High Accuracy Near-infrared Carbon Dioxide Intensity Measurements To Support Remote Sensing
Department of Commerce
@usgov.doc_gov_high_accuracy_near_infrared_carbon_dioxide_int_219bf4b3
Department of Commerce
@usgov.doc_gov_high_accuracy_near_infrared_carbon_dioxide_int_219bf4b3
Data files for the publication "High Accuracy Near-infrared Carbon Dioxide Intensity Measurements to Support Remote Sensing" in Geophysical Research Letters
Organization: Department of Commerce
Last updated: 2020-11-12T14:51:28.662972
Tags: carbon-dioxide, greenhouse-gases, remote-sensing
CREATE TABLE figure1 (
"figure_1_relative_intensity_differences_and_correspond_1360c1b7" VARCHAR -- Figure 1. Relative Intensity Differences And Corresponding Standard Uncertainties For The Present Measurements Of The (30012) <- (00001) [top Panel], (30013) <- (00001) [middle Panel], And (30014) <- (00001),
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5,
"unnamed_6" VARCHAR -- Unnamed: 6,
"unnamed_7" VARCHAR -- Unnamed: 7,
"unnamed_8" VARCHAR -- Unnamed: 8,
"unnamed_9" VARCHAR -- Unnamed: 9,
"unnamed_10" VARCHAR -- Unnamed: 10
);CREATE TABLE figure2 (
"figure_2_retrieved_volume_mixing_ratio_scale_factors_v_0e8c20e3" VARCHAR -- Figure 2. Retrieved Volume Mixing Ratio Scale Factors (VSF) Relative To Coincident Aircraft Profiles At The Lamont, OK Total Carbon Column Observing Network (TCCON) Site On 14 January 2012 For The (30012) <- (00001) (top Panel), (30013) <- (00001) (middle Panel), (30014) <- (00001) (bottom Panel),
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5,
"unnamed_6" VARCHAR -- Unnamed: 6
);CREATE TABLE figures1 (
"figure_s1_comparison_of_the_line_mixing_parameters_det_6816f94c" VARCHAR -- Figure S1. Comparison Of The Line Mixing Parameters Determined Herein With Those Of Malathy Devi Et Al. [Malathy Devi Et Al., 2007b] At 296 K For The (30012) <-(00001) CO2 Band. Note That 1 Atm?1 = 9.869233 MPa?1.,
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4
);CREATE TABLE figures2 (
"figure_s2_comparison_of_the_line_mixing_parameters_det_607687c6" VARCHAR -- Figure S2. Comparison Of The Line Mixing Parameters Determined Herein With Those Of Malathy Devi Et Al. [Malathy Devi Et Al., 2007a] At 296 K For The (30013)?(00001) CO2 Band. Note That 1 Atm?1 = 9.869233 MPa?1.,
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4
);CREATE TABLE figures3 (
"figure_s3_upper_panel_model_solar_spectrum_for_the_300_30a9fd50" VARCHAR -- Figure S3. (Upper Panel) Model Solar Spectrum For The (30012)?(00001) CO2 Band. Also Shown Are The Contribution Of H2O, HDO, And Solar Lines To The Observed Spectrum. (Lower Panel) Spectroscopic Residuals Arising From The Use Of The Present Intensities As Well,
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5,
"unnamed_6" VARCHAR -- Unnamed: 6
);CREATE TABLE figures4 (
"figure_s4_upper_panel_model_solar_spectrum_for_the_300_06e14559" VARCHAR -- Figure S4. (Upper Panel) Model Solar Spectrum For The (30013)?(00001) CO2 Band. Also Shown Are The Contribution Of H2O, HDO, And Solar Lines To The Observed Spectrum. (Lower Panel) Spectroscopic Residuals Arising From The Use Of The Present Intensities As Well,
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5,
"unnamed_6" VARCHAR -- Unnamed: 6
);CREATE TABLE figures5 (
"figure_s5_upper_panel_model_solar_spectrum_for_the_300_49654e41" VARCHAR -- Figure S5. (Upper Panel) Model Solar Spectrum For The (30014)<-(00001) CO2 Band. Also Shown Are The Contribution Of H2O, CH4, And Solar Lines To The Observed Spectrum. (Lower Panel) Spectroscopic Residuals Arising From The Use Of The Present Intensities As Well As,
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5,
"unnamed_6" VARCHAR -- Unnamed: 6
);CREATE TABLE n_30012_co2_626_betahitran (
"wavenumber_cm_1" DOUBLE -- Wavenumber (cm-1),
"line_intensity_cm_molec_at_296_k" DOUBLE -- Line Intensity (cm/molec. At 296 K)
);CREATE TABLE n_30012_co2_626_expdata (
"m" BIGINT,
"line_intensity_cm_molec_at_296_k" DOUBLE -- Line Intensity (cm/molec. At 296 K),
"type_a_unc_cm_molec_1_sigma" DOUBLE -- Type A Unc. (cm/molec., 1-sigma)
);CREATE TABLE n_30013_co2_626_betahitran (
"wavenumber_cm_1" DOUBLE -- Wavenumber (cm-1),
"line_intensity_cm_molec_at_296_k" DOUBLE -- Line Intensity (cm/molec. At 296 K)
);CREATE TABLE n_30013_co2_626_expdata (
"m" BIGINT,
"line_intensity_cm_molec_at_296_k" DOUBLE -- Line Intensity (cm/molec. At 296 K),
"type_a_unc_cm_molec_1_sigma" DOUBLE -- Type A Unc. (cm/molec., 1-sigma)
);CREATE TABLE n_30014_co2_626_betahitran (
"wavenumber_cm_1" DOUBLE -- Wavenumber (cm-1),
"line_intensity_cm_molec_at_296_k" DOUBLE -- Line Intensity (cm/molec. At 296 K)
);CREATE TABLE n_30014_co2_626_expdata (
"m" BIGINT,
"line_intensity_cm_molec_at_296_k" DOUBLE -- Line Intensity (cm/molec. At 296 K),
"type_a_unc_cm_molec_1_sigma" DOUBLE -- Type A Unc. (cm/molec., 1-sigma)
);CREATE TABLE table1 (
"n__1_gas_cylinders_utilized_in_these_measurements_incl_634038b3" VARCHAR -- Table 1. Gas Cylinders Utilized In These Measurements Including Their CO2 Mole Fractions (xCO2) And Combined Standard Uncertainties (u(xCO2)) As Well As The 13C/12C And 18O/16O Isotopic Ratios Expressed As Delta Values On The Respective Vienna-Pee Dee Belemnite Scales.,
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5
);CREATE TABLE table2 (
"n__2_estimated_systematic_relative_standard_uncertaint_561f6252" VARCHAR -- Table 2. Estimated Systematic Relative Standard Uncertainties (Type B).,
"unnamed_1" VARCHAR -- Unnamed: 1
);CREATE TABLE table3 (
"n__3_fitted_integrated_band_intensity_at_296_k_smeas_a_73204803" VARCHAR -- Table 3. Fitted Integrated Band Intensity At 296 K (Smeas) And Its Ratio Relative To HITRAN 2016 [Gordon Et Al., 2017]. We Note That SmeasŁ Was Determined Over The Range Of M Shown By The Measurements Shown In Figure 1, Thus Care Should Be Taken In Extrapolating To Large |m|. Also Shown Are The Corresponding Random (Type A), Systematic (Type B), And Relative Combined Standard Uncertainties (Total Unc.), The Reduced Chi-squared(Red. Chi. Sq.),
"unnamed_1" VARCHAR -- Unnamed: 1,
"unnamed_2" VARCHAR -- Unnamed: 2,
"unnamed_3" VARCHAR -- Unnamed: 3,
"unnamed_4" VARCHAR -- Unnamed: 4,
"unnamed_5" VARCHAR -- Unnamed: 5,
"unnamed_6" VARCHAR -- Unnamed: 6,
"unnamed_7" VARCHAR -- Unnamed: 7
);Anyone who has the link will be able to view this.