J/A+AS/145/491      Lyα dipolar emission              (Gonzalez, 2000)

Tables of dipolar emission and two-photon absorption Lyman-α profiles Gonzalez M.A., Gigosos M.A. <Astron. Astrophys. Suppl. Ser. 145, 491 (2000)> =2000A&AS..145..491G 2000A&AS..145..491G
ADC_Keywords: Line Profiles ; Atomic physics Keywords: line profiles - plasmas Description: Computer simulation techniques have been used to calculate the Stark broadening profiles of the hydrogen dipolar Lyman-α transition and of two-photon absorption, dispersion and polarization profiles in the 1S->2S transition. The calculations have considered electron densities in the range between 4.64*1019(m-3) and 1*1023(m-3), and temperatures in the range between 2000 and 100000K. The fine structure of level n=2 has been taken into account in the calculations. Four different sets of tables are given. The two first sets are the tables of the autocorrelation function for the dipolar moment of the emitter and for the operator that gives the transition amplitude for a two-photon absorption between the 1S and the 2S levels. This tables have the names rXXnYYYY.c1p and rXXnYYYY.c2p. The .c1p and .c2p extensions stands for 1 photon dipolar moment and for two-photon absorption transition amplitude. XX is 100*ρ, ρ being the quotient between the mean distance between particles and the Debye radius for the conditions of the plasma for which the profiles where calculated. YYYY is 100*Log(Ne), Ne being the electron density (m-3) of the plasma considered. The last two sets of tables correspond to the 1 photon Lyman-α profiles (rXXnYYYY.d1p) and to two-photon polarization profiles (rXXnYYYY.p2p). In each file the results obtained considering perturbers of different reduced masses (µ) are tabulated in different columns. The caption of each file contains the conditions of electron density and plasma temperature for which the calculation was made. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file ident.dat 51 280 Initial parameters files/* . 281 Data files (280 data files + data description file) c1p.dat 127 17920 Autocorrelation functions for dipolar emission (tables rXXnYYYY.c1p) c2p.dat 127 17920 Autocorrelation functions for 2 photon absorption (tables rXXnYYYY.c2p) d1p.dat 89 17920 1 photon lyman-α dipolar emission profiles (tables rXXnYYYY.d1p) p2p.dat 89 17920 1S->2S two-photon polarization profiles (tables rXXnYYYY.p2p) -------------------------------------------------------------------------------- Byte-by-byte Description of file: ident.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Ident Identification parameters filename (1) 14- 25 E12.6 m-3 Ne Electronic density 27- 32 I6 K T Temperature 34- 45 E12.6 s Time ? Time step (for r*.c[12]p files) 47- 51 F5.3 --- rho ? rho parameter, i.e. mean distance between particles in Debye radius. (for r*.d1p and r*..p2p files) (G1) -------------------------------------------------------------------------------- Note (1): For c[12]p files: Density Temperature Time step For d1p.dat and p2p.dat files: Electronic density Plasma temperature ρ -------------------------------------------------------------------------------- Byte-by-byte Description of file: c1p.dat c2p.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Ident Identification parameters filename 14- 22 E9.3 s t Time in seconds 25- 33 F9.6 --- CR0.5 Autocorrelation function (real part); µ=0.5 35- 43 F9.6 --- CI0.5 Autocorrelation function (imag. part); µ=0.5 46- 54 F9.6 --- CR0.8 Autocorrelation function (real part); µ=0.8 56- 64 F9.6 --- CI0.8 Autocorrelation function (imag. part); µ=0.8 67- 75 F9.6 --- CR0.9 Autocorrelation function (real part); µ=0.9 77- 85 F9.6 --- CI0.9 Autocorrelation function (imag. part); µ=0.9 88- 96 F9.6 --- CR1.0 Autocorrelation function (real part); µ=1.0 98-106 F9.6 --- CI1.0 Autocorrelation function (imag. part); µ=1.0 109-117 F9.6 --- CR2.0 Autocorrelation function (real part); µ=2.0 119-127 F9.6 --- CI2.0 Autocorrelation function (imag. part); µ=2.0 -------------------------------------------------------------------------------- Byte-by-byte Description of file: p2p.dat d1p.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 12 A12 --- Ident Identification parameters file name 15- 25 E11.4 m DeltaL Displacement in wavelength 28- 37 E10.4 m-1 I0.5 Intensity of the profile for µ=0.5 41- 50 E10.4 m-1 I0.8 Intensity of the profile for µ=0.8 54- 63 E10.4 m-1 I0.9 Intensity of the profile for µ=0.9 67- 76 E10.4 m-1 I1.0 Intensity of the profile for µ=1.0 80- 89 E10.4 m-1 I2.0 Intensity of the profile for µ=2.0 -------------------------------------------------------------------------------- Note (G1): The Debye length is defined as (rD)2 = kTe/(4πe2Ne) Acknowledgements: Manuel Angel Gonzalez
(End) Patricia Bauer [CDS] 03-Jul-2000
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line