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Detailed Description of J/A+AS/140/191
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Individual files can be fetched (via http) from
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The catalogue can be queried from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+AS/140/191
This standardized document follows the rules of the Standard Description for Astronomical Catalogues. For those having to work on this catalogue using FORTRAN programs, this ReadMe file can be transformed into a f77-compliant program which reads the files making up this catalogue, in two versions: either a f77 program loading whole files into arrays, or a f77-program reading each data file line by line.
J/A+AS/140/191 Stark broadening of Ca I (Dimitrijevic+, 1999)
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Stark broadening of neutral calcium spectral lines
Dimitrijevic M.S., Sahal-Brechot S.
<Astron. Astrophys. Suppl. Ser. 140, 191 (1999)>
=1999A&AS..140..191D
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ADC_Keywords: Atomic physics
Keywords: atomic data - line profiles
Abstract:
Using the semiclassical perturbation approach, we have calculated
electron-, proton-, He II-, Mg II-, Si II- and Fe II-impact line
widths and shifts for 189 Ca I multiplets as a function of
temperature and perturber density. Perturbers selected here are
the main perturbers in solar atmospheres. Obtained results have
been compared with the existing theoretical and experimental data.
File Summary:
FileName Lrecl Records Explanations
× ReadMe 80 . This file
× table1.dat 123 1134 Stark broadening parameters due to e-, p- and
He II-impacts for Ca I for a perturber density
of 1.E+11cm-3.
× table2.dat 123 2862 Stark broadening parameters due to e-, p- and
He II-impacts for Ca I for perturber densities
1.E+12cm-3 - 1.E+19cm-3.
× table3.dat 123 1134 Stark broadening parameters due to Mg II-,
Si II- and Fe II-impacts for Ca I for a
perturber density of 1.E+11cm-3.
See also:
VI/98 : Stark broadening of H lines (Stehle+, 1999)
Stark broadening of other elements (Dimitrijevic, Sahal-Brechot, Popovic)
J/A+AS/105/243 : BeI lines (Dimitrijevic+ 1994)
J/A+AS/105/245 : Al XI and Si XII (Dimitrijevic+ 1994)
J/A+AS/107/349 : Ne VIII and Na IX (Dimitrijevic+ 1994)
J/A+AS/109/551 : OIV and OV (Dimitrijevic+ 1995)
J/A+AS/115/351 : C V and P V (Dimitrijevic+, 1996)
J/A+AS/116/359 : Xe II lines (Popovic+, 1996)
J/A+AS/117/127 : solar Mg I lines (Dimitrijevic+, 1996)
J/A+AS/119/369 : Be III and B III (Dimitrijevic+, 1996)
J/A+AS/119/529 : Sr I spectral lines (Dimitrijevic+, 1996)
J/A+AS/120/373 : Sc II, Y II and Zr II Stark width (Popovic+ 1996)
J/A+AS/122/163 : Ba I and Ba II lines (Dimitrijevic+, 1996)
J/A+AS/122/533 : P IV spectral lines (Dimitrijevic+, 1997)
J/A+AS/127/295 : Kr II lines (Popovic+ 1998)
J/A+AS/127/543 : S V lines (Dimitrijevic+ 1998)
J/A+AS/128/203 : Mn, Ga & Ge multiplets (Popovic+ 1998)
J/A+AS/128/359 : Ca IX and Ca X lines (Dimitrijevic+ 1998)
J/A+AS/129/155 : Si XI and Si XIII lines (Dimitrijevic+ 1998)
J/A+AS/130/539 : Na X (Dimitrijevic+ 1998)
J/A+AS/131/141 : O VII and Mg XI (Dimitrijevic+ 1998)
J/A+AS/131/143 : Sc X, Sc XI, Ti XI and Ti XII (Dimitrijevic+ 1998)
J/A+AS/133/227 : K VIII and K IX (Dimitrijevic+ 1998)
J/A+AS/140/193 : Zn I (Dimitrijevic+ 1999)
J/A+A/400/791 : Be III (Dimitrijevic+ 2003)
J/A+A/417/375 : Cd III (Milovanovic+, 2004)
J/A+A/423/397 : Si V (Ben Nessib+, 2004)
J/A+A/425/1147 : Ga I (Dimitrijevic+, 2004)
Byte-by-byte Description of file: table[12].dat
Bytes Format Units Label Explanations
1- 7 E7.2 cm-3 N Perturber density
10- 13 A4 --- El Element
15- 21 A7 --- Tr Transition (4)
23- 30 F8.1 0.1nm lambda Wavelength
33- 40 E8.2 0.1nm/cm3 C Parameter C (1)
43- 50 F8.0 K T Temperature
52 A1 --- n_We [*] (5)
53- 61 E9.3 0.1nm We FWHM for electron impacts (2)
63 A1 --- n_de [*] (5)
64- 73 E10.3 0.1nm de shift for electron impacts (3)
76 A1 --- n_Wp [*] (5)
77- 85 E9.3 0.1nm Wp FWHM for proton impacts (2) (6)
88 A1 --- n_dp [*] (5)
89- 98 E10.3 0.1nm dp shift for proton impacts (3) (6)
101 A1 --- n_WHe+ [*] (5)
102-110 E9.3 0.1nm WHe+ FWHM for He II-impacts (2)
113 A1 --- n_dHe+ [*] (5)
114-123 E10.3 0.1nm dHe+ shift for He II-impacts (3)
Note (1): C/FWHM gives an estimate of the maximum perturber density for which
the line may be treated as isolated and tabulated data may be used
Note (2): FWHM denotes Full Width at Half Maximum
Note (3): A positive (resp. negative) shift is towards the red (resp. blue)
Note (4): In the first part of the Table are singlets and in the second triplets
Note (5): An asterisk in this column indicates that 0.1<NV<0.5, (V = collision
volume); beware of the fact that the limit of validity of
the impact approximation is attained for the value that follows
Note (6): Values for NV>0.5 are not given, because in this case the impact
approximation is no longer valid
Byte-by-byte Description of file: table3.dat
Bytes Format Units Label Explanations
1- 7 E7.2 cm-3 N Perturber density
10- 13 A4 --- El Element
15- 21 A7 --- Tr Transition (4)
23- 30 F8.1 0.1nm lambda Wavelength
33- 40 E8.2 0.1nm/cm3 C Parameter C (1)
43- 50 F8.0 K T Temperature
53- 61 E9.3 0.1nm WMg+ FWHM for Mg II impacts (2)
64- 73 E10.3 0.1nm dMg+ Shift for Mg II impacts (3)
77- 85 E9.3 0.1nm WSi+ FWHM for Si II impacts (2)
89- 98 E10.3 0.1nm dSi+ Shift for Si II impacts (3)
102-110 E9.3 0.1nm WFe+ FWHM for Fe II-impacts (2)
114-123 E10.3 0.1nm dFe+ Shift for Fe II-impacts (3)
Note (1): C/FWHM gives an estimate of the maximum perturber density for which
the line may be treated as isolated and tabulated data may be used
Note (2): FWHM denotes Full Width at Half Maximum
Note (3): A positive (resp. negative) shift is towards the red (resp. blue)
Note (4): In the first part of the Table are singlets and in the second triplets
Acknowledgements: Dr Milan Dimitrijevic
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(End) Patricia Bauer [CDS] 09-Sep-1999
