A posteriori calculation of δ<sup>18</sup>O and δD in atmospheric water vapour from ground-based near-infrared FTIR retrievals of H<sub>2</sub><sup>16</sup>O, H<sub>2</sub><sup>18</sup>O, and HD<sup>16</sup>O

This paper investigates the scientific value of retrieving H<sub>2</sub><sup>18</sup>O and HDO columns in addition to H<sub>2</sub><sup>16</sup>O columns from high-resolution ground-based near-infrared spectra. We present a set of refined H<sub>2...

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Bibliographic Details
Main Authors: N. V. Rokotyan, V. I. Zakharov, K. G. Gribanov, M. Schneider, F.-M. Bréon, J. Jouzel, R. Imasu, M. Werner, M. Butzin, C. Petri, T. Warneke, J. Notholt
Format: Article
Language:English
Published: Copernicus Publications 2014-08-01
Series:Atmospheric Measurement Techniques
Online Access:http://www.atmos-meas-tech.net/7/2567/2014/amt-7-2567-2014.pdf
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Summary:This paper investigates the scientific value of retrieving H<sub>2</sub><sup>18</sup>O and HDO columns in addition to H<sub>2</sub><sup>16</sup>O columns from high-resolution ground-based near-infrared spectra. We present a set of refined H<sub>2</sub><sup>16</sup>O, H<sub>2</sub><sup>18</sup>O, and HDO spectral windows. The retrieved H<sub>2</sub><sup>16</sup>O, H<sub>2</sub><sup>18</sup>O, and HDO columns are used for an a posteriori calculation of columnar δD and δ<sup>18</sup>O. We estimate the uncertainties for the so-calculated columnar δD and δ<sup>18</sup>O values. These estimations include uncertainties due to the measurement noise, errors in the a priori data, and uncertainties in spectroscopic parameters. Time series of δ<sup>18</sup>O obtained from ground-based FTIR (Fourier transform infrared) spectra are presented for the first time. <br><br> For our study we use a full physics isotopic general circulation model (ECHAM5-wiso). We show that the full physics simulation of HDO and H<sub>2</sub><sup>18</sup>O can already be reasonably predicted from the H<sub>2</sub><sup>16</sup>O columns by a simple linear regression model (scatter values between full physics and linear regression simulations are 35 and 4&permil; for HDO and H<sub>2</sub><sup>18</sup>O, respectively). We document that the columnar δD and δ<sup>18</sup>O values as calculated a posteriori from the retrievals of H<sub>2</sub><sup>16</sup>O, H<sub>2</sub><sup>18</sup>O, and HDO show a better agreement with the ECHAM5-wiso simulation than the δD and δ<sup>18</sup>O values as calculated from the H<sub>2</sub><sup>16</sup>O retrievals and the simple linear regression model. This suggests that the H<sub>2</sub><sup>18</sup>O and HDO column retrievals add complementary information to the H<sub>2</sub><sup>16</sup>O retrievals. However, these data have to be used carefully, because of the different vertical sensitivity of the H<sub>2</sub><sup>16</sup>O, H<sub>2</sub><sup>18</sup>O, and HDO columnar retrievals. Furthermore, we have to note that the retrievals use reanalysis humidity profiles as a priori input and the results are thus not independent of the reanalysis data.
ISSN:1867-1381
1867-8548