

FOLLOWUS
1.Key Laboratory of Marine Ecology and Environmental Sciences, Institute of Oceanology, Chinese Academy of Sciences, Qingdao 266071, China
2.Laboratory for Marine Ecology and Environmental Science, Qingdao National Laboratory for Marine Science and Technology, Qingdao 266237, China
3.Center for Ocean Mega-Science, Chinese Academy of Sciences, Qingdao 266071, China
4.University of Chinese Academy of Sciences, Beijing 100049, China
5.Jiaozhou Bay Marine Ecosystem Research Station, Chinese Academy of Sciences, Qingdao 266071, China
SUN Song, sunsong@qdio.ac.cn
收稿:2019-04-26,
录用:2019-7-11,
网络首发:2020-09-30,
纸质出版:2020-11
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An enhanced underwater camera apparatus for seabed observation of megabenthic epifauna in the northern Yellow Sea[J]. 海洋湖沼学报(英文), 2020,38(6):1799-1810.
Nan YU, Song SUN, Shiwei WANG, et al. An enhanced underwater camera apparatus for seabed observation of megabenthic epifauna in the northern Yellow Sea[J]. Journal of Oceanology and Limnology, 2020, 38(6): 1799-1810.
An enhanced underwater camera apparatus for seabed observation of megabenthic epifauna in the northern Yellow Sea[J]. 海洋湖沼学报(英文), 2020,38(6):1799-1810. DOI: 10.1007/s00343-019-9122-9.
Nan YU, Song SUN, Shiwei WANG, et al. An enhanced underwater camera apparatus for seabed observation of megabenthic epifauna in the northern Yellow Sea[J]. Journal of Oceanology and Limnology, 2020, 38(6): 1799-1810. DOI: 10.1007/s00343-019-9122-9.
Seabed photographing has been applied with various underwater camera apparatuses (UCAs) for observations of megabenthic epifauna
which reveals more details than traditional sampling tools do. In this study
we improved a UCA named a towed underwater video-camera system (TUV system) with image processing software for seabed photographing in coastal areas up to 100 m. In May 2017
the TUV system was tested at 4 stations in the Zhangzi Island marine area in the northern Yellow Sea to investigate local megabenthic epifauna
especially brittle stars. At each station
more than 500 good seabed photographs each in area of 0.155 0 m
2
were obtained in just 10 min. Almost all of the epifauna larger than 1 mm could be identified from the photographs
including echinoderms
bivalves
cnidarians
and crustaceans. Three dominant brittle stars (
Ophiopholis mirabilis
Ophiura sarsii vadicola
and
Stegophiura sladeni
) were spotted
and their abundance
disc diameter
cluster size
and coverage area were calculated and analyzed from the seabed photographs. The results show that the TUV system could be applied in coastal waters of hard sandy bottoms and could be used for quantitative investigations of megabenthic epifauna.
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