FN Archimer Export Format PT J TI Quantifying Tidal Fluctuations in Remote Sensing Infrared SST Observations BT AF González-Haro, Cristina PONTE, Aurelien AUTRET, Emmanuelle AS 1:2;2:1;3:1; FF 1:;2:PDG-ODE-LOPS-OH;3:PDG-ODE-LOPS-SIAM; C1 Laboratoire d’Océanographie Physique et Spatiale (LOPS), IUEM, Univ. Brest, CNRS, IRD, Ifremer, 29238 Brest, France Laboratoire d’Océanographie Physique et Spatiale (LOPS), IUEM, Univ. Brest, CNRS, IRD, Ifremer, 29238 Brest, France C2 IFREMER, FRANCE CNRS, FRANCE SI BREST SE PDG-ODE-LOPS-OH PDG-ODE-LOPS-SIAM UM LOPS IN WOS Ifremer UMR WOS Cotutelle UMR DOAJ copubli-france IF 2.1 TC 3 UR https://archimer.ifremer.fr/doc/00589/70075/68048.pdf LA English DT Article DE ;sea surface temperature;satellite observations;tidal currents;internal tides AB The expected amplitude of fixed-point sea surface temperature (SST) fluctuations induced by barotropic and baroclinic tidal flows is estimated from tidal current atlases and SST observations. The fluctuations considered are the result of the advection of pre-existing SST fronts by tidal currents. They are thus confined to front locations and exhibit fine-scale spatial structures. The amplitude of these tidally induced SST fluctuations is proportional to the scalar product of SST frontal gradients and tidal currents. Regional and global estimations of these expected amplitudes are presented. We predict barotropic tidal motions produce SST fluctuations that may reach amplitudes of 0.3 K. Baroclinic (internal) tides produce SST fluctuations that may reach values that are weaker than 0.1 K. The amplitudes and the detectability of tidally induced fluctuations of SST are discussed in the light of expected SST fluctuations due to other geophysical processes and instrumental (pixel) noise. We conclude that actual observations of tidally induced SST fluctuations are a challenge with present-day observing systems. PY 2019 PD OCT SO Remote Sensing SN 2072-4292 PU MDPI AG VL 11 IS 19 UT 000496827100127 DI 10.3390/rs11192313 ID 70075 ER EF