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Ultraviolet photoabsorption in the B 3Σ- − X 3Σ- and C 3Π − X 3Σ- band systems of SO sulphur isotopologues

dc.contributor.authorHeays, A. N.
dc.contributor.authorStark, Glenn
dc.contributor.authorLyons, J. R.
dc.contributor.authorDe Oliveira, N.
dc.contributor.authorLewis, Brenton
dc.contributor.authorGibson, Stephen
dc.date.accessioned2026-01-15T00:05:22Z
dc.date.available2026-01-15T00:05:22Z
dc.date.issued2023
dc.date.updated2023-10-22T07:16:51Z
dc.description.abstractHigh-resolution far-ultraviolet broadband Fourier-transform photoabsorption spectra of 32S16O, 33S16O, 34S16O, and 36S16O are recorded in a microwave discharge seeded with SO2. The (Formula presented.) and (Formula presented.) bands are observed or inferred in the (Formula presented.) –51,000 cm−1 (196 to 233 nm) spectral range. This is the first experimental detection of a (Formula presented.) level and of any of these observed bands in an S-substituted isotopologue. Additional measurements of (Formula presented.) provide a calibration of the SO column density. Measured band profiles are fitted to an effective-Hamiltonian model of coupled excited B 3Σ− and C 3Π states along with their predissociation linewidths and absorption band strengths. Electronic-state potential-energy curves and transition moments are deduced. The end result is a list of line frequencies, f-values, and dissociation widths describing the far-ultraviolet photodissociation spectrum of SO that is accurate enough for computing atmospheric photolytic isotope-fractionation. Linelists, and photoabsorption and photodissociation cross sections are available as supplementary data.
dc.description.sponsorshipAH was funded by the NASA Postdoctoral Program through the NASA Astrobiology Institute, by grant number 19-03314S of the Czech Science Foundation, and the European Regional Development Fund (ERDF/ESF) \u2018Centre of Advanced Applied Sciences\u2019 [grant number CZ.02.1. 01/0.0/0.0/16_019/0000778]. JRL acknowledges support from the NASA Exobiology program [grant #80NSSC19K0475 to Arizona State University].
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.citationA. N. Heays, G. Stark, J. R. Lyons, N. de Oliveira, B. R. Lewis & S. T. Gibson (2023) Ultraviolet photoabsorption in the B3Σ- − X3Σ- and C3Π − X3Σ- band systems of SO sulphur isotopologues, Molecular Physics, 121:17-18, e2153092, DOI: 10.1080/00268976.2022.2153092
dc.identifier.issn0026-8976
dc.identifier.urihttps://hdl.handle.net/1885/733804259
dc.language.isoen_AUen_AU
dc.publisherTaylor & Francis Group
dc.rights© 2022 Informa UK Limited, trading as Taylor & Francis Group
dc.sourceMolecular Physics
dc.titleUltraviolet photoabsorption in the B 3Σ- − X 3Σ- and C 3Π − X 3Σ- band systems of SO sulphur isotopologues
dc.typeJournal article
local.bibliographicCitation.issue17-18
local.contributor.affiliationHeays, A. N., Arizona State University
local.contributor.affiliationStark, Glenn, Wellesley College
local.contributor.affiliationLyons, J. R., Arizona State University
local.contributor.affiliationDe Oliveira, N., Synchrotron SOLEIL
local.contributor.affiliationLewis, Brenton, College of Science, ANU
local.contributor.affiliationGibson, Stephen, College of Science, ANU
local.contributor.authoruidLewis, Brenton, u7901135
local.contributor.authoruidGibson, Stephen, u8601433
local.description.embargo2099-12-31
local.description.notesImported from ARIES
local.identifier.absfor510201 - Atomic and molecular physics
local.identifier.ariespublicationa383154xPUB38352
local.identifier.citationvolume121
local.identifier.doi10.1080/00268976.2022.2153092
local.identifier.scopusID2-s2.0-85144110862
local.type.statusPublished Version
publicationvolume.volumeNumber121

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