gorshelev_2014 ============== V\. Gorshelev, A\. Serdyuchenko, M\. Weber, W\. Chehade and J\. P\. Burrows, "High spectral resolution ozone absorption cross\-sections \- Part 1\: Measurements, data analysis and comparison with previous measurements around 293 K", Atmos\. Meas\. Tech\. 7, 609 \(2014\) `Source record `__ · :doc:`Catalogue ` · :doc:`Review register ` DOI: `10\.5194/amt\-7\-609\-2014 `__ **Source kind:** measurement **Recorded technique:** Two double\-jacketed quartz cells \(140 cm long, 5 cm bore; paths 5 cm across the middle, 135 and 270 cm, and about 2000 cm with White multipass optics\), cooled by flowing ethanol \(Haake cryostats, 293\-193 K, stable to \+\-0\.3 K; internal and Pt\-100 sensors agree to 1 K\); an echelle spectrometer \(ESA 4000, ICCD; 0\.018\-0\.02 nm\) and a Bruker HR120 Fourier\-transform spectrometer \(1 cm^\-1, 2 cm^\-1 in the NIR, boxcar apodisation\); deuterium, xenon and tungsten lamps\. Absolute measurements with pure O3 \(trapped from an O2/O3 flow in liquid nitrogen, about 50 mbar\) in the Huggins band \(310\-335 nm, 135 cm\) and the Chappuis band \(450\-780 nm, 270 cm\), the O3 pressure from the total pressure during decay, p\(t\) = 3 p\_i \- 2 p\_total\(t\) \(Eq\. 3\), corrected for the decay during filling; relative measurements with O2/O3 mixtures in 213\-310 nm \(O3 left on the optics after evacuation\), 335\-350, 350\-450 and 780\-1100 nm, concatenated to the absolute ones by scaling and offset in their overlaps \(Table 1; pp\. 611\-613\)\. **Materials in structured entries:** O3 **Dataset quantities:** absorption\_cross\_section **Contents:** 29 datasets; 0 formulas. Curation notes -------------- Identity checked against the first page \(PDF page 1, journal p\. 609\)\: Gorshelev, Serdyuchenko, Weber, Chehade and Burrows, Atmos\. Meas\. Tech\. 7, 609\-624 \(2014\), Part 1 \(the 293 K measurement; Part 2 is serdyuchenko\_2014\)\. Journal pages 609\-624 = PDF pages 1\-16\. O3 only\. Facts for the data files \(the Bremen 'Serdyuchenko/Gorshelev' set\)\: \- Range and temperatures\: 213\-1100 nm at eleven temperatures 193\-293 K in 10 K steps \(abstract\); this paper analyses 293 K\. \- Resolution \(Table 1, pp\. 612\-613\)\: echelle 0\.018 nm \(213\-310 nm\) and 0\.02 nm \(350\-450 nm\), FWHM 'from about 0\.015 nm in the UV to 0\.025 nm in the visible' \(Hg\-Cd lines\); FTS 1 cm^\-1 \(310\-350 and 450\-780 nm\) and 2 cm^\-1 \(780\-1100 nm\)\: 'about 0\.01 nm in the Huggins band, 0\.02\-0\.06 nm in the Chappuis band, and 0\.12\-0\.24 nm in the Wulf band'\. Sampling\: echelle 0\.01 nm; FTS 0\.005 nm/point \(near UV\), 0\.01\-0\.03 nm/point \(visible\), about 0\.1 nm/point \(NIR\)\. The published cross sections 'were linearly interpolated onto an equidistant wavelength grid in steps of 0\.01 nm for the spectral range from 213 to 1100 nm' \(one to three interpolated points between measured ones in 450\-750 nm, up to nine in the NIR, Fig\. 2\) \(p\. 613\)\. \- Wavelengths\: VACUUM\. 'The echelle spectrometer delivers data on air wavelength scale, which was converted into vacuum wavelength scale using Edlen's equation \(Edlen, 1966\) \.\.\. Wave number scale delivered by FTS was converted into the vacuum wavelength scale' \(p\. 613\)\. Calibration accuracy 0\.005 nm \(abstract, p\. 613\)\. The comparisons were made 'on the same grid of vacuum wavelengths in steps of 0\.01 nm' \(p\. 617\)\. \- Absolute scale\: pure\-O3 pressure measurements \(above\) in the Huggins and Chappuis bands; the Hartley band, the 350\-450 nm minimum and the Wulf band are relative, scaled to the absolute spectra in the overlaps \(pp\. 611\-612, 621\)\. Not normalised to any other data set\. \- Uncertainty \(Table 2, image checked, p\. 615; 'upper estimations' for the absolute measurements at 50 mbar, 293 K\)\: systematic 1\.3 % \(pressure sensor 0\.5 %, temperature sensor 0\.3 %, temperature non\-uniformity 0\.3 %, leaks 0\.1 %, cell length 0\.04\-0\.07 %, O2 impurity 0\.005 %\); statistical \(RMS\) 1\-3 % \(ozone decay 1 %, light\-source stability 0\.28\-2\.8 % at OD 1, pressure 0\.08 %, temperature 0\.1 %\)\. 'The absolute accuracy is better than three percent for most parts of the spectral region' \(abstract\); 'uncertainty of our dataset \(2\-3 % for most of the spectral regions\)' \(p\. 614\); in weak absorption the statistical uncertainty 'can reach up to 20 % or more' \(p\. 614\); 'greater than 30 %' near 385 nm and at 1020 nm \(p\. 619\); 'about 30 % or more' around 1000 nm \(p\. 621\)\. Levels not stated\. \- The published file\: 'made available from the website of the molecular spectroscopy laboratory of the Institute of the Environmental Physics, University of Bremen' \(p\. 622\), with technical documentation\. Band\-integrated cross sections \(Table 3, image checked, p\. 617; cm^2 molecule^\-1 nm, 293\-298 K; Orphal's limits\)\: Hartley 245\-340 nm \(x 10^\-16\) Orphal 3\.55 \+\- 0\.6 %, this work 3\.53, Brion 3\.52, Burrows 3\.57, Bogumil 3\.56; Huggins 325\-340 nm \(x 10^\-20\) 8\.30 \+\- 0\.7 %, 8\.29, 8\.30, 8\.33, 8\.31; Chappuis 410\-690 nm \(x 10^\-19\) 6\.38 \+\- 1\.6 %, 6\.22, 6\.29, 6\.45, 6\.40; Wulf 633\-1000 nm \(x 10^\-19\) this work 1\.04, Bogumil 1\.10\. Not extracted\: no vocabulary quantity for a cross section integrated over wavelength \(format need\)\. The Wulf limits are printed 633\-1000 nm in Table 3 but '663\-1000 nm \(Banichevich et al\., 1993\)' in the text \(p\. 616\)\. Comparisons \(pp\. 616\-621\)\: agreement with BMD about 1 % and better; within 1 % of all datasets in the Hartley and Huggins bands, 1\-4 % in the Chappuis and 6 % in the Wulf band \(integrated\); several per cent below the satellite sets and BP near 255 nm; in 323\-340 nm lower by 2\-3 % than BMD and 2\-7 % than BP; wavelength shifts\: BP\_exp \+0\.026 \+\- 0\.002 nm, BP\_calc \+0\.023, BP\_HITRAN \+0\.008, Voigt \+0\.005, Bogumil \+0\.006 nm; a non\-linear BMD calibration \(different shifts in 323\-330 and 332\-340 nm\)\. The MPI \(Mainz\) BP and BMD data are on AIR wavelengths \(p\. 617\)\. Datasets\: Tables 4\-7 \(images checked\), one per source column; 'This work' at 293 K is a set of points of the data file\: 'check'\. The other columns are other data sets evaluated by these authors at vacuum wavelengths \('in some cases data were interpolated', p\. 620\)\: reproduced\. Captions\: Tables 4, 6 and 7 'at 295 \+\- 3 K'; Table 5 the same with typical FWHM in brackets\. Attribution check\: Table 6's 'Anderson and Mauersberger \(1992\)' column \(3\.075, 4\.569, 5\.125, 4\.633, 3\.383\) is brion\_1998's, which supports brion\_1998 against burrows\_1999's Table 2 labels \(see burrows\_1999\)\. **Recorded bibliographic identity status:** VALIDATED. This concerns identification of the source; it does not establish the scientific correctness of its contents. Datasets -------- gorshelev\_2014/this\_work\_uv ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "this_work_uv", "material": "O3", "file": "O3/gorshelev_2014__this_work_uv.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "check", "uncertainty": { "relative": 0.03, "level": "not stated" }, "parameters": { "temperature_k": 293.0 } } Table 4 'This work'\: 7 UV wavelengths \(vacuum\), 293 K\. 2\-3 % \(source notes\)\. Row 248\.32 printed a factor 10 low \(erratum\)\. gorshelev\_2014/this\_work\_380 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "this_work_380", "material": "O3", "file": "O3/gorshelev_2014__this_work_380.csv", "table": "tbl_8eb4cf894101", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-23, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "check", "uncertainty": { "relative": 0.2, "level": "not stated" }, "parameters": { "temperature_k": 293.0 } } Table 5 'This work'\: 365, 405, 455 nm \(vacuum\), FWHM 0\.02 nm, 293 K\. In the absorption minimum the statistical uncertainty 'can reach up to 20 % or more' \(p\. 614\)\: 20 % used\. gorshelev\_2014/this\_work\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "this_work_vis", "material": "O3", "file": "O3/gorshelev_2014__this_work_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "check", "uncertainty": { "relative": 0.03, "level": "not stated" }, "parameters": { "temperature_k": 293.0 } } Table 6 'This work'\: 6 visible wavelengths \(vacuum\), 293 K\. 2\-3 % \(source notes\)\. gorshelev\_2014/this\_work\_nir ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "this_work_nir", "material": "O3", "file": "O3/gorshelev_2014__this_work_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "check", "uncertainty": { "relative": 0.03, "level": "not stated", "relative_rows": { "991.841": 0.3, "1046.766": 0.3 } }, "parameters": { "temperature_k": 293.0 } } Table 7 'This work'\: 16 NIR wavelengths \(vacuum\), 293 K\. 2\-3 % below 950 nm; 'about 30 % or more' around 1000 nm \(p\. 621\)\: 30 % for 991\.841 and 1046\.766 nm\. gorshelev\_2014/orphal\_2003\_uv ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "orphal_2003_uv", "material": "O3", "file": "O3/gorshelev_2014__orphal_2003_uv.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Orphal, J.: A critical review of the absorption cross-sections of O3 and NO2 in the ultraviolet and visible, J. Photoch. Photobiol. A, 157, 185-209, 2003" ] } Table 4 'Orphal \(2003\)'\: mean values over several data sets; the printed \+\- % \(the standard deviation of the averaging\) stays in 'printed'\. gorshelev\_2014/orphal\_2003\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "orphal_2003_vis", "material": "O3", "file": "O3/gorshelev_2014__orphal_2003_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Orphal, J.: A critical review of the absorption cross-sections of O3 and NO2 in the ultraviolet and visible, J. Photoch. Photobiol. A, 157, 185-209, 2003" ] } Table 6 'Orphal \(2003\)'\: mean values; the printed \+\- % stays in 'printed'\. gorshelev\_2014/hearn\_1961\_uv ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "hearn_1961_uv", "material": "O3", "file": "O3/gorshelev_2014__hearn_1961_uv.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Hearn, A. G.: The absorption of ozone in the ultra-violet and visible regions of the spectrum, P. Phys. Soc., 78, 932-940, 1961" ] } Table 4 'Hearn \(1961\)' at four Hg lines \(vacuum wavelengths here\)\. gorshelev\_2014/bmd\_uv ~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bmd_uv", "material": "O3", "file": "O3/gorshelev_2014__bmd_uv.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "daumont_1992" ], "parameters": { "temperature_k": 295.0 } } Table 4 'BMD \(1998\)'\: the Brion/Daumont/Malicet data evaluated at vacuum wavelengths \(295 K in the UV\: daumont\_1992's measurement; matches daumont\_1992's Table III to the rounding\: 1131, 151, 61\.5, 29\.8\)\. Row 248\.32 printed a factor 10 low \(erratum\)\. gorshelev\_2014/bmd\_380 ~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bmd_380", "material": "O3", "file": "O3/gorshelev_2014__bmd_380.csv", "table": "tbl_8eb4cf894101", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-23, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "brion_1998" ], "parameters": { "temperature_k": 295.0 } } Table 5 'BMD \(1998\)' \(FWHM 0\.02 nm\), from the brion\_1998 data\. gorshelev\_2014/bmd\_vis ~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bmd_vis", "material": "O3", "file": "O3/gorshelev_2014__bmd_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "brion_1998" ], "parameters": { "temperature_k": 295.0 } } Table 6 'BMD \(1998\)'\: matches brion\_1998's Table II to the rounding\. gorshelev\_2014/bmd\_nir ~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bmd_nir", "material": "O3", "file": "O3/gorshelev_2014__bmd_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "brion_1998" ], "parameters": { "temperature_k": 295.0 } } Table 7 'BMD \(1998\)', 8 wavelengths to 817 nm, from the brion\_1998 data\. gorshelev\_2014/burrows\_1999\_uv ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burrows_1999_uv", "material": "O3", "file": "O3/gorshelev_2014__burrows_1999_uv.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "burrows_1999" ], "parameters": { "temperature_k": 293.0 } } 'Burrows et al\. \(1999a\)', the GOME FM data at 293 K\: Table 4; 1150 at 253\.73 nm is burrows\_1999's Table 1 value\. Row 248\.32 printed a factor 10 low \(erratum\)\. gorshelev\_2014/burrows\_1999\_380 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burrows_1999_380", "material": "O3", "file": "O3/gorshelev_2014__burrows_1999_380.csv", "table": "tbl_8eb4cf894101", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-23, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "burrows_1999" ], "parameters": { "temperature_k": 293.0 } } 'Burrows et al\. \(1999a\)', the GOME FM data at 293 K\: Table 5 \(FWHM 0\.17\-0\.29 nm\)\. gorshelev\_2014/burrows\_1999\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burrows_1999_vis", "material": "O3", "file": "O3/gorshelev_2014__burrows_1999_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "burrows_1999" ], "parameters": { "temperature_k": 293.0 } } 'Burrows et al\. \(1999a\)', the GOME FM data at 293 K\: Table 6 \(3\.17, 4\.76, 4\.69, 3\.51 against burrows\_1999's Table 2 3167, 4756, 4700, 3505 x 10^\-24\: 612\.14 nm differs by 0\.2 %\)\. gorshelev\_2014/burrows\_1999\_nir ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burrows_1999_nir", "material": "O3", "file": "O3/gorshelev_2014__burrows_1999_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "burrows_1999" ], "parameters": { "temperature_k": 293.0 } } 'Burrows et al\. \(1999a\)', the GOME FM data at 293 K\: Table 7, 748\-779 nm\. gorshelev\_2014/bogumil\_2003\_uv ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bogumil_2003_uv", "material": "O3", "file": "O3/gorshelev_2014__bogumil_2003_uv.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Bogumil, K., Orphal, J., Homann, T., Voigt, S., Spietz, P., Fleischmann, O. C., Vogel, A., Hartmann, M., Bovensmann, H., Frerick, J., and Burrows, J. P.: Measurements of molecular absorption spectra with the SCIAMACHY pre-flight model: instrument characterization and reference data for atmospheric remote-sensing in the 230-2380 nm region, J. Photoch. Photobiol. A., 157, 157-167, 2003" ], "parameters": { "temperature_k": 293.0 } } 'Bogumil et al\. \(2003\)', the SCIAMACHY pre\-flight\-model data at 293 K \(p\. 618\), scaled to Bass and Paur \(at least 2 % systematic, p\. 614\)\: Table 4\. Row 248\.32 printed a factor 10 low \(erratum\)\. gorshelev\_2014/bogumil\_2003\_380 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bogumil_2003_380", "material": "O3", "file": "O3/gorshelev_2014__bogumil_2003_380.csv", "table": "tbl_8eb4cf894101", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-23, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Bogumil, K., Orphal, J., Homann, T., Voigt, S., Spietz, P., Fleischmann, O. C., Vogel, A., Hartmann, M., Bovensmann, H., Frerick, J., and Burrows, J. P.: Measurements of molecular absorption spectra with the SCIAMACHY pre-flight model: instrument characterization and reference data for atmospheric remote-sensing in the 230-2380 nm region, J. Photoch. Photobiol. A., 157, 157-167, 2003" ], "parameters": { "temperature_k": 293.0 } } 'Bogumil et al\. \(2003\)', the SCIAMACHY pre\-flight\-model data at 293 K \(p\. 618\), scaled to Bass and Paur \(at least 2 % systematic, p\. 614\)\: Table 5 \(FWHM 0\.21\-0\.52 nm\)\. gorshelev\_2014/bogumil\_2003\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bogumil_2003_vis", "material": "O3", "file": "O3/gorshelev_2014__bogumil_2003_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Bogumil, K., Orphal, J., Homann, T., Voigt, S., Spietz, P., Fleischmann, O. C., Vogel, A., Hartmann, M., Bovensmann, H., Frerick, J., and Burrows, J. P.: Measurements of molecular absorption spectra with the SCIAMACHY pre-flight model: instrument characterization and reference data for atmospheric remote-sensing in the 230-2380 nm region, J. Photoch. Photobiol. A., 157, 157-167, 2003" ], "parameters": { "temperature_k": 293.0 } } 'Bogumil et al\. \(2003\)', the SCIAMACHY pre\-flight\-model data at 293 K \(p\. 618\), scaled to Bass and Paur \(at least 2 % systematic, p\. 614\)\: Table 6\. gorshelev\_2014/bogumil\_2003\_nir ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "bogumil_2003_nir", "material": "O3", "file": "O3/gorshelev_2014__bogumil_2003_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Bogumil, K., Orphal, J., Homann, T., Voigt, S., Spietz, P., Fleischmann, O. C., Vogel, A., Hartmann, M., Bovensmann, H., Frerick, J., and Burrows, J. P.: Measurements of molecular absorption spectra with the SCIAMACHY pre-flight model: instrument characterization and reference data for atmospheric remote-sensing in the 230-2380 nm region, J. Photoch. Photobiol. A., 157, 157-167, 2003" ], "parameters": { "temperature_k": 293.0 } } 'Bogumil et al\. \(2003\)', the SCIAMACHY pre\-flight\-model data at 293 K \(p\. 618\), scaled to Bass and Paur \(at least 2 % systematic, p\. 614\)\: Table 7, 16 wavelengths\. gorshelev\_2014/petersen\_2012\_hearn ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "petersen_2012_hearn", "material": "O3", "file": "O3/gorshelev_2014__petersen_2012_hearn.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Petersen, M., Viallon, J., Moussay, P., and Wielgosz, R. I.: Relative measurements of ozone absorption cross-sections at three wavelengths in the Hartley band using a well-defined UV laser beam, J. Geophys. Res., 117, D05301, 2012" ] } Table 4 'Petersen et al\. \(2012\) using Hearn/BMD value', first value\: relative measurements at three laser wavelengths \(0\.085 % relative\) scaled with Hearn's 253\.65 nm value \(p\. 616\)\. Row 248\.32 printed a factor 10 low \(erratum\)\. gorshelev\_2014/petersen\_2012\_bmd ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "petersen_2012_bmd", "material": "O3", "file": "O3/gorshelev_2014__petersen_2012_bmd.csv", "table": "tbl_102450bc135d", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-20, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Petersen, M., Viallon, J., Moussay, P., and Wielgosz, R. I.: Relative measurements of ozone absorption cross-sections at three wavelengths in the Hartley band using a well-defined UV laser beam, J. Geophys. Res., 117, D05301, 2012" ] } Table 4 'Petersen et al\. \(2012\) using Hearn/BMD value', second value\: the same measurements scaled with BMD's 253\.65 nm value\. Row 248\.32 printed a factor 10 low \(erratum\)\. gorshelev\_2014/burkholder\_talukdar\_1994\_380 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burkholder_talukdar_1994_380", "material": "O3", "file": "O3/gorshelev_2014__burkholder_talukdar_1994_380.csv", "table": "tbl_8eb4cf894101", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-23, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Burkholder, J. B. and Talukdar, R. K.: Temperature dependence of the ozone absorption spectrum over the wavelength range 410-760 nm, Geophys. Res. Lett., 21, 581-584, 1994" ] } Table 5 'Burkholder and Talukdar \(1994\)'\: 455 nm only\. gorshelev\_2014/burkholder\_talukdar\_1994\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burkholder_talukdar_1994_vis", "material": "O3", "file": "O3/gorshelev_2014__burkholder_talukdar_1994_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Burkholder, J. B. and Talukdar, R. K.: Temperature dependence of the ozone absorption spectrum over the wavelength range 410-760 nm, Geophys. Res. Lett., 21, 581-584, 1994" ] } Table 6 'Burkholder and Talukdar \(1994\)', scaled to Anderson and Mauersberger \(1992\) \(p\. 620\)\. gorshelev\_2014/burkholder\_talukdar\_1994\_nir ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "burkholder_talukdar_1994_nir", "material": "O3", "file": "O3/gorshelev_2014__burkholder_talukdar_1994_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Burkholder, J. B. and Talukdar, R. K.: Temperature dependence of the ozone absorption spectrum over the wavelength range 410-760 nm, Geophys. Res. Lett., 21, 581-584, 1994" ] } Table 7 'Burkholder and Talukdar \(1994\)', 748\-760 nm\. gorshelev\_2014/axson\_2011\_380 ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "axson_2011_380", "material": "O3", "file": "O3/gorshelev_2014__axson_2011_380.csv", "table": "tbl_8eb4cf894101", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-23, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Axson, J. L., Washenfelder, R. A., Kahan, T. F., Young, C. J., Vaida, V., and Brown, S. S.: Absolute ozone absorption cross section in the Huggins Chappuis minimum (350-470 nm) at 296 K, Atmos. Chem. Phys., 11, 11581-11590, 2011" ], "parameters": { "temperature_k": 296.0 } } Table 5 'Axson et al\. \(2011\)' \(FWHM 0\.27\-0\.5 nm\)\: cavity\-enhanced relative measurements scaled to Orphal's 253\.65 nm value, 4\-30 % \(p\. 619\); 296 K per the cited title\. gorshelev\_2014/anderson\_mauersberger\_1992\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "anderson_mauersberger_1992_vis", "material": "O3", "file": "O3/gorshelev_2014__anderson_mauersberger_1992_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Anderson, S. M. and Mauersberger, K.: Laser measurements of ozone absorption cross-sections in the Chappuis band, Geophys. Res. Lett., 19, 933-936, 1992" ] } Table 6 'Anderson and Mauersberger \(1992\)'\: laser measurements with pure O3, overall uncertainty below 1 % \(p\. 620\); the same values as brion\_1998's column of that name\. gorshelev\_2014/anderson\_1993\_nir ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "anderson_1993_nir", "material": "O3", "file": "O3/gorshelev_2014__anderson_1993_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "Anderson, S. M., Hupalo, P., and Mauersberger, K.: Ozone absorption cross-section measurements in the Wulf bands, Geophys. Res. Lett., 20, 1579-1582, 1993" ] } Table 7 'Anderson et al\. \(1993\)'\: the Wulf band, scaled to Anderson and Mauersberger \(1992\) \(p\. 620\)\. gorshelev\_2014/el\_helou\_2005\_vis ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "el_helou_2005_vis", "material": "O3", "file": "O3/gorshelev_2014__el_helou_2005_vis.csv", "table": "tbl_a995b8119c7a", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-21, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "El Helou, Z., Churassy, S., Wannous, G., Bacis, R., and Boursey, E.: Absolute cross sections of ozone at atmospheric temperatures for the Wulf and the Chappuis bands, J. Chem. Phys., 122, 244311, 2005" ] } Table 6 'El Helou et al\. \(2005\)'\: FTS with pure O3, 0\.82 % \(p\. 620\)\. gorshelev\_2014/el\_helou\_2005\_nir ~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ .. code-block:: text { "id": "el_helou_2005_nir", "material": "O3", "file": "O3/gorshelev_2014__el_helou_2005_nir.csv", "table": "tbl_6fa5f0d2dae8", "quantity": "absorption_cross_section", "unit": "cm2", "scale": 1e-22, "abscissa_unit": "nm", "wavelength_medium": "vacuum", "use": "reproduced", "reproduced_from": [ "El Helou, Z., Churassy, S., Wannous, G., Bacis, R., and Boursey, E.: Absolute cross sections of ozone at atmospheric temperatures for the Wulf and the Chappuis bands, J. Chem. Phys., 122, 244311, 2005" ] } Table 7 'El Helou et al\. \(2005\)'\. Formulas -------- No formulas are recorded. Corrections ----------- .. code-block:: text [ { "dataset": "this_work_uv", "row": "248.32", "column": "value", "printed": "105.1", "corrected": "1051", "reason": "Table 4's row 248.32 nm is printed a factor of ten low in every column (105.1, 103.8, 106.3, 106.3, 106.1/104.5 x 10^-20 cm^2), between 946-965 at 244.06 nm and 1107-1129 at 257.34 nm.", "evidence": "Table image checked: the row is printed so. The Hartley band rises smoothly from 244 nm to its maximum near 254 nm (1120-1150 at 253.73 nm in the same table) and a cross section of about 1.05e-19 cm^2 lies near 290 nm (151 at 289.44 nm), far from 248 nm; ten times the printed values (1038-1063) lies between the neighbouring rows for all six values at once. To confirm against the data file (TC-188)." }, { "dataset": "bmd_uv", "row": "248.32", "column": "value", "printed": "103.8", "corrected": "1038", "reason": "Table 4's row 248.32 nm is printed a factor of ten low in every column (105.1, 103.8, 106.3, 106.3, 106.1/104.5 x 10^-20 cm^2), between 946-965 at 244.06 nm and 1107-1129 at 257.34 nm.", "evidence": "Table image checked: the row is printed so. The Hartley band rises smoothly from 244 nm to its maximum near 254 nm (1120-1150 at 253.73 nm in the same table) and a cross section of about 1.05e-19 cm^2 lies near 290 nm (151 at 289.44 nm), far from 248 nm; ten times the printed values (1038-1063) lies between the neighbouring rows for all six values at once. To confirm against the data file (TC-188)." }, { "dataset": "burrows_1999_uv", "row": "248.32", "column": "value", "printed": "106.3", "corrected": "1063", "reason": "Table 4's row 248.32 nm is printed a factor of ten low in every column (105.1, 103.8, 106.3, 106.3, 106.1/104.5 x 10^-20 cm^2), between 946-965 at 244.06 nm and 1107-1129 at 257.34 nm.", "evidence": "Table image checked: the row is printed so. The Hartley band rises smoothly from 244 nm to its maximum near 254 nm (1120-1150 at 253.73 nm in the same table) and a cross section of about 1.05e-19 cm^2 lies near 290 nm (151 at 289.44 nm), far from 248 nm; ten times the printed values (1038-1063) lies between the neighbouring rows for all six values at once. To confirm against the data file (TC-188)." }, { "dataset": "bogumil_2003_uv", "row": "248.32", "column": "value", "printed": "106.3", "corrected": "1063", "reason": "Table 4's row 248.32 nm is printed a factor of ten low in every column (105.1, 103.8, 106.3, 106.3, 106.1/104.5 x 10^-20 cm^2), between 946-965 at 244.06 nm and 1107-1129 at 257.34 nm.", "evidence": "Table image checked: the row is printed so. The Hartley band rises smoothly from 244 nm to its maximum near 254 nm (1120-1150 at 253.73 nm in the same table) and a cross section of about 1.05e-19 cm^2 lies near 290 nm (151 at 289.44 nm), far from 248 nm; ten times the printed values (1038-1063) lies between the neighbouring rows for all six values at once. To confirm against the data file (TC-188)." }, { "dataset": "petersen_2012_hearn", "row": "248.32", "column": "value", "printed": "106.1", "corrected": "1061", "reason": "Table 4's row 248.32 nm is printed a factor of ten low in every column (105.1, 103.8, 106.3, 106.3, 106.1/104.5 x 10^-20 cm^2), between 946-965 at 244.06 nm and 1107-1129 at 257.34 nm.", "evidence": "Table image checked: the row is printed so. The Hartley band rises smoothly from 244 nm to its maximum near 254 nm (1120-1150 at 253.73 nm in the same table) and a cross section of about 1.05e-19 cm^2 lies near 290 nm (151 at 289.44 nm), far from 248 nm; ten times the printed values (1038-1063) lies between the neighbouring rows for all six values at once. To confirm against the data file (TC-188)." }, { "dataset": "petersen_2012_bmd", "row": "248.32", "column": "value", "printed": "104.5", "corrected": "1045", "reason": "Table 4's row 248.32 nm is printed a factor of ten low in every column (105.1, 103.8, 106.3, 106.3, 106.1/104.5 x 10^-20 cm^2), between 946-965 at 244.06 nm and 1107-1129 at 257.34 nm.", "evidence": "Table image checked: the row is printed so. The Hartley band rises smoothly from 244 nm to its maximum near 254 nm (1120-1150 at 253.73 nm in the same table) and a cross section of about 1.05e-19 cm^2 lies near 290 nm (151 at 289.44 nm), far from 248 nm; ten times the printed values (1038-1063) lies between the neighbouring rows for all six values at once. To confirm against the data file (TC-188)." } ] Formula corrections, where recorded, appear with their formulas above. Curation notes may also discuss corrections or unresolved interpretation. Consult the :doc:`review register ` for the checks and decisions.