy levels may be much more accurate. In such cases, we may give more significant figures than justified by the total uncertainty. This concerns the Ritz wavelengths derived from purely theoretical levels.

 Wavelengths

When there is no stored Ritz wavelength value in ASD, it is calculated online from the available energies of the lower and upper levels, and either an asterisk "*" or a plus "+" is appended to the Ritz wavelength value. The former simply indicates that this value was calculated online, while the latter points out that there are no critically evaluated values of the level uncertainties in ASD, and their estimation involves a number of trailing zeros in the stored energies, which were presumed insignificant. Therefore, the actual accuracy of the Ritz wavelengths followed by "+" may be higher. This involves only the energy values that do not contain a decimal point, usually in highly ionized atoms.

The subsequent procedure depends on the type of wavelength to be displayed: in vacuum or air.

• If the wavelength is to be displayed in vacuum,
  • Observed wavelengths are displayed with the same relative precision as they are stored, regardless of the uncertainty. The latter is given with the same precision as the wavelength.
  • Ritz wavelengths are always calculated from the energy levels. If we have a stored critically evaluated value of the Ritz wavelength, its precision is preserved in the output. Otherwise, it is rounded according to the rule of 25 using the stored or estimated uncertainty value. Estimated uncertainties are not displayed in ASD, as they are not critically evaluated. Critically evaluated uncertainties are displayed with the same precision as the Ritz wavelengths.
    
    Precision of the stored Ritz wavelengths overrides the rule of 25 for the following reason:
    
    There are many cases when the energy levels derived from observed wavelengths are strongly correlated, i.e., the intervals between them are known more accurately than the energy levels themselves (which are defined as separations from the ground level). In such cases, more significant figures may be required to adequately represent the data precision.
• If the wavelength is to be displayed in air,
  • If the uncertainty of the air refractive index δn/n is less than 10 % of the relative uncertainty of the wavelength, the wavelength uncertainty is not modified, and the precision of the output values is determined by the same rule as for vacuum wavelengths (see above).
  • Otherwise, the relative uncertainty of the wavelength δλ/λ is combined in quadrature with δn/n. If the latter is smaller than half of the wavelength uncertainty stored in ASD, the number of significant figures in both the wavelength and its increased uncertainty will be preserved as stored in ASD. Otherwise, both are rounded according to rule of 25. ASD displays critically evaluated uncertainties only.

 Wavenumbers

The Ritz wavenumbers are calculated from the energy levels stored in ASD. Their precision is entirely determined by their uncertainties, either stored in ASD (if they were critically evaluated) or estimated from the uncertainties of the energy levels by combining in quadrature the uncertainties of the lower and upper level of the transition. If there are no stored critically evaluated uncertainties of the levels, they are estimated as ten units of the least significant figure of the level value. Then the wavenumber value is rounded according to the rule of 25.

Definition of Ritz wavelength and wavenumber

σ = E_k − E_i.

The Ritz wavelength λ in vacuum is equal to the inverse of σ. If σ is in units of cm⁻¹, and λ is in nanometers,

λ_vac [nm] = 10⁷/(σ [cm⁻¹]).

Wavelengths in air are decreased by the refractive index of air.

Rounding Rule of 25

If the rounding is too harsh, i.e., the uncertainty is smaller than 2.5 units of the least significant figure, the value of the uncertainty is statistical meaningless and the rounded value cannot be used in rigorous statistical analyses. See more about it in A. E. Kramida, Comput. Phys. Commun. 182, 419–434 (2011).

If the rounding is too mild, i.e., the uncertainty is greater than 2.5 units of the least significant figure, the precision of the value cannot be used to estimate the uncertainty. In cases when there are strong correlations between the given values, mild rounding may be needed to adequately represent the relative uncertainties of the presented data.

 Conversion between air and vacuum wavelengths

In ASD, the index of refraction of air is derived from the five-parameter formula given by E.R. Peck and K. Reeder, J. Opt. Soc. Am. 62, 958 (1972). These authors fitted data between 185 nm and 1700 nm. The conversion between air and vacuum wavelength entails an ambiguity near the boundary of the air region. For example, a wavelength of 200.0648 nm in vacuum corresponds to 200.0000 nm in "standard air" (i.e., 15 °C, 101 325 Pa pressure, with 0.033 % CO₂). Conversely, an air wavelength of 199.9352 &nm corresponds to 200.0000 nm in vacuum. In this database, as the default, the following convention is adopted in terms of the energy difference or wavenumber, σ=E_k-E_i:

Thus, if the tabulated wavelength lies within 200 ± 0.0648 nm, one must check the energy difference to ascertain whether it is for vacuum or air.

The relative uncertainty δλ/λ of the formula of Peck & Reeder is 5×10⁻⁹ for wavelengths λ > 400 nm and increases according to the approximate formula

for shorter wavelengths (λ is in nm). The maximum uncertainty is about 9×10⁻⁸ at 185 nm.

It should be noted that a number of other formulas for the refractive index of air exist in the literature. In particular, the formulas given by K. P. Birch and M. J. Downs, Metrologia 31, 315–316 (1994) have a five times lower uncertainty than the formula of Peck & Reeder, but only in a restricted wavelength range from 350 nm to 650 nm. Their validity in the extended wavelength region covered by the Peck & Reeder formula has never been verified.

Similarly, the "corrected" formulas given by P. E. Ciddor, Appl. Opt. 35, 1566–1573 (1996) are valid only in the wavelength range from 350 nm to 1200 nm and give increasingly large errors for shorter wavelengths: about −1.0×10⁻⁸ at 228 nm and −1.6×10⁻⁶ at 185 nm.

 Relative Intensity

These are values intended to represent the strengths of the lines of a spectrum as they would appear in emission. The values in the Database are taken from the cited publications. Usually, they are not normalized in any way. In some cases, the intensity values were derived from observed photometric signals. This would be true for spectra measured by Fourier transform spectroscopy or in special cases where spectra were recorded photometrically. However, in most cases the values represent blackening of photographic emulsions used to record an observed spectrum. These values can be semi-quantitative in that the transmission of the blackened emulsion was quantitatively measured and used to determine the intensity values. In other cases, the blackening was estimated visually and the estimates were used for the intensity values. Thus, the values can range from being approximately quantitative to only qualitative. Since the Database does not contain information on the origin of the relative intensities, the relative intensities should be considered as qualitative values that describe the appearance of a particular spectrum in emission.

1. There is no common scale for relative intensities. The values in the database are taken from the values given by the authors of the cited publications. Since different authors use different scales, the relative intensities have meaning only within a given spectrum; that is, within the spectrum of a given element in a given stage of ionization.
2. The relative intensities are most useful in comparing strengths of spectral lines that are not separated widely. This results from the fact that most relative intensities are not corrected for spectral sensitivity of the measuring instruments (spectrometers, photomultipliers, photographic emulsions).
3. The relative intensities for a spectrum depend on the light source used for the excitation. These values can change from source to source, and this is another reason to regard the values as being only qualitative.

Descriptors to the relative intensities have the following meaning:

     *    Intensity is shared by several lines (typically, for multiply classified lines).
     :    Observed value given is actually the rounded Ritz value, e.g., Ar IV, λ = 443.40 Å.
     -    Somewhat lower intensity than the value given.
     a    Observed in absorption.
     b    Band head.
     bl   Blended with another line that may affect the wavelength and intensity.
     B    Line or feature having large width due to autoionization broadening.
     c    Complex line.
     d    Diffuse line.
     D    Double line.
     E    Broad due to overexposure in the quoted reference
     f    Forbidden line.
     g    Transition involving a level of the ground term.
     G    Line position roughly estimated.
     H    Very hazy line.
     h    Hazy line (same as "diffuse").
     hfs  Line has hyperfine structure.
     i    Identification uncertain.
     j    Wavelength smoothed along isoelectronic sequence.
     l    Shaded to longer wavelengths; NB: This may look like a "one" at the end
          of the number!
     m    Masked by another line (no wavelength measurement).
     p    Perturbed by a close line. Both wavelength and intensity may be affected.
     q    Asymmetric line.
     r    Easily reversed line.
     s    Shaded to shorter wavelengths.
     t    Tentatively classified line.
     u    Unresolved from a close line.
     w    Wide line.
     x    Extrapolated wavelength

The difficulty of obtaining reliable relative intensities can be understood from the fact that in optically thin plasmas the intensity of a spectral line is proportional to:

I_ik N_kA_kihν_ik,

 Transition Strengths

Either transition probability "A_ki" weighted transition probability "g_kA_ki" (s⁻¹ or 10⁸ s⁻¹), absorption oscillator strength or f value ("f_ik"), line strength "S", or "log(gf)" can be displayed. Note that f_ik, S, and log(gf) are not displayed by default. Also note that log(gf) is shorthand for log₁₀(g_i f_ik).

A_ki represents the emission transition probability. In the following formulas, it is assumed to be in units of 10⁸ sec⁻¹.

f_ik is the absorption oscillator strength or f-value.

f_ik = A_ki ·1.49919·10⁻¹⁶ g_k/g_i λ², for all multipole types,
where λ is the wavelength in ångströms

log(gf) is the log₁₀(g_i f_ik), where g_i = 2J_i + 1.

S is the line strength. It is the electric dipole matrix element squared and is independent of the transition wavelength.

More details on these quantities can be found in this review.

 Accuracy

The uncertainties are obtained from critical assessments, and in general, reflect estimates of predominantly systematic effects discussed in the NIST critical compilations, cited in the Bibliography. Accuracies are not available for values listed in the CRC handbook.

If the accuracy is followed by a prime (′), then a multiplet in the original compilation has been separated into its component lines and the transition probability was derived from the compiled value assuming pure LS coupling. This may decrease the listed accuracy, especially for weaker transitions.

 Conversion between transition probabilities and line strengths

where λ is the wavelength in angstroms and g_k is the statistical weight of the upper level. The numerical factor for the electric quadrupole conversion from A_ki to S follows a more modern convention than that used in the original publications, which will be used in future NIST publications.

 E_i-E_k

If the "No Javascript" checkbox is not checked, the level energies appear in the output as active links, even if the ASCII format is chosen. Clicking on such an active level-value link will open a new tab containing a list of all lines originating from or terminating on this level.

Configurations

Terms 

J-values

g_i-g_k

Type

M1    - Magnetic dipole.
E2    - Electric quadrupole.
M2    - Magnetic quadrupole.
E3    - Electric octupole.
M3    - Magnetic octupole.
M1+E2 - Mixed magnetic dipole and electric quadrupole transition.
        The selection rules for these two types of transitions are the same, so
        both types of transitions can contribute to the observed intensity and
        radiative rate Aki. The line strength is undefined for such mixed transitions.
2P    - Two-photon transition.
HF    - Hyperfine-induced transition (may occur only in isotopes with a
        non-zero nuclear magnetic moment).
UT    - Forbidden transition of an unspecified type.


Transitions that are strongly forbidden in isolated atoms may be enabled by environmental effects such as external electric or magnetic fields. Such forbidden transitions would be denoted as type = UT in ASD.

 TP Ref. and Line Ref.

Plasma diagnostics data

 Graphical Output

 Dynamic Plots

Line Identification Plot

The Line Identification Plot is a stick plot showing the line positions for all chosen ions in the given wavelength range. It can be used to diagnose which ions produce spectral lines is an observed spectrum. For that, the image should be magnified or reduced to approximately the same wavelength scale as in the experimental spectrum. Then the patterns of intervals between the observed spectral lines could be matched with those in one or more of the ion spectra in the Line Identification Plot, which can help the user to identify the observed lines.

If there are too many lines in the chosen spectra, the user can use the "Relative intensity minimum" or other options in the Optional Search Criteria section in the Advanced Settings block of the Lines Input Form to reduce the number of shown lines.

Spectrum Image Plots

Saha-LTE Spectrum Plots

If the "Saha-LTE Plot" option has been selected on the Lines Form, two or more links will appear at the very bottom of the tabular output page. One of them is a link to a PDF file containing an image of the plot. One of the other links with text "Relative Line Intensities" is to a new popup window displaying the wavelengths of the spectral lines shown on the PDF plot and their relative intensities. If the user requested a Doppler-broadened spectrum (by checking the corresponding box in the Lines Form), there will be two additional links, one to table of calculated intensities of each ion in the Doppler-broadened spectrum, and one to a table showing the distribution of intensities in the total spectrum (sum of contributions from each ion). Both these tables are two-column plane fixed-column-width ASCII files with the first column having the wavelength grid points and the second column having relative intensities in arbitrary units. These tables can be used to plot the spectra with other software.

The header of the plot shown in the PDF file shows the user-defined parameters: composition of the element mixture in the plasma, electron temperature and density, as well as the total number of lines in the synthetic spectrum. If a Doppler-broadened spectrum was requested, the header also shows the ion temperature used to calculate the Doppler broadening. It may be greater than the Ion Temperature specified by the user in the Lines Input Form, if the number of required points in the grid was too large for the given selection of spectral lines. In such cases, to display narrower lines (corresponding to a lower ion temperature), the user needs to reduce the selected wavelength range, reduce the number of requested spectra, or use some line-filtering options in the Optional Search Criteria section in the Advanced Settings block of the Lines Input Form.

If higher resolution (narrower lines) is needed, and only neutral, singly-ionized, or doubly-ionized atoms are involved, consider using the LIBS Interface of ASD. Although this interface does not allow drawing spectra for a particular ionization stage, its plots can be calculated on the user's computer with much higher resolution, and they have flexible interactive features.

 Plotting Grotrian diagrams

Working with the Grotrian diagram plot

Basically, only a computer mouse and a space bar are used for interaction with this plot.

• Default view
  
  Initially all levels and transitions are shown on the Grotrian Diagram (GD) plot. Each energy level is shown by a horizontal bar. The colors (black and blue) have no meaning and are used simply to help with visualization of the plot. The X-axis corresponds to different level series, and the Y-axis shows the level energy in cm⁻¹. The radiative transitions between the levels are shown as slanted gray lines. The ionization limits are shown as magenta horizontal lines. At the top of the plot, the total number of levels, lines and ionization limits is displayed. These parameters are automatically updated when zooming in or out. In the bottom right part of the plot, the maximum and minimum values of the transition probability for the displayed lines are given in the input text fields. The "Submit" and "Reset" buttons are used for setting the limits for transition probabilities, while the "Isolate" button is used to single out one level and all relevant transitions. The green field ("zoom field" below) next to the Y-axis is used for zooming in and out. Below, the top right part of the plot will be referred to as the "info field."
  
  
• Controls block
  
  The appearance of the GD plot can be changed in many ways by using the various control elements (action buttons, radio buttons, and input boxes) located in the control block above the GD plot. These control elements are explained below.

• Plot size
  A user change the size of the GD plot by clicking on the "Enlarge" or "Shrink" buttons.
  
  
• Grouping by configuration, subconfiguration, or J values
  By default, the levels are grouped into series according to their electronic-shell configuration. For instance, in O I the levels belonging to configurations 2s²2p³nl (l = s, p, d, f, g) or 2s2p⁴np are assigned to different series, each displayed in a separate vertical column in the plot. However, there are different core configurations in all these series, and stronger transitions tend to occur between the series having the same core. To better see the connections between the series based on different cores, the user can choose grooping of levels by subconfigurations. In this case, the 2s²2p³(⁴S°)nl and 2s²2p³(²D°)nl levels would be assigned to different series. For the purpose of seeing connections between the levels having different total orbital momentum J, the levels can be grouped by J. The choice of level grouping is made in the "Group by" set of radio buttons in the left part of the control block
  
  
• Filtering by J-values, multiplicities, configurations, and subconfigurations
  The menus with the corresponding names contain the sets of values available for the chosen spectrum. By default, all these values are included in the selection of levels displayed in the plot. The user can restrict the number of levels and transitions displayed by selecting a subset of the available values and then clicking the "Filter lines/levels" button. For example, selecting only "3" in the "Multiplicities" menu for O I would result in display of only triplet levels and transitions between them, while selecting only "0" and "1" in the "J values" menu would produce a GD only for levels having J = 0 and 1 and corresponding transitions. Clicking the button "Reset filters" will restore the default setting (no filtering).
  
  
• Show only radiatively linked levels
  By default, all levels belonging to the chosen ion are displayed in the GD. Selecting the "Radiatively linked" option would result in display of only those levels that are connected by radiative transitions.
  
  
• Filtering A-values
  The range of A-values for transitions displayed in the GD can be specified by entering the limiting values in the "min A" and "max A" input boxes and then clicking the "Filter lines/levels" button. By default, the values in these boxes are 0 and the maximum available A-value for this spectrum. The zero minimum value implies that transitions with unknown A-values are included in the GD.
  
  Other filtering options, such as displaying only the observed lines, only the allowed or forbidden lines, as well as different units for levels and wavelengths can be implemented by returning to the Lines Input form and sellecting appropriate options in the Advanced Settings section.
  
  

• Selecting, deselecting and cycling over objects
  
  Mouse:
  
  • Clicking on any level colors it and all relevant transitions in red. In addition, the basic data on this level, e.g., energy, configuration, etc., are displayed in the info field.
  • Clicking on any line colors the line and the lower and upper level in red. In addition, the basic data on the levels and line (wavelength, transition probability, etc.) are shown in the info field.
  • Consecutive clicking on two levels is equivalent to clicking on the corresponding spectral line. If there is no line connecting the levels, no Line information is shown in the info field although the data on both levels are displayed.
  • Clicking anywhere in the white background of the GD subwindow deselects the already selected object(s).
    
    
  Space bar:
  
  • If no objects have been selected, pressing a space bar selects a first spectral line in the following order: the levels are assumed to be arranged first according to the X-axis label (from left to right) and then according to the level energy. Since the ground state always has a zero energy, pressing the bar would normally highlight a line originating from the ground state.
  • If a line has been selected, pressing a space bar cycles over all spectral lines on the plot in the order described above, that is, (i) for the same lower level, the upper level is updated, and (ii) after all lines for a particular lower level have been cycled through, the lower level is updated, and so on.
  • If a level has been selected, pressing a space bar cycles over all energy levels within the levels series.
  • The data shown in the info field is the same as for the mouse selection.
    
    
• Zooming in and out
  
  The green field to the right of the Y-axis is used for zooming in. The upper and lower limits for the energy levels are set up by clicking the mouse in the zoom field. The upper and lower limits are shown by horizontal blue lines. When both limits are selected, the "Zoom" button above the Y-axis becomes highlighted and clicking on it with the mouse results in updating the subwindow. This procedure can be repeated infinitely. After zooming in, the "Reset" button on the above the Y-axis becomes highlighted, and clicking on it restores the original plot.
  
  
• Isolating a level
  
  In order to isolate one energy level with all radiatively connected levels, one has first to select a level by a mouse click. Then, the "Isolate" button in the bottom right part of the plot becomes highlighted, and pressing it would result in displaying the red group of levels and lines only. If necessary, a user can then perform zoom or transition probability limiting procedures on this subset of levels. After isolating a level, the "Isolate" button changes its label to "Show All," and pressing this new button would show all available levels and transitions.

 Creating an output for importing into a spreadsheet