Diel variation in the vertical distribution of particulate matter (> 0.15 mm) in the NW Mediterranean Sea investigated with the Underwater Video Profiler
L. Stemmann et al., Diel variation in the vertical distribution of particulate matter (> 0.15 mm) in the NW Mediterranean Sea investigated with the Underwater Video Profiler, DEEP-SEA I, 47(3), 2000, pp. 505-531
Citations number
51
Categorie Soggetti
Aquatic Sciences","Earth Sciences
Journal title
DEEP-SEA RESEARCH PART I-OCEANOGRAPHIC RESEARCH PAPERS
Day/night variations in the size distribution of the particulate matter > 0
.15 mm (PM) were studied in May 1995 during the DYNAPROC time-series cruise
in the northwestern Mediterranean Sea. Data on vertical distributions of P
M (>0.15 mm) and zooplankton were collected with the Underwater Video Profi
ler (UVP). The comparisons of the UVP data with plankton net data and POC d
ata from water bottles indicated that more than 97% of the particles detect
ed by the UVP were non-living particles (0.15 mm) and that the PM contribut
ed 4-34% of the total dry weight measured on GF/F filters. Comparison of se
ven pairs of day and night vertical profiles performed during the cruise sh
owed that in the upper 800 m, the mean size and the volume of particles was
higher at night than during the day. During the night, the integrated volu
me of the Ph I increased on average by 32 +/- 20%. This increase correspond
ed to a shift of smaller size classes ( < 0.5 mm) towards the larger ones (
> 0.5 mm). During the day, the pattern was reversed, and the quantity of PM
> 0.5 mm decreased. During the study period, the standing stock of PM (60-
800 m) decreased from 7.5 to less than 2gm(-2) but the diel variations pers
isted, except for two short periods in the superficial layer following a wi
nd event. The cyclic feeding activity induced by the diel vertical migratio
n of zooplankton could be the best candidate to explain the observed diel f
luctuations in the size classes of PM in the water column. However, our res
ults also suggest that in the upper layer additional driving forces such as
the increase of the level of turbulence after a wind event or the modifica
tion of the zoo- and phytoplankton community can influence the PM temporal
evolution. (C) 2000 Elsevier Science Ltd. All rights reserved.