Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90060-7
Ken O Buesseler , Michael P Bacon , J Kirk Cochran , Hugh D Livingston
The disequilibrium between the particle-reactive tracer 234Th ( days) and its soluble parent, 238U, was used to examine Th scavenging and export fluxes during the U.S. JGOFS North Atlantic Bloom Experiment (24 April–30 May 1989) at ∼47°N, 20°W. Four profiles of dissolved and particulate 234Th in the upper 300 m and a non-steady box model were used to quantify dissolved 234Th uptake and particle export rates. The highest export fluxes occured during the first half of May. From POC/234Th and PON/234Th ratios, particulate organic C and N fluxes were calculated. Results were 5–41 mmol C m−2 day−1 and 0.9–6.5 mmol N m−2 day−1 from the 0–35 m layer. The ratio of POC export flux to primary production ranged from 0.05 to 0.42, peaking in the first half of May. The estimated fluxes agree with the observed losses of total C and N from the upper ocean during the bloom, but yield significantly higher fluxes than were measured by floating traps at 150 and 300 m.
在美国JGOFS北大西洋水华实验(1989年4月24日至5月30日)期间,粒子反应性示踪剂234Th(t12=24.1天)与其可溶性母体238U之间的不平衡被用于检测Th清除和输出通量,温度为~47°N,20°W。使用上部300m溶解和颗粒234Th的四个剖面图和非稳态箱模型来量化溶解234Th吸收和颗粒输出率。从POC/234Th和PON/234Th比值计算了有机碳和氮的颗粒通量。0–35 m层的结果为5–41 mmol C m−2 d−1和0.9–6.5 mmol N m−2 day−1。POC出口通量与初级生产的比率在0.05至0.42之间,在5月上半月达到峰值。估计的通量与观测到的赤潮期间上层海洋总碳和氮的损失一致,但在150米和300米处产生的通量明显高于浮动捕集器测得的通量。
{"title":"Carbon and nitrogen export during the JGOFS North Atlantic Bloom experiment estimated from 234Th: 238U disequilibria","authors":"Ken O Buesseler , Michael P Bacon , J Kirk Cochran , Hugh D Livingston","doi":"10.1016/0198-0149(92)90060-7","DOIUrl":"https://doi.org/10.1016/0198-0149(92)90060-7","url":null,"abstract":"<div><p>The disequilibrium between the particle-reactive tracer <sup>234</sup>Th (<span><math><mtext>t</mtext><msub><mi></mi><mn><mtext>1</mtext><mtext>2</mtext></mn></msub><mtext> = 24.1</mtext></math></span> days) and its soluble parent, <sup>238</sup>U, was used to examine Th scavenging and export fluxes during the U.S. JGOFS North Atlantic Bloom Experiment (24 April–30 May 1989) at ∼47°N, 20°W. Four profiles of dissolved and particulate <sup>234</sup>Th in the upper 300 m and a non-steady box model were used to quantify dissolved <sup>234</sup>Th uptake and particle export rates. The highest export fluxes occured during the first half of May. From POC/<sup>234</sup>Th and PON/<sup>234</sup>Th ratios, particulate organic C and N fluxes were calculated. Results were 5–41 mmol C m<sup>−2</sup> day<sup>−1</sup> and 0.9–6.5 mmol N m<sup>−2</sup> day<sup>−1</sup> from the 0–35 m layer. The ratio of POC export flux to primary production ranged from 0.05 to 0.42, peaking in the first half of May. The estimated fluxes agree with the observed losses of total C and N from the upper ocean during the bloom, but yield significantly higher fluxes than were measured by floating traps at 150 and 300 m.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1115-1137"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90060-7","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72275705","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90065-2
Jorge E. Capella , Robin M. Ross , Langdon B. Quetin , Eileen E. Hofmann
Sixteen XBT sections were occupied from December 1982 to July 1987 in and around the Bransfield Strait and the South Shetland Islands. These and other temperature data from the FDRAKE75, FDRAKE76 and DRAKE79 field programs provide a description of the temperature structure and water mass distribution of the upper 500 m in this region. Temperature distributions at 300 and 500 m show Circumpolar Deep Water (>0°C) north of the South Shetland Islands, which enters Bransfield Strait through a gap between Smith and Snow Islands. Inside the Strait this water is confined to a narrow band along the southern flank of the Islands. The fine spatial resolution of the XBT sections shows a sharp thermal gradient between the cold (<0°C) Bransfield Strait waters and the warmer (>0°C) waters of Drake Passage origin. The presence of cold Bransfield Strait waters, over the northeast portion of the Island slope region, is related to north-south motions of this temperature boundary. The Polar Slope Current, on the northern side of the South Shetland Islands, appears as a tongue of cold (<0°C) water that extends westward from Elephant Island to the gap between Smith and Snow Islands.
{"title":"A note on the thermal structure of the upper ocean in the Bransfield Strait-South Shetland Islands region","authors":"Jorge E. Capella , Robin M. Ross , Langdon B. Quetin , Eileen E. Hofmann","doi":"10.1016/0198-0149(92)90065-2","DOIUrl":"10.1016/0198-0149(92)90065-2","url":null,"abstract":"<div><p>Sixteen XBT sections were occupied from December 1982 to July 1987 in and around the Bransfield Strait and the South Shetland Islands. These and other temperature data from the FDRAKE75, FDRAKE76 and DRAKE79 field programs provide a description of the temperature structure and water mass distribution of the upper 500 m in this region. Temperature distributions at 300 and 500 m show Circumpolar Deep Water (>0°C) north of the South Shetland Islands, which enters Bransfield Strait through a gap between Smith and Snow Islands. Inside the Strait this water is confined to a narrow band along the southern flank of the Islands. The fine spatial resolution of the XBT sections shows a sharp thermal gradient between the cold (<0°C) Bransfield Strait waters and the warmer (>0°C) waters of Drake Passage origin. The presence of cold Bransfield Strait waters, over the northeast portion of the Island slope region, is related to north-south motions of this temperature boundary. The Polar Slope Current, on the northern side of the South Shetland Islands, appears as a tongue of cold (<0°C) water that extends westward from Elephant Island to the gap between Smith and Snow Islands.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1221-1229"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90065-2","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"92832915","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90072-2
O.C. Zafiriou , L.A. Ball , Q. Hanley
We describe a modified (Garside, 1982, Marine Chemistry, 11, 159–167) nitrite method that permits measurements down to subnanomolar concentrations and present datafrom Atlantic and Carribean deepwater profiles for comparison with a published Pacific section.
This important intermediate in the nitrogen cycle was detected in all samples. Concentrations were consistently lowest (0.1–0.4 nM) in oligotrophic surface waters. Below 1 km, carribean and Southwest Sargasso sea nitrite concentrations were 0.4–1 nM, decreasing with increasing depth; reported Pacific [NO2] averages are several times higher. Profiles in the upper kilometer beneath the classical primary nitrate maximum (PNM) were qualitatively similar, exhibiting a smooth supra-exponential drop with depth to vvalues of ∼1–4 nM at 1 km.
Then nitrite inventory in this “tail” of the PNM above 1 km with 1 nM ≤[NO2]≤50 nM roughly equals that in the classical PNM. Significant differences among profiles in the 0.1–1 km regionn are observed, consistent with nitrite pool turnover of 3–7 days estimated from Redfield stoichiometry and tritium-helium ages. Thus seasonal and/or regional variations in factors altering the nitrite production-consumption balance, rather than transport, seem to be responsible for nitrite variability.
Nitrite profiles with anomalous midwater or near-bottom fine structure, including multi-point maxima and minima, were found along the Venezuelan continental margin and at ≈ 13°N. These featurers are tentatively ascribed to boundary effects, as hydrographic and circumstantial evidence suggests that these waters interacted previously with the bottom.
{"title":"Trace nitrate in oxic waters","authors":"O.C. Zafiriou , L.A. Ball , Q. Hanley","doi":"10.1016/0198-0149(92)90072-2","DOIUrl":"10.1016/0198-0149(92)90072-2","url":null,"abstract":"<div><p>We describe a modified (Garside, 1982, <em>Marine Chemistry</em>, <strong>11</strong>, 159–167) nitrite method that permits measurements down to subnanomolar concentrations and present datafrom Atlantic and Carribean deepwater profiles for comparison with a published Pacific section.</p><p>This important intermediate in the nitrogen cycle was detected in all samples. Concentrations were consistently lowest (0.1–0.4 nM) in oligotrophic surface waters. Below 1 km, carribean and Southwest Sargasso sea nitrite concentrations were 0.4–1 nM, decreasing with increasing depth; reported Pacific [NO<sub>2</sub>] averages are several times higher. Profiles in the upper kilometer beneath the classical primary nitrate maximum (PNM) were qualitatively similar, exhibiting a smooth supra-exponential drop with depth to vvalues of ∼1–4 nM at 1 km.</p><p>Then nitrite inventory in this “tail” of the PNM above 1 km with 1 nM ≤[NO<sub>2</sub>]≤50 nM roughly equals that in the classical PNM. Significant differences among profiles in the 0.1–1 km regionn are observed, consistent with nitrite pool turnover of 3–7 days estimated from Redfield stoichiometry and tritium-helium ages. Thus seasonal and/or regional variations in factors altering the nitrite production-consumption balance, rather than transport, seem to be responsible for nitrite variability.</p><p>Nitrite profiles with anomalous midwater or near-bottom fine structure, including multi-point maxima and minima, were found along the Venezuelan continental margin and at ≈ 13°N. These featurers are tentatively ascribed to boundary effects, as hydrographic and circumstantial evidence suggests that these waters interacted previously with the bottom.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1329-1347"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90072-2","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"111323420","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90069-6
Sophie Wacongne , Boër Piton
Northeast of a line joining approximately 35°W, 5°S to 15°E, 25°S in the South Atlantic is the locus of a large-scale cyclonic geostrophic gyre, masked by northwestward Ekman flow at the surface and coincident with a zone of cyclonic wind stress curl. According to some descriptions, the gyre is centered near 4°E, 13°S, has a northern limb of eastward-flowing South Equatorial Countercurrernt and an eastern limb of poleward-flowing coastal Angola Current. It therefore appears to be eastern-intensified, a curious situation in view of the dynamics thought to govern motion in large-scale gyres. The northeastern corner of this ocean is also where two other eastward currents, the Equatorial Undercurrent and the South Equatorial Undercurrent, terminate and possibly feed the coastal flow.
The apparent eastern intensification of the observed geostrophic circulation is likely to be caused by the superposition of different dynamical regimes: on the one hand, a relatively weak circulation in Sverdrup balance including the South Equatorial Countercurrent and closing cyclonically within the interior, and on the other, relatively strong near-equatorial and coastal flows which, though geostrophic in the cross-stream direction, have entirely separate dynamics. Previous observations in the northeastern corner of the South Atlantic and relevant model results are examined within the framework of this hypothesis. An analysis of unpublished current measurements off Gabon and Congo (8°E-12°E, 1°S-6°S) shows a highly variable poleward undercurrent along the continental break. We refer to this current as the Gabon-Congo Undercurrent and compare it to the Peru-Chile Undercurrent in the eastern South Pacific, discussing its interpretation as a branch of the terminating Equatorial Undercurrent.
{"title":"The near-surface circulation in the northeastern corner of the South Atlantic ocean","authors":"Sophie Wacongne , Boër Piton","doi":"10.1016/0198-0149(92)90069-6","DOIUrl":"10.1016/0198-0149(92)90069-6","url":null,"abstract":"<div><p>Northeast of a line joining approximately 35°W, 5°S to 15°E, 25°S in the South Atlantic is the locus of a large-scale cyclonic geostrophic gyre, masked by northwestward Ekman flow at the surface and coincident with a zone of cyclonic wind stress curl. According to some descriptions, the gyre is centered near 4°E, 13°S, has a northern limb of eastward-flowing South Equatorial Countercurrernt and an eastern limb of poleward-flowing coastal Angola Current. It therefore appears to be eastern-intensified, a curious situation in view of the dynamics thought to govern motion in large-scale gyres. The northeastern corner of this ocean is also where two other eastward currents, the Equatorial Undercurrent and the South Equatorial Undercurrent, terminate and possibly feed the coastal flow.</p><p>The apparent eastern intensification of the observed geostrophic circulation is likely to be caused by the superposition of different dynamical regimes: on the one hand, a relatively weak circulation in Sverdrup balance including the South Equatorial Countercurrent and closing cyclonically within the interior, and on the other, relatively strong near-equatorial and coastal flows which, though geostrophic in the cross-stream direction, have entirely separate dynamics. Previous observations in the northeastern corner of the South Atlantic and relevant model results are examined within the framework of this hypothesis. An analysis of unpublished current measurements off Gabon and Congo (8°E-12°E, 1°S-6°S) shows a highly variable poleward undercurrent along the continental break. We refer to this current as the Gabon-Congo Undercurrent and compare it to the Peru-Chile Undercurrent in the eastern South Pacific, discussing its interpretation as a branch of the terminating Equatorial Undercurrent.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1273-1298"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90069-6","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"99028655","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90064-Z
Jorge E. Capella , Langdon B. Quetin , Eileen E. Hofmann , Robin M. Ross
A three-dimensional time-dependent model of the circulation in the Bransfield Strait-South Shetland Islands region and a physiologically-based, temperature-dependent model of the descent-ascent behavior of the embryos and larvae of Euphausia superba were combined in a Lagrangian particle tracing model to simulate trajectories of krill embryos and larvae. The Lagrangian calculations show that: (1) surface flow is the primary factor influencing the final location of the embryo-larva particle; and (2) timing of krill spawning affects the eventual position of the feeding larvae. Seasonal changes in the wind stress field result in variability in direction and velocity of surface currents, which affects the embryo-larva trajectories. Conditions favourable for the transport of larvae to Bransfield Strait occur early in the spawning season. East of the Antarctic Peninsula larvae have a greater probability of entering Bransfield Strait if the krill embryos are released in mid-summer, January to February. Embryos released to the north of the South Shetland Islands, west of 62°W are transported into Drake Passage. Embryos released to the north of the South Shetland Islands and east of Livingston Island are transported westward where they can eventually enter Bransfield Strait. Krill larvae also are transported into Bransfield Strait from the Bellingshausen and Weddell Seas. The Lagrangian trajectories show that the western Bransfield Strait is a region of potentially high larval concentration due to transport from surrounding areas as well as local production. This is in agreement with observed krill larvae distributions, which show higher concentrations in this region.
{"title":"Models of the early life history of Euphausia superba—Part II. Lagrangian calculations","authors":"Jorge E. Capella , Langdon B. Quetin , Eileen E. Hofmann , Robin M. Ross","doi":"10.1016/0198-0149(92)90064-Z","DOIUrl":"10.1016/0198-0149(92)90064-Z","url":null,"abstract":"<div><p>A three-dimensional time-dependent model of the circulation in the Bransfield Strait-South Shetland Islands region and a physiologically-based, temperature-dependent model of the descent-ascent behavior of the embryos and larvae of <em>Euphausia superba</em> were combined in a Lagrangian particle tracing model to simulate trajectories of krill embryos and larvae. The Lagrangian calculations show that: (1) surface flow is the primary factor influencing the final location of the embryo-larva particle; and (2) timing of krill spawning affects the eventual position of the feeding larvae. Seasonal changes in the wind stress field result in variability in direction and velocity of surface currents, which affects the embryo-larva trajectories. Conditions favourable for the transport of larvae to Bransfield Strait occur early in the spawning season. East of the Antarctic Peninsula larvae have a greater probability of entering Bransfield Strait if the krill embryos are released in mid-summer, January to February. Embryos released to the north of the South Shetland Islands, west of 62°W are transported into Drake Passage. Embryos released to the north of the South Shetland Islands and east of Livingston Island are transported westward where they can eventually enter Bransfield Strait. Krill larvae also are transported into Bransfield Strait from the Bellingshausen and Weddell Seas. The Lagrangian trajectories show that the western Bransfield Strait is a region of potentially high larval concentration due to transport from surrounding areas as well as local production. This is in agreement with observed krill larvae distributions, which show higher concentrations in this region.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1201-1220"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90064-Z","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"99723168","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90063-Y
Eileen E. Hofmann , Jorge E. Capella , Robin M. Ross , Langdon B. Quetin
A time- and temperature-dependent model was developed to simulate the descent-ascent behavior of the embryos and early larval stages of the Antarctic krill, Euphausia superba. This model combines laboratory measurements of temperature effects on developmental times, density and physiology of krill embryos and larvae and the observed water temperature structure in the Bransfield Strait-South Shetland Islands region. Simulations with observed vertical temperature profiles from this region show that embryos that develop at temperatures less than 0°C hatch relatively deep (≈1000 m) or hit the bottom before hatching. The presence of warm (1–2°C) Circumpolar Deep Water (CDW), between 200 and 700 m, results in hatching depths of about 700 m. The sinking rate pattern characteristic of the embryos of Euphausia superba retains the embryos in the CDW, where development is accelerated. Larval ascent rate through the CDW is rapid, so larvae reach the surface before metamorphosing into the first feeding stage, and have sufficient carbon reserves to drift at the surface for several weeks before needing to find food. These results suggest that the sinking rate pattern characteristic of embryos of Antarctic krill may be part of a reproductive strategy that evolved in response to the thermal structure of its environment. The complementary component of this reproductive strategy is the observed correlation between the distribution of krill schools containing reproducing individuals and the presence of CDW. With this reproductive strategy, the spawning regions of Antarctic krill are in areas where oceanic conditions enhance the probability of survival of its embryos and non-feeding larvae.
{"title":"Models of the early life history of Euphausia superba—Part I. Time and temperature dependence during the descent-ascent cycle","authors":"Eileen E. Hofmann , Jorge E. Capella , Robin M. Ross , Langdon B. Quetin","doi":"10.1016/0198-0149(92)90063-Y","DOIUrl":"10.1016/0198-0149(92)90063-Y","url":null,"abstract":"<div><p>A time- and temperature-dependent model was developed to simulate the descent-ascent behavior of the embryos and early larval stages of the Antarctic krill, <em>Euphausia superba</em>. This model combines laboratory measurements of temperature effects on developmental times, density and physiology of krill embryos and larvae and the observed water temperature structure in the Bransfield Strait-South Shetland Islands region. Simulations with observed vertical temperature profiles from this region show that embryos that develop at temperatures less than 0°C hatch relatively deep (≈1000 m) or hit the bottom before hatching. The presence of warm (1–2°C) Circumpolar Deep Water (CDW), between 200 and 700 m, results in hatching depths of about 700 m. The sinking rate pattern characteristic of the embryos of <em>Euphausia superba</em> retains the embryos in the CDW, where development is accelerated. Larval ascent rate through the CDW is rapid, so larvae reach the surface before metamorphosing into the first feeding stage, and have sufficient carbon reserves to drift at the surface for several weeks before needing to find food. These results suggest that the sinking rate pattern characteristic of embryos of Antarctic krill may be part of a reproductive strategy that evolved in response to the thermal structure of its environment. The complementary component of this reproductive strategy is the observed correlation between the distribution of krill schools containing reproducing individuals and the presence of CDW. With this reproductive strategy, the spawning regions of Antarctic krill are in areas where oceanic conditions enhance the probability of survival of its embryos and non-feeding larvae.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1177-1200"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90063-Y","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"108296001","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
The particulate fluxes of A1 are generally greater in the western North Pacific than in the central and eastern North Pacific, Atlantic and Antarctic oceans. For instance, sediment trap data reported in this paper show the Al flux in the northern part of the Japan Trench is 12.7 mg m−2 day−1 at 5.2 km depth, 130 times greater than that in the deep Antarctic, even though total particulate fluxes are similar. The particulate fluxes of A1 extrapolated to the ocean surface layer roughly equals the observed A1 flux occurring at the ocean-atmosphere interface, suggesting that particulate A1 is atmospheric in origin. Excess A1 fluxes in the subsurface water probably indicate horizontal transport from the continental margin. This is indicated by the different Mg/K ratios of settling particles between the western and eastern North Pacific.
北太平洋西部的A1颗粒通量一般大于北太平洋中部和东部、大西洋和南极海洋。例如,本文报告的沉积物捕集器数据显示,日本海沟北部在5.2公里深度处的Al通量为12.7 mg m - 2 day - 1,是南极深处的130倍,尽管总颗粒通量相似。外推到海洋表层的A1颗粒通量大致等于在海洋-大气界面观测到的A1通量,这表明A1颗粒起源于大气。地下水中过量的A1通量可能表明来自大陆边缘的水平输送。北太平洋西部和东部沉降颗粒的Mg/K比值不同表明了这一点。
{"title":"Particulate flux of A1, a component of land origin, in the western North Pacific","authors":"Chizuru Saito , Shinichiro Noriki , Shizuo Tsunogai","doi":"10.1016/0198-0149(92)90071-Z","DOIUrl":"https://doi.org/10.1016/0198-0149(92)90071-Z","url":null,"abstract":"<div><p>The particulate fluxes of A1 are generally greater in the western North Pacific than in the central and eastern North Pacific, Atlantic and Antarctic oceans. For instance, sediment trap data reported in this paper show the Al flux in the northern part of the Japan Trench is 12.7 mg m<sup>−2</sup> day<sup>−1</sup> at 5.2 km depth, 130 times greater than that in the deep Antarctic, even though total particulate fluxes are similar. The particulate fluxes of A1 extrapolated to the ocean surface layer roughly equals the observed A1 flux occurring at the ocean-atmosphere interface, suggesting that particulate A1 is atmospheric in origin. Excess A1 fluxes in the subsurface water probably indicate horizontal transport from the continental margin. This is indicated by the different Mg/K ratios of settling particles between the western and eastern North Pacific.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1315-1327"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90071-Z","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"137435252","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90068-5
Arthur J Mariano , Otis B Brown
We develop a generalized approach for the objective analysis of nonstationary, heterogeneous fields. An algorithm is presented that uses an anisotropic, time-dependent correlation function with correlation parameters that vary in space/time and a time-dependent trend surface for efficient objective analysis of dynamically heterogeneous and nonstationary fields. The algorithm, which we term the “parameter matrix algorithm”, is applied to two data sets. The first is tropical Pacific sea surface temperature (SST) derived from satellite AVHRR data and Pan-Toga drifting buoys. The SST appliclication illustrates how the parameter matrix is used for the computationally efficient objective analysis of the tropical Pacific SST from 30°S to 30°N at 0.2° resolution (over 290,000 grid points) using approximately 350,000 data points from 12 2-day satellite SST composites. The second example uses data from the Anatomy of a Meander/ BIOSYNOP experiment in the Gulf Stream ring and meander region and illustrates that an objective analysis using the parameter matrix can yield a more accurate representation of oceanic features than typical objective analysis techniques.
{"title":"Efficient objective analysis of dynamically heterogeneous and nonstationary fields via the parameter matrix","authors":"Arthur J Mariano , Otis B Brown","doi":"10.1016/0198-0149(92)90068-5","DOIUrl":"https://doi.org/10.1016/0198-0149(92)90068-5","url":null,"abstract":"<div><p>We develop a generalized approach for the objective analysis of nonstationary, heterogeneous fields. An algorithm is presented that uses an anisotropic, time-dependent correlation function with correlation parameters that vary in space/time and a time-dependent trend surface for efficient objective analysis of dynamically heterogeneous and nonstationary fields. The algorithm, which we term the “parameter matrix algorithm”, is applied to two data sets. The first is tropical Pacific sea surface temperature (SST) derived from satellite AVHRR data and Pan-Toga drifting buoys. The SST appliclication illustrates how the parameter matrix is used for the computationally efficient objective analysis of the tropical Pacific SST from 30°S to 30°N at 0.2° resolution (over 290,000 grid points) using approximately 350,000 data points from 12 2-day satellite SST composites. The second example uses data from the Anatomy of a Meander/ BIOSYNOP experiment in the Gulf Stream ring and meander region and illustrates that an objective analysis using the parameter matrix can yield a more accurate representation of oceanic features than typical objective analysis techniques.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1255-1271"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90068-5","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"72275709","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90078-8
W.H. Thomas , C.H. Gibson
Gymnodinium sanguineum dinoflagellate cultures were subjected to constant staining flows to quantify the threshold level for growth inhibition by viscous streses for this organisms and to compare its response to that of a red tide species Gonyaulax polyedra previously studied. Growth inhibition of Gymnodinium was detected at rates-of-strain γ as small as 1 rad s−1 and was independent of γ in the range 1–40 rad s−1. Growth was delayed for 2–5 days, but not prevented entirely. For Gonyaulax, growth inhibition began for γ ≈ 3 rad s−, and growth was prevented entirely above 8 rads s−1. The fishery implication is that the apparent necessity of calm seas (Lasker Events) for the growth of larval northern anchovies may not be due to turbulence inhibition of their Gymnodinium food supply.
我们对裸子藻(Gymnodinium sanguineum dinoflagellate)培养物进行了持续染色,以量化这种生物在粘性胁迫下生长抑制的阈值水平,并将其与先前研究过的赤潮物种Gonyaulax polydra的反应进行了比较。菌株γ的速率小至1 rad s- 1,且在1 - 40 rad s- 1范围内与γ无关。生长延迟2-5天,但不能完全阻止。对于Gonyaulax,在γ≈3 rads−时开始抑制生长,在8 rads−1以上完全阻止生长。渔业的含义是,平静的海洋(拉斯克事件)对北方凤尾鱼幼体生长的明显必要性可能不是由于湍流抑制了它们的裸子鱼食物供应。
{"title":"Effects of quantified small-scale turbulence on the dinoflagellate, Gymnodium sanguineum (splendens): contrasts with Gonyaulax (Lingulodinium) polyedra, and the fishery implication","authors":"W.H. Thomas , C.H. Gibson","doi":"10.1016/0198-0149(92)90078-8","DOIUrl":"10.1016/0198-0149(92)90078-8","url":null,"abstract":"<div><p><em>Gymnodinium sanguineum</em> dinoflagellate cultures were subjected to constant staining flows to quantify the threshold level for growth inhibition by viscous streses for this organisms and to compare its response to that of a red tide species <em>Gonyaulax polyedra</em> previously studied. Growth inhibition of <em>Gymnodinium</em> was detected at rates-of-strain γ as small as 1 rad s<sup>−1</sup> and was independent of γ in the range 1–40 rad s<sup>−1</sup>. Growth was delayed for 2–5 days, but not prevented entirely. For <em>Gonyaulax</em>, growth inhibition began for γ ≈ 3 rad s<sup>−</sup>, and growth was prevented entirely above 8 rads s<sup>−1</sup>. The fishery implication is that the apparent necessity of calm seas (Lasker Events) for the growth of larval northern anchovies may not be due to turbulence inhibition of their <em>Gymnodinium</em> food supply.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1429-1437"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90078-8","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"106086157","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 1992-07-01DOI: 10.1016/0198-0149(92)90062-X
R.D Pingree , B Le Cann
Jet-like extensions of the slope current off northern Spain and France in the southern Bay of Biscay in the winter develop into anticyclonic eddies with an upper core of slope water. Three eddies were observed to develop in the winter of 1989/1990, subsequently named F90a, F90b and O90. F90a was an anticclonic eddy of radius 50–60 km, with a central core of mixed water of slope origin (from the slopes in the vicinity of Cap Ferret Canyon) and of volume ∼400 k3. In the eddt centre, the mixed core extended from ∼70 to ∼280 m. Measurements at sea showed minimal changes in the core characteristics of F90a (potential temperature, 12.95°C, salinity, 35.74 psu) with time, and remote sensing studies demonstrated that these slope water core eddies can maintain their identities for about a year. Rotation rates in the central core of F90a were about 3 days and values of normalized relative vorticity were about −0.5. Maximummean azimuthal velocities were about 30 cm s−1 at a radius of 30 km. Hydrographic data showed that the presence of the core was felt to a depth of ∼1500m, resulting in an azimuthal transport of about 8 Sv. Both F90a and O90 moved westward across the deep (4800 m) Bay of Biscay, and the westward migration speed (2 cm s−1) seems in excess of simple theoretical estimates for the β-induced westward propagation speed (0.4 cm s−1) of anticyclonic eddies. If the latter figure is used for self-advection and the effects of topography and mutual influence are neglected, the observed westward movement suggests a clockwise mean circulation −2 cm s−1) for the oceanic water in the Bay of Biscay. By contrast, F90b remained nearly stationary near 4°W. Remote sensing studies indicate that the occurence of a 4°W eddy in the summer of any year miight be attributed to warm slope water inflow along the northern Spanish slope in the previous winter.
冬季,西班牙北部和法国南部比斯开湾的斜坡流的射流状延伸发展成反气旋涡流,上部核心为斜坡水。1989/1990年冬季观测到形成了三个涡旋,随后命名为F90a、F90b和O90。F90a是一个半径为50-60 km的反涡旋,其中心核心是斜坡来源的混合水(来自雪雷帽峡谷附近的斜坡),体积约为400 k3。在eddt中心,混合岩心从~ 70米延伸到~ 280米。海上测量显示,F90a的核心特征(位势温度12.95°C,盐度35.74 psu)随时间变化很小,遥感研究表明,这些斜坡水核心漩涡可以保持大约一年的特征。F90a中心涡旋速率约为3 d,标准化相对涡度值约为- 0.5。在半径30公里处,最大平均方位角速度约为30 cm s - 1。水文数据显示,在约1500米的深度可以感觉到岩心的存在,导致了大约8 Sv的方位传输。F90a和O90都在比斯开湾深处(4800 m)向西移动,向西移动的速度(2 cm s−1)似乎超过了β诱导的反气旋涡旋向西传播速度(0.4 cm s−1)的简单理论估计。如果后一个图用于自平流,并且忽略地形和相互影响的影响,则观测到的向西运动表明比斯开湾海水的平均顺时针环流为- 2 cm s - 1)。相比之下,F90b在4°W附近几乎保持静止。遥感研究表明,每年夏季出现的4°W涡旋可能是由于前一个冬季沿西班牙北部斜坡流入的暖坡水。
{"title":"Three anticyclonic slope water oceanic eDDIES (SWODDIES) in the Southern Bay of Biscay in 1990","authors":"R.D Pingree , B Le Cann","doi":"10.1016/0198-0149(92)90062-X","DOIUrl":"10.1016/0198-0149(92)90062-X","url":null,"abstract":"<div><p>Jet-like extensions of the slope current off northern Spain and France in the southern Bay of Biscay in the winter develop into anticyclonic eddies with an upper core of slope water. Three eddies were observed to develop in the winter of 1989/1990, subsequently named F90a, F90b and O90. F90a was an anticclonic eddy of radius 50–60 km, with a central core of mixed water of slope origin (from the slopes in the vicinity of Cap Ferret Canyon) and of volume ∼400 k<sup>3</sup>. In the eddt centre, the mixed core extended from ∼70 to ∼280 m. Measurements at sea showed minimal changes in the core characteristics of F90a (potential temperature, 12.95°C, salinity, 35.74 psu) with time, and remote sensing studies demonstrated that these slope water core eddies can maintain their identities for about a year. Rotation rates in the central core of F90a were about 3 days and values of normalized relative vorticity were about −0.5. Maximummean azimuthal velocities were about 30 cm s<sup>−1</sup> at a radius of 30 km. Hydrographic data showed that the presence of the core was felt to a depth of ∼1500m, resulting in an azimuthal transport of about 8 Sv. Both F90a and O90 moved westward across the deep (4800 m) Bay of Biscay, and the westward migration speed (2 cm s<sup>−1</sup>) seems in excess of simple theoretical estimates for the β-induced westward propagation speed (0.4 cm s<sup>−1</sup>) of anticyclonic eddies. If the latter figure is used for self-advection and the effects of topography and mutual influence are neglected, the observed westward movement suggests a clockwise mean circulation −2 cm s<sup>−1</sup>) for the oceanic water in the Bay of Biscay. By contrast, F90b remained nearly stationary near 4°W. Remote sensing studies indicate that the occurence of a 4°W eddy in the summer of any year miight be attributed to warm slope water inflow along the northern Spanish slope in the previous winter.</p></div>","PeriodicalId":81079,"journal":{"name":"Deep-sea research. Part A, Oceanographic research papers","volume":"39 7","pages":"Pages 1147-1175"},"PeriodicalIF":0.0,"publicationDate":"1992-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0198-0149(92)90062-X","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"91295014","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}