FN Archimer Export Format PT J TI Comparison and validation of physical wave parameterizations in spectral wave models BT AF STOPA, Justin ARDHUIN, Fabrice BABANIN, Alexander ZIEGER, Stefan AS 1:1;2:1,2,4;3:3;4:3; FF 1:PDG-ODE-LOPS-SIAM;2:;3:;4:; C1 IFREMER, LOS, Plouzane, France. IFREMER, LPO, Plouzane, France. Swinburne Univ Technol, Ctr Ocean Engn Sci & Technol, Hawthorn, Vic 3122, Australia. C2 IFREMER, FRANCE IFREMER, FRANCE UNIV TECHNOL SWINBURNE, AUSTRALIA CNRS, FRANCE SI BREST SE PDG-ODE-LOPS-SIAM UM LOPS IN WOS Ifremer jusqu'en 2018 copubli-france copubli-int-hors-europe IF 3.341 TC 119 UR https://archimer.ifremer.fr/doc/00280/39122/38300.pdf LA English DT Article DE ;WAVEWATCH III;Spectral wave modeling;Wave hindcasting;Source terms;Higher order wave moments;Swell dissipation AB Recent developments in the physical parameterizations available in spectral wave models have already been validated, but there is little information on their relative performance especially with focus on the higher order spectral moments and wave partitions. This study concentrates on documenting their strengths and limitations using satellite measurements, buoy spectra, and a comparison between the different models. It is confirmed that all models perform well in terms of significant wave heights; however higher-order moments have larger errors. The partition wave quantities perform well in terms of direction and frequency but the magnitude and directional spread typically have larger discrepancies. The high-frequency tail is examined through the mean square slope using satellites and buoys. From this analysis it is clear that some models behave better than the others, suggesting their parameterizations match the physical processes reasonably well. However none of the models are entirely satisfactory, pointing to poorly constrained parameterizations or missing physical processes. The major space-time differences between the models are related to the swell field stressing the importance of describing its evolution. An example swell field confirms the wave heights can be notably different between model configurations while the directional distributions remain similar. It is clear that all models have difficulty in describing the directional spread. Therefore, knowledge of the source term directional distributions is paramount in improving the wave model physics in the future. PY 2016 PD JUN SO Ocean Modelling SN 1463-5003 PU Elsevier Sci Ltd VL 103 UT 000377391800002 BP 2 EP 17 DI 10.1016/j.ocemod.2015.09.003 ID 39122 ER EF