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Chromophoric signatures of microbial by‐products in the dark ocean
Author(s) -
Catalá Teresa S.,
Reche Isabel,
Ramón Cintia L.,
LópezSanz Àngel,
Álvarez Marta,
Calvo Eva,
ÁlvarezSalgado Xosé A.
Publication year - 2016
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2016gl069878
Subject(s) - chromophore , absorption (acoustics) , spectral line , absorption spectroscopy , analytical chemistry (journal) , nitrate , visible spectrum , spectral slope , chemistry , photochemistry , physics , environmental chemistry , optics , organic chemistry , astronomy
Detailed examination of the absorption spectra from dark ocean samples allowed us to identify and deconvolve two distinct chromophores centered at 302 nm (UV) and 415 nm (visible) from the exponential decay curve characteristic of humic substances. The UV chromophore was ubiquitous in intermediate and deep waters, and it has been proposed as the secondary absorption peak of nitrate. The visible chromophore was prominent at the central and intermediate water masses of the North Pacific, and it has been proposed as cytochrome c. Subtraction of the modeled absorption spectra of the two chromophores from the measured absorption spectrum of the samples leads to a spectral slope overestimation by 13.3 ± 6.0% for S 275–295 and 14.8 ± 10.6% for S 350–400 . To only consider the chromophoric fraction of DOM, the absorption spectra of nitrate should be subtracted in samples with a [NO 3− ]: a 302 ratio > 70 µ M  m.

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