Temporal and Spatial Flux Changes of Radiolarians in the Northwestern

Total Page:16

File Type:pdf, Size:1020Kb

Temporal and Spatial Flux Changes of Radiolarians in the Northwestern ARTICLE IN PRESS Deep-Sea Research II 52 (2005) 2240–2274 www.elsevier.com/locate/dsr2 Temporal and spatial flux changes of radiolarians in the northwestern Pacific Ocean during 1997–2000 Yusuke Okazakia,Ã, Kozo Takahashib, Jonaotaro Onoderab, Makio C. Hondac aOcean Research Institute, University of Tokyo, Minamidai 1-15-1, Nakano-ku, Tokyo 164-8639, Japan bDepartment of Earth and Planetary Sciences, Graduate School of Science, Kyushu University, Hakozaki 6-10-1, Fukuoka 812-8581, Japan cJapan Agency for Marine-Earth Science and Technology, Natsushima 2-15, Yokosuka 237-0061, Japan Received 30 September 2003; accepted 28 July 2005 Available online 20 October 2005 Abstract In order to examine the radiolarian fluxes and evaluate their relationship to the physical and biological environments, time-series sediment traps were deployed at three stations (Stations 50N, KNOT, and 40N) in the northwestern North Pacific from 1997 to 2000. Station 50N (501N, 1651E, 3260 m) is located in the center of Western Subarctic Gyre (WSAG); Station KNOT (441N, 1551E, 2957 m) is located toward the margin of WSAG; and Station 40N (401N, 1651E, 2986 m) is located in the Subarctic Boundary. Total radiolaria fluxes at Station 40N showed higher values than those at the other two stations, and were mainly attributed to the influence of relatively high-temperature and high-salinity subtropical gyre waters. Correlation coefficients between total mass fluxes (mainly composed of diatoms) and radiolarian fluxes at three stations were relatively low. This is primarily because of the wide vertical distribution of radiolarians and various trophic patterns corresponding to their niche. Radiolarian species were classified according to their geographic water mass and vertical distributions based on previous studies using sediment samples. As a result, seasonal changes of radiolarian fluxes in each water mass showed patterns corresponding to particular controlling factors such as physical hydrography and food conditions. Among these patterns, temporal changes in radiolarian taxonomic composition in the upper layer (0–100 m) seemed to reflect well the sea-surface temperature anomaly (SSTA) changes, affected by El Nin˜o and La Nin˜a events, at Station 40N. Therefore, radiolarian assemblages can be used to reconstruct past SSTA changes and to understand the past El Nin˜o and La Nin˜a teleconnection in the Kuroshio-Oyashio Extension region. r 2005 Elsevier Ltd. All rights reserved. Keywords: Radiolaria; Sediment trap; Temporal flux variation; Western Subarctic Gyre; Subarctic Boundary; El Nin˜o; La Nin˜a 1. Introduction change and ecological environment. Therefore, a better knowledge of the present relationship be- Microplankton shells and skeletons have been tween the ecology of microplankton and the used as various proxies to reconstruct past climate physical and biological environmental conditions will improve our understanding of both paleocea- Ã Corresponding author at: Institute of Observational Research nography and present-day oceanography. Radiolar- for Global Change, Japan Agency for Marine-Earth Science and Technology, 2-15 Natsushima-cho, Yokosuka 237-0061, Japan. ia are siliceous microzooplankton with high Tel.: +81 46 867 9515; fax: +81 46 867 9455. diversity that dwell in a wide range of depth zones E-mail address: [email protected] (Y. Okazaki). from the surface water down to several thousand 0967-0645/$ - see front matter r 2005 Elsevier Ltd. All rights reserved. doi:10.1016/j.dsr2.2005.07.006 ARTICLE IN PRESS Y. Okazaki et al. / Deep-Sea Research II 52 (2005) 2240–2274 2241 meters. Thus, they have a potential to be a proxy of 1993). However, paleoceanographic knowledge in various vertical water masses. this region is still meager mainly because of the Radiolaria are classified into two taxonomic carbonate dissolution caused by the shallow carbo- groups: Polycystina and Phaeodaria. The skeletons nate compensation depth (CCD). of polycystine radiolarians are often preserved in The northwestern Pacific Ocean is characterized the sediments, whereas phaeodarian radiolarians are by high primary production attributed to diatoms. easily dissolved in the water column because of their Therefore, the efficiency of the biological pump in skeletal constitution and thus are rarely preserved in this region is significantly high (Honda et al., 2002) the sediments (Takahashi et al., 1983). Recently, the and thus, important for the global carbon cycle. importance of the oscillation in the intermediate- There have been some previous taxon-quantitative water production rate during the Quaternary works on radiolarian flux in the subarctic North climate change has been recognized (e.g., Talley, Pacific using time-series sediment traps: the Alaskan 1999). Ganopolski et al. (1998) indicated the Gyre (Stations PAPA and C: Takahashi, 1987, expansion of the North Pacific Intermediate Water 1997), and the central subarctic Pacific (Station SA: (NPIW) formation in the north during the Last Fukumura and Takahashi, 2000). In the north- Glacial Maximum (LGM) and the oscillations in western Pacific, Bernstein et al. (1990) reported the the production of NPIW during the late Quaternary radiolarian fluxes at seven stations. However, they might have been influenced by the major climatic used free-drifting sediment traps and their sampling changes (Kennett et al., 2002). A part of the NPIW durations were only for ca. 24 h. originates in the Okhotsk Sea today (e.g., Talley, In this study we present the modern seasonal 1991; Freeland et al., 1998; Wong et al., 1998), and changes in the time-series radiolarian flux over a 2- the NPIW is distributed mainly between 300 and year period in the northwestern North Pacific and 700 m in the northwestern North Pacific (Talley, evaluate their relationships to the physical and 60°N Bering Sea Gyre Okhotsk KAMCHATKA Gyre East Kamchatka Current 50N 50° SAKHALIN Western Subarctic Gyre HOKKAIDO Oyashio Current KNOT 40° 40N Subarctic Boundary Kuroshio Extension 140°E 150° 160° 170° 180° Fig. 1. Map showing the locations of the three sediment trap stations in the northwestern North Pacific. General circulation patterns are also shown (Map drawn by ‘‘Online Map Creation’’). ARTICLE IN PRESS 2242 Y. Okazaki et al. / Deep-Sea Research II 52 (2005) 2240–2274 biological environmental conditions as an impor- Monthly hydrographic data from the sea surface tant step in reconstructing the past oceanographic to 1000 m depth at each sediment trap station were conditions. obtained from the World Ocean Atlas 1994 (Levitus and Boyer, 1994), and illustrated with the Ocean 2. Materials and methods Data View software package (Fig. 2; Schlitzer, 2002). Time-series sediment traps (McLane Mark 7G- 21) with 21 collecting cups (Honjo and Doherty, 3. Oceanographic setting 1988) were deployed at approximately 3000 m depths at three stations in the northwestern North The subarctic circulation system in the North Pacific (Stations 50N, KNOT, and 40N) from Pacific has a large-scale counterclockwise surface December 1997 to May 2000 (Fig. 1; Table 1). circulation characterized by low salinity (o34.0 psu) The trapping efficiency of the Mark 7G-21 is and relatively low temperature (ca. 4–12 1C) with a approximately 1, indicating an almost 100% collec- sharp halocline (ca. 150–200 m; Favorite et al., tion efficiency in the bathypelagic zone (at depths 1976). The subarctic circulation system has four 41500 m), based on 231Pa and 230Th (Yu et al., gyres from east to west: Alaskan Gyre, Bering Sea 2001). Their recovery, maintenance and redeploy- Gyre, Western Subarctic Gyre (WSAG), and ment were carried out during the cruises of the R.V. Okhotsk Sea Gyre (OSG). The features of the Mirai, Japan Agency for Marine-Earth Science and WSAG water mass are as follows: (1) strong vertical Technology (JAMSTEC). mixing down to 150 m water depth caused by the Samples for radiolarian analyses were sieved cooling of the sea-surface water accompanied by through a stainless screen with 1 mm mesh to radiative atmospheric cooling during winter, (2) the remove larger plankton, and then split into an strong and stable stratification beneath the surface appropriate aliquot size ranging from 1/100 to layer resulting in a significant halocline, (3) the 1/132. The split samples were sieved through a sharp thermocline formation caused by heating of stainless steel screen with 63 mm mesh and filtered the sea-surface water accompanied by the rise of air through Gelmans membrane filters with a nominal temperature during summer. The most significant pore size of 0.45 mm. The filtered samples were characteristic of the WSAG is the presence of a washed with distilled water to remove salt, dried in temperature minimum (ca. 2–4 1C) subsurface layer an oven at 50 1C overnight, and then permanently (ca. 50–150 m) called the ‘‘dichothermal layer’’ mounted with Canada balsam on microslides. All (Nagata et al., 1992). The temperature maximum coarse-sized radiolarian skeletons (463 mm) on a layer below the dichothermal layer is also a microslide were counted with a light microscope and characteristic of the WSAG (Nagata et al., 1992). computed to derive radiolarian fluxes (No. radi- Below the dichothermal layer, the NPIW is defined olarians mÀ2 dayÀ1) at each station. Species identi- as the main salinity minimum in the subtropical fication of radiolarians was performed according to North Pacific at a density of 26.7–26.8sy (ca. the taxonomy of the following works: Nigrini 300–700 m; Talley, 1993). In the WSAG, the East (1970), Renz (1976), Bjørklund (1976), Boltovskoy Kamchatka Current flows southward along the and Riedel (1987), Takahashi (1991), Abelmann Kamchatka Peninsula (Fig. 1). A part of the East (1992b), Welling (1996), Nigrini and Moore (1979), Kamchatka Current flows into the Okhotsk Sea Bjørklund et al. (1998), and Nimmergut and through the passes in the northern Kuril Islands. Abelmann (2002). Diversity indices using the The Okhotsk Sea water plays a significant role in Shannon-Wiener log-base 2 formula (H: Shannon the water-mass formation and modification of the and Weaver, 1949) were used.
Recommended publications
  • First Application of PDMPO to Examine Silicification in Polycystine Radiolaria
    Plankton Benthos Res 4(3): 89–94, 2009 Plankton & Benthos Research © The Plankton Society of Japan First application of PDMPO to examine silicification in polycystine Radiolaria KAORU OGANE1,*, AKIHIRO TUJI2, NORITOSHI SUZUKI1, TOSHIYUKI KURIHARA3 & ATSUSHI MATSUOKA4 1 Institute of Geology and Paleontology, Graduate School of Science, Tohoku University, Sendai, 980–8578, Japan 2 Department of Botany, National Museum of Nature and Science, Tsukuba, 305–0005, Japan 3 Graduate School of Science and Technology, Niigata University, Niigata 950–2181, Japan 4 Department of Geology, Faculty of Science, Niigata University, Niigata 950–2181, Japan Received 4 February 2009; Accepted 10 April 2009 Abstract: 2-(4-pyridyl)-5-[(4-(2-dimethylaminoethylaminocarbamoyl)methoxy)-phenyl] oxazole (PDMPO) is a fluo- rescent compound that accumulates in acidic cell compartments. PDMPO is accumulated with silica under acidic con- ditions, and the newly developed silica skeletons show green fluorescent light. This study is the first to use PDMPO in polycystine radiolarians, which are unicellular planktonic protists. We tested Acanthodesmia sp., Rhizosphaera trigo- nacantha, and Spirocyrtis scalaris for emission of green fluorescence. Entire skeletons of Acanthodesmia sp. and Sr. scalaris emitted green fluorescent light, whereas only the outermost shell and radial spines of Rz. trigonacantha showed fluorescence. Two additional species, Spongaster tetras tetras and Rhopalastrum elegans did not show fluorescence. Green fluorescence of the entire skeleton is more like the “skeletal thickening growth” defined by silica deposition throughout the surface of the existing skeleton. The brightness of the fluorescence varied with each cell. This difference in fluorescence may reflect the rate of growth in these cells. Green fluorescence in PDMPO-treated polycystines sug- gests the presence of similar metabolic systems with controlled pH.
    [Show full text]
  • Radiozoa (Acantharia, Phaeodaria and Radiolaria) and Heliozoa
    MICC16 26/09/2005 12:21 PM Page 188 CHAPTER 16 Radiozoa (Acantharia, Phaeodaria and Radiolaria) and Heliozoa Cavalier-Smith (1987) created the phylum Radiozoa to Radiating outwards from the central capsule are the include the marine zooplankton Acantharia, Phaeodaria pseudopodia, either as thread-like filopodia or as and Radiolaria, united by the presence of a central axopodia, which have a central rod of fibres for rigid- capsule. Only the Radiolaria including the siliceous ity. The ectoplasm typically contains a zone of frothy, Polycystina (which includes the orders Spumellaria gelatinous bubbles, collectively termed the calymma and Nassellaria) and the mixed silica–organic matter and a swarm of yellow symbiotic algae called zooxan- Phaeodaria are preserved in the fossil record. The thellae. The calymma in some spumellarian Radiolaria Acantharia have a skeleton of strontium sulphate can be so extensive as to obscure the skeleton. (i.e. celestine SrSO4). The radiolarians range from the A mineralized skeleton is usually present within the Cambrian and have a virtually global, geographical cell and comprises, in the simplest forms, either radial distribution and a depth range from the photic zone or tangential elements, or both. The radial elements down to the abyssal plains. Radiolarians are most useful consist of loose spicules, external spines or internal for biostratigraphy of Mesozoic and Cenozoic deep sea bars. They may be hollow or solid and serve mainly to sediments and as palaeo-oceanographical indicators. support the axopodia. The tangential elements, where Heliozoa are free-floating protists with roughly present, generally form a porous lattice shell of very spherical shells and thread-like pseudopodia that variable morphology, such as spheres, spindles and extend radially over a delicate silica endoskeleton.
    [Show full text]
  • Order Spumellaria Family Collosphaeridae
    Order Spumellaria Family Collosphaeridae Acrosphaera murrayana (Haeckel) (Figure 15.19) [=Polysolenia murrayana]. Large pores, each surrounded by a crown of short spines. Shell diameter: 70-180 µm. Ref: Strelkov and Reshetnjak (1971), Nigrini and Moore (1979). Acrosphaera spinosa (Haeckel) group? (Figure 1D, 15.18) [=Polysolenia spinosa, ?P. lappacea, ?P. flammabunda]. Irregular pores and many irregularly arranged spines scattered about the surface, some of the latter extending from the pore-rims. Spine and pore patterns are variable. Shell diameter: 60-160 µm. Ref: Strelkov and Reshetnjak (1971), Boltovskoy and Riedel (1980). Buccinosphaera invaginata Haeckel (Figure 15.17) [=Collosphaera imvaginata]. The smooth shell produces several pored tubes directed toward the center of the sphere. Rather small, irregular pores. Shell diameter: 100-130 µm. Ref: Strelkov and Reshetnjak (1971), Nigrini (1971). 35 Collosphaera huxleyi Müller (Figure 1E, 15.13). Shells with small to medium-sized pores scattered about the surface only; no spines or tubes. Shell diameter: 80-150 µm. Ref: Strelkov and Reshetnjak (1971), Boltovskoy and Riedel (1980). Collosphaera macropora Popofsky (Figure 15.15). No spines or tubes on shell surface; few very large pores, sometimes angular. Shell diameter: 100-120 µm. Ref: Strelkov and Reshetnjak (1971), Boltovskoy and Riedel (1980). Collosphaera tuberosa Haeckel (Figure 15.14). No spines or tubes on shell surface, but with conspicuous lumps and depressions; many small, irregularly shaped pores. Shell diameter: 50-300 µm. Ref: Strelkov and Reshetnjak (1971), Boltovskoy and Riedel (1980). Siphonosphaera martensi Brandt (Figure 15.20). Each pore bears a short centrifugal tube, tube walls are imperforate. Shell diameter: 90-100 µm. Ref: Strelkov and Reshetnjak (1971).
    [Show full text]
  • Einführung in Das Studium Der Radiolarien
    Naturwissenschaftliche Vereinigung Hagen e.V. Mikroskopische Arbeitsgemeinschaft GERHARD GÖKE Einführung in das Studium der Radiolarien Veröffentlichung der NWV-Hagen e.V Sonderheft SH 2 September 1994 Von der MIKRO-HAMBURG mit neuem Layout versehen 2008 2 Gerhard Göke Einführung in das Studium der Radiolarien Präparation und Untersuchungsmethoden Inhaltsverzeichnis Geschichte der Radiolarienforschung 3 Die Radiolarien der Challenger-Expedition 12 Zur Bearbeitung der Barbados-Radiolarien 19 Weichkörper, Fortpflanzung, Ökologie, Bathymetrie 22 Stammesgeschichte, Skelettbau und System 26 Fang und Lebendbeobachtung rezenter Radiolarien 32 Aufbereitung fossiler Radiolarien 33 Die Herstellung von Mikropräparaten: 34 Streupräparate 34 Gelegte Einzelformen 35 Typenplatten und Fundortplatten 35 Auflichtpräparate 36 System der Radiolarien 37 Tafeln 41 3 Geschichte der Radiolarienforschung Bereits in der ersten Hälfte des 19.Jahrhunderts waren Radiolarien bekannt, obgleich man diese Rhizopoden nicht richtig in das zoologische System einord- nen konnte. In der zweiten Hälfte wurden sie dann so intensiv bearbeitet, daß der Umfang der in diesem Zeitabschnitt veröffentlichten Radiolarienliteratur im 20.Jahrhundert nicht mehr erreicht werden konnte. F.MEYEN beobachtete während seiner „Reise um die Erde" (1832 -1834) die ersten lebenden Radiolarien im Meeresplankton (1). Er nannte sie Palmellarien. Seine Beschreibungen von Sphaerozoum fuscum und Physematium atlanticum blieben lange Zeit das Einzige, was man über die Vertreter dieser Tiergruppe wußte. Noch ältere Beobachtungen von Planktonorganismen, die sich mit gro- ßer Wahrscheinlichkeit als Radiolarien deuten lassen, hat CH.G.EHRENBERG in seiner Abhandlung „Über das Leuchten des Meeres“ zitiert (2). Nach seinen Angaben hat der Naturforscher TILESIUS, der KRUSENSTERN in den Jahren 1803 bis 1806 auf seiner Erdumseglung begleitete, in tropischen Meeren bei großer Hitze und anhaltender Windstille „Infusionsthierchen“ beobachtet, die große Ähnlichkeit mit Acanthometren hatten (3).
    [Show full text]
  • The Horizontal Distribution of Siliceous Planktonic Radiolarian Community in the Eastern Indian Ocean
    water Article The Horizontal Distribution of Siliceous Planktonic Radiolarian Community in the Eastern Indian Ocean Sonia Munir 1 , John Rogers 2 , Xiaodong Zhang 1,3, Changling Ding 1,4 and Jun Sun 1,5,* 1 Research Centre for Indian Ocean Ecosystem, Tianjin University of Science and Technology, Tianjin 300457, China; [email protected] (S.M.); [email protected] (X.Z.); [email protected] (C.D.) 2 Research School of Earth Sciences, Australian National University, Acton 2601, Australia; [email protected] 3 Department of Ocean Science, Hong Kong University of Science and Technology, Kowloon, Hong Kong 4 College of Biotechnology, Tianjin University of Science and Technology, Tianjin 300457, China 5 College of Marine Science and Technology, China University of Geosciences, Wuhan 430074, China * Correspondence: [email protected]; Tel.: +86-606-011-16 Received: 9 October 2020; Accepted: 3 December 2020; Published: 13 December 2020 Abstract: The plankton radiolarian community was investigated in the spring season during the two-month cruise ‘Shiyan1’ (10 April–13 May 2014) in the Eastern Indian Ocean. This is the first comprehensive plankton tow study to be carried out from 44 sampling stations across the entire area (80.00◦–96.10◦ E, 10.08◦ N–6.00◦ S) of the Eastern Indian Ocean. The plankton tow samples were collected from a vertical haul from a depth 200 m to the surface. During the cruise, conductivity–temperature–depth (CTD) measurements were taken of temperature, salinity and chlorophyll a from the surface to 200 m depth. Shannon–Wiener’s diversity index (H’) and the dominance index (Y) were used to analyze community structure.
    [Show full text]
  • Articles and Minimizes the Loss of Material
    Clim. Past, 16, 2415–2429, 2020 https://doi.org/10.5194/cp-16-2415-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Technical note: A new automated radiolarian image acquisition, stacking, processing, segmentation and identification workflow Martin Tetard1, Ross Marchant1,a, Giuseppe Cortese2, Yves Gally1, Thibault de Garidel-Thoron1, and Luc Beaufort1 1Aix Marseille Univ, CNRS, IRD, Coll France, INRAE, CEREGE, Aix-en-Provence, France 2GNS Science, Lower Hutt, New Zealand apresent address: School of Electrical Engineering and Robotics, Queensland University of Technology, Brisbane, Australia Correspondence: Martin Tetard ([email protected]) Received: 3 June 2020 – Discussion started: 9 July 2020 Revised: 22 September 2020 – Accepted: 5 October 2020 – Published: 2 December 2020 Abstract. Identification of microfossils is usually done ing, processing, segmentation and recognition, is entirely by expert taxonomists and requires time and a significant automated via a LabVIEW interface, and it takes approx- amount of systematic knowledge developed over many years. imately 1 h per sample. Census data count and classi- These studies require manual identification of numerous fied radiolarian images are then automatically exported and specimens in many samples under a microscope, which is saved. This new workflow paves the way for the analysis very tedious and time-consuming. Furthermore, identifica- of long-term, radiolarian-based palaeoclimatic records from tion may differ between operators, biasing reproducibility. siliceous-remnant-bearing samples. Recent technological advances in image acquisition, pro- cessing and recognition now enable automated procedures for this process, from microscope image acquisition to taxo- nomic identification. 1 Introduction A new workflow has been developed for automated radio- larian image acquisition, stacking, processing, segmentation The term radiolarians currently refers to the polycystine ra- and identification.
    [Show full text]
  • First Application of PDMPO to Examine Silicification in Polycystine Radiolaria
    Plankton Benthos Res 4(3): 89–94, 2009 Plankton & Benthos Research © The Plankton Society of Japan First application of PDMPO to examine silicification in polycystine Radiolaria KAORU OGANE1,*, AKIHIRO TUJI2, NORITOSHI SUZUKI1, TOSHIYUKI KURIHARA3 & ATSUSHI MATSUOKA4 1 Institute of Geology and Paleontology, Graduate School of Science, Tohoku University, Sendai, 980–8578, Japan 2 Department of Botany, National Museum of Nature and Science, Tsukuba, 305–0005, Japan 3 Graduate School of Science and Technology, Niigata University, Niigata 950–2181, Japan 4 Department of Geology, Faculty of Science, Niigata University, Niigata 950–2181, Japan Received 4 February 2009; Accepted 10 April 2009 Abstract: 2-(4-pyridyl)-5-[(4-(2-dimethylaminoethylaminocarbamoyl)methoxy)-phenyl] oxazole (PDMPO) is a fluo- rescent compound that accumulates in acidic cell compartments. PDMPO is accumulated with silica under acidic con- ditions, and the newly developed silica skeletons show green fluorescent light. This study is the first to use PDMPO in polycystine radiolarians, which are unicellular planktonic protists. We tested Acanthodesmia sp., Rhizosphaera trigo- nacantha, and Spirocyrtis scalaris for emission of green fluorescence. Entire skeletons of Acanthodesmia sp. and Sr. scalaris emitted green fluorescent light, whereas only the outermost shell and radial spines of Rz. trigonacantha showed fluorescence. Two additional species, Spongaster tetras tetras and Rhopalastrum elegans did not show fluorescence. Green fluorescence of the entire skeleton is more like the “skeletal thickening growth” defined by silica deposition throughout the surface of the existing skeleton. The brightness of the fluorescence varied with each cell. This difference in fluorescence may reflect the rate of growth in these cells. Green fluorescence in PDMPO-treated polycystines sug- gests the presence of similar metabolic systems with controlled pH.
    [Show full text]
  • An Evaluated List of Cenozic-Recent Radiolarian Species Names (Polycystinea), Based on Those Used in the DSDP, ODP and IODP Deep-Sea Drilling Programs
    Zootaxa 3999 (3): 301–333 ISSN 1175-5326 (print edition) www.mapress.com/zootaxa/ Article ZOOTAXA Copyright © 2015 Magnolia Press ISSN 1175-5334 (online edition) http://dx.doi.org/10.11646/zootaxa.3999.3.1 http://zoobank.org/urn:lsid:zoobank.org:pub:69B048D3-7189-4DC0-80C0-983565F41C83 An evaluated list of Cenozic-Recent radiolarian species names (Polycystinea), based on those used in the DSDP, ODP and IODP deep-sea drilling programs DAVID LAZARUS1, NORITOSHI SUZUKI2, JEAN-PIERRE CAULET3, CATHERINE NIGRINI4†, IRINA GOLL5, ROBERT GOLL5, JANE K. DOLVEN6, PATRICK DIVER7 & ANNIKA SANFILIPPO8 1Museum für Naturkunde, Invalidenstrasse 43, 10115 Berlin, Germany. E-mail: [email protected] 2Institute of Geology and Paleontology, Tohoku University, Sendai 980-8578 Japan. E-mail: [email protected] 3242 rue de la Fure, Charavines, 38850 France. E-mail: [email protected] 4deceased 5Natural Science Dept, Blinn College, 2423 Blinn Blvd, Bryan, Texas 77805, USA. E-mail: [email protected] 6Minnehallveien 27b, 3290 Stavern, Norway. E-mail: [email protected] 7Divdat Consulting, 1392 Madison 6200, Wesley, Arkansas 72773, USA. E-mail: [email protected] 8Scripps Institution of Oceanography, University of California San Diego, La Jolla, California 92093, USA. E-mail: [email protected] Abstract A first reasonably comprehensive evaluated list of radiolarian names in current use is presented, covering Cenozoic fossil to Recent species of the primary fossilising subgroup Polycystinea. It is based on those species names that have appeared in the literature of the Deep Sea Drilling Project and its successor programs, the Ocean Drilling Program and Integrated Ocean Drilling Program, plus additional information from the published literature, and several unpublished taxonomic da- tabase projects.
    [Show full text]
  • Radiolarian Paleontologists
    RADI LARIA VOLUME 23 SEPTEMBER 2005 NEWSLETTER OF THE INTERNATIONAL ASSOCIATION OF RADIOLARIAN PALEONTOLOGISTS ISSN: 0297.5270 INTERRAD International Association of Radiolarian Paleontologists A Research Group of the International Paleontological Association Officers of the Association President Past President CHRIS HOLLIS PETER BAUMGARTNER Inst. of Geol. and Nuclear Sciences Lausanne, Switzerland Lower Hutt, New Zealand [email protected] [email protected] Secretary Treasurer GIUSEPPE CORTESE ELSPETH URQUHART Alfred Wegener Institute (AWI) P.O. Box 13697 for Polar and Marine Research Musselburgh – East Lothian P.O.Box 120161 Scotland EH21 8YD 27515 Bremerhaven U.K. Germany Tel: 1-305-361-4668 Tel: (471) 2831 1207 Fax: 1-305-361-4632 Fax: (471) 2831 1149 Email: [email protected] e-mail: [email protected] Working Group Chairmen Paleozoic Cenozoic PATRICIA WHALEN, U.S.A. ANNIKA SANFILIPPO California, U.S.A. [email protected] [email protected] Mesozoic Recent LUIS O’DOGHERTY, Cadiz, SPAIN DEMETRIO BOLTOVSKOY Buenos Aires, ARGENTINA [email protected] [email protected] INTERRAD is an international non-profit organization for researchers interested in all aspects of radiolarian taxonomy, palaeobiology, morphology, biostratigraphy, biology, ecology and paleoecology. INTERRAD is a Research Group of the International Paleontological Association (IPA). Since 1978 members of INTERRAD meet every three years to present papers and exchange ideas and materials. INTERRAD MEMBERSHIP: The international Association of Radiolarian Paleontologists is open to any one interested on receipt of subscription. The actual fee is US $ 15 per year. Membership queries and subscription are sent to the Treasurer. Changes of address can be sent to the Secretary.
    [Show full text]
  • De Wever Family
    Table 2 Summary of radiolarian hierarchy as described in De Wever et al. (2002), summarised by F.J.Gregory 2004 Order Superfamily Subsuperfamily Family Subfamily Archaeospicularia Echidninacea Echidninidae Secuicollactacea Secuicollactidae Pseudorotasphaeridae Albaillellaria Ceratoikiscidae Albaillellidae Follicucullidae Corythoecidae Palacantholithidae Latentifistularia Pseudolitheliidae** Latentifistulidae Ruzhencevispongidae Cauletellidae Ormistonellidae** Spumellaria** Anakrusidae Actinommacea** (A) Astrosphaeridae Pantanelliidae Capnodocinae Pantanelliinae Vallupinae Parvivaccidae** Acaeniotylinae Heleninae Leugeoninae Parvivaccinae** Cavaspongiidae Xiphostylidae** Stylosphaeridae Entapiidae* Actinommacea** (B) Actinommidae** Coccodiscidae Coccodiscinae Artiscinae Heliodiscidae Suttoniidae Actinommacea** (C) Conocaryommidae** Pyloniacea Dactyliosphaerilae** Patruliidae Catenopylidae Veghicycliidae Dactyliosphaeridae Hagiastridae Emiluviidae Hexaporobrachiidae Patulibracchiilae** Angulobracchiidae** Patulibracchiidae** Pseudoaulophacidae Pseudoaulophacinae** Pentapyloniinae* Tritrabidae Pyloniilae Miropylidae Pyloniidae Palaeotetrapylinae Pyloniinae Dipylissinae Pylodiscinae Larnacillilae Larnacillidae Larnacillinae Circodiscinae Cryptolarnaciinae Histriastrinae Tholoniidae Spongodiscacea Spongodiscidae Myelastridae Relindellidae Sponguracea Archaeospongoprunidae Gomberellidae** Litheliidae Phaseliformidae Pyramispongiidae** Sponguridae Oertlispongidae Collodaria Collosphaeridae Thalassosphaeridae Sphaerozoidae Entactinaria Proventocitidae
    [Show full text]
  • Radiolaria Divided Into Polycystina and Spasmaria in Combined 18S and 28S Rdna Phylogeny
    Radiolaria Divided into Polycystina and Spasmaria in Combined 18S and 28S rDNA Phylogeny Anders K. Krabberød1., Jon Bra˚te1., Jane K. Dolven4, Randi F. Ose3, Dag Klaveness1, Tom Kristensen1,3, Kjell R. Bjørklund1,2, Kamran Shalchian-Tabrizi1* 1 Microbial Evolution Research Group (MERG), Department of Biology, University of Oslo, Oslo, Norway, 2 Natural History Museum, University of Oslo, Oslo, Norway, 3 Department of Molecular Biosciences, University of Oslo, Oslo, Norway, 4 Department of Geosciences, University of Oslo, Oslo, Norway Abstract Radiolarians are marine planktonic protists that belong to the eukaryote supergroup Rhizaria together with Foraminifera and Cercozoa. Radiolaria has traditionally been divided into four main groups based on morphological characters; i.e. Polycystina, Acantharia, Nassellaria and Phaeodaria. But recent 18S rDNA phylogenies have shown that Phaeodaria belongs within Cerocozoa, and that the previously heliozoan group Taxopodida should be included in Radiolaria. 18S rDNA phylogenies have not yet resolved the sister relationship between the main Radiolaria groups, but nevertheless suggests that Spumellaria, and thereby also Polycystina, are polyphyletic. Very few sequences other than 18S rDNA have so far been generated from radiolarian cells, mostly due to the fact that Radiolaria has been impossible to cultivate and single cell PCR has been hampered by low success rate. Here we have therefore investigated the mutual evolutionary relationship of the main radiolarian groups by using the novel approach of combining single cell whole genome amplification with targeted PCR amplification of the 18S and 28S rDNA genes. Combined 18S and 28S phylogeny of sequences obtained from single cells shows that Radiolaria is divided into two main lineages: Polycystina (Spumellaria+Nassellaria) and Spasmaria (Acantharia+Taxopodida).
    [Show full text]
  • Radiolarians in the Adriatic Sea Plankton (Eastern Mediterranean)
    View metadata, citation and similar papers at core.ac.uk brought to you by CORE ISSN: 0001-5113 ACTA ADRIAT., UDC: 593.14(262.3)”1993/1995” AADRAY 53(2): 189 - 212, 2012 Radiolarians in the Adriatic Sea plankton (Eastern Mediterranean) frano kRŠINIĆ1* and Ana kRŠINIĆ2 1Institute of Oceanography and Fisheries Split, P. P. 500, Split, Croatia 2University of Zagreb, Faculty of Mining, Geology and Petroleum Engineering, Department of Mineralogy, Petrology and Mineral resources, Pierottijeva 6, 10000 Zagreb, Croatia *Corresponding author: [email protected] Samples for the study of radiolarians in the Southern Adriatic were collected during five cruises at three stations along the Dubrovnik transect (stations S-100 to S-1000) from April 1993 through February 1995. Moreover, samples were collected during 21 cruises at the deepest station, S-1000/1200, from June 2001 through December 2009. Samples were taken in 2 to 8 vertical layers with a Nansen net 53 µm equipped with a closing system. In the central part of the southern Adriatic Pit, a total of 95 radiolarian taxa were recorded: 32 species of spumellaria, 46 species of nassellaria and 17 species of phaeodaria. The present research added 49 taxa to the known radiolarian fauna of the Adriatic Sea. The most common species were the phaeodarian Challengeria xiphodon, the spumellarian Stylodictya multispina and the nassellarian Cornutella profunda, which were present in 99% of the vertical series. Radiolarians were rarely present in coastal areas and in the central Adriatic, whereas the highest abundances were recorded in the deepest parts of the south Adriatic Pit. Phaeodaria represented 20-86 % of the total average abundance.
    [Show full text]