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- Data for: Ab initio calculations of collisional line-shape parameters and generalized spectroscopic cross-sections for rovibrational dipole lines in HD perturbed by HeDescription of supplementary material for : Ab initio calculations of collisional line–shape parameters and generalized spectroscopic cross-sections for rovibrational dipole lines in HD perturbed by He by Kamil Stankiewicz, Hubert Jóźwiak, Maciej Gancewski, Nikodem Stolarczyk, Franck Thibault, Piotr Wcisło The generalized spectroscopic cross-sections as a function of collision relative kinetic energy defined by Eq.4 are given in files HD_HeXS*.txt. The values in subsequent columns are the kinetic energy, the real part of σ0q (PBXS), the imaginary part of σ0q (PSXS), the real part of σ1q (RDXS), the imaginary part of σ1q (IDXS) and the inelastic contribution to the PBXS (Inel. Contr.). Kinetic energy is given in cm-1, the cross-sections and inelastic contribution in Å2. For example the file HD_HeXS2_0R_4.txt provides the cross-sections for the electric dipole R(4) line of the 2-0 band. The thermally averaged pressure broadening and shift coefficients (PBC and PSC), real and imaginary parts of the optical frequencies of velocity-changing collisions (Re(νopt) and Im(νopt)), defined by Eqs. 6 and 7, are given in the HD_Heline_shape*.txt files. Temperature is given in K and the values of the coefficients in 10-3 cm-1/atm. For example file HD_Heline_shape5_0P_3.txt contains data for electric dipole P(3) line of 5-0 band.
- Data for: Extinction, scattering and absorption of electromagnetic waves in the coupled-dipole approximationData for Figs.3-6: the ratio a/lambda_0, gamma/lambda_0 as encoded in the file names. The terms corr=0 means no corrections, corr=1, radiative correction only, corr=2 - nonradiative correction only, corr=3 - both corrections used. Columns: omega/omega_0, Qe, Qs, Qa. Data for Fig.7: same as above but a=5 means "a=5nm" and a=10 means "a=10nm"; the ratio gamma/omega_p=0.002 is fixed. The bfirst column is omega/omega_p. Data for Fig.9. Cubic lattice (qa_met_c) and distorted BCC lattice (qa_met_bcc). The columns are: (1) - L (size of the square in terms of the lattice step); (2) - sigma_e/sigma_g; (3) - sigma_a/sigma_g; (4) - sigma_s/sigma_g. Here sigma_g is the geometrical cross section, sigma_e is the extinction cross section, sigma_s is the scattering cross section and sigma_a is the absorption cross section. Only the first two columns (sigma_e/sigma_g vs L) are shown in Fig.3. Not all data are displayed in the plots.
- Data for: A Biased Sampling Approach to Accelerate Backward Monte Carlo Atmospheric Radiative Transfer Simulations and its Application to Arctic Heterogeneous Cloud and Surface ConditionsThe LEIPSIC results of the IPRT benchmark validations.
- Data for: Isotopologue Consistency of Semi-Empirically Computed InfraRed Line Lists and Further Improvement for Rare Isotopologues: CO2 and SO2 Case StudiesSee the README file and the abstract of paper. All intensities use 100% abundance, i.e. no terrestrial abundances.
- Data for: Different Water and Ice Cloud Optical Thickness Changes and Radiative Effects in East Asia1.MODIS_M3_08data 2. BCC_RAD radiation transfer model
- Data for: Determining complex refractive index of cellulose nanocrystals by combination of Beer-Lambert and immersion matching methods Complex refractive index of CNC as a function of wavelength (400 -700 nm) .
- Data for: Empirical rovibrational energy levels of ammonia up to 7500 cm-1Supplementary data to Empirical rovibrational energy levels of ammonia up to 7500 cm-1
- Data for: Kr I spectra in the 5–14 µm rangeinput and output files for LOPT and POLAR programs Kr1-out-lin.txt : LOPT Output line list Kr1_lin_Civis.txt : LOPT Input line list Kr1-out-lev.txt : LOPT Output level list input_polar.pol.txt output_polar.out.txt
- Data for: The N$_2$ Second Positive ($C^{3}\Pi_{u} \rightarrow B^{3}\Pi_{g}$) system reviewed: improved data and analysisThe raw data used in our work is included in this file. This listing is organized as follows: J' assignment, symmetry of the upper state, J'' assignment, symmetry of the lower state, observed wavenumber, calculated wavenumber, difference between observed and calculated wavenumbers, branch, vibrational quantum number of the upper state and vibrational quantum number of the lower state. The format chosen to send the supplementary data iss .txt, so that it can be read by any code or computer program. The intention is to make the use of this data as comprehensive as possible. At the end of the file, some extra-lines, not included in the fits, are listed. It should be noted that no assignment has been made to these last lines.
- Data for: Night Sky Brightness Monitoring Network in Wuxi, ChinaThese data reflect night sky brightness in the areas where the monitoring stations are located. The brightness of the night sky is an important factor in astronomical observation, which is also closely related to the local environment and economic development level.
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