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Chetverikov PE, Bolton SJ, Craemer C, Gankevich VD, Zhuk AS. Atypically Shaped Setae in Gall Mites (Acariformes, Eriophyoidea) and Mitogenomics of the Genus Leipothrix Keifer (Eriophyidae). Insects 2023; 14:759. [PMID: 37754727 PMCID: PMC10531682 DOI: 10.3390/insects14090759] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/16/2023] [Revised: 09/06/2023] [Accepted: 09/08/2023] [Indexed: 09/28/2023]
Abstract
The setae in Eriophyoidea are filiform, slightly bent and thickened near the base. Confocal microscopy indicates that their proximal and distal parts differ in light reflection and autofluorescence. Approximately 50 genera have atypically shaped setae: bifurcated, angled or swollen. These modifications are known in the basal part of prosomal setae u', ft', ft″, d, v, bv, ve, sc and caudal setae h2. We assessed the distribution of atypically shaped setae in Eriophyoidea and showed that they are scattered in different phylogenetic lineages. We hypothesized that the ancestral setae of eriophyoid mites were bifurcated before later simplifying into filiform setae. We also proposed that hypo-furcating setae are a synapomorphy that unites Eriophyoidea with Nematalycidae. We analyzed four new mitochondrial genomes of Leipothrix, the largest genus with bifurcated d, and showed that it is monophyletic and has a unique mitochondrial gene order with translocated trnK. We exclude Cereusacarus juniperensisn. comb. Xue and Yin, 2020 from Leipothrix and transfer five Epitrimerus spp. to Leipothrix: L. aegopodii (Liro 1941) n. comb., L. femoralis (Liro 1941) n. comb., L. geranii (Liro 1941) n. comb., L. ranunculi (Liro 1941) n. comb., and L. triquetra (Meyer 1990) n. comb.
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Affiliation(s)
- Philipp E. Chetverikov
- Zoological Institute of Russian Academy of Sciences, Universitetskaya Naberezhnaya 1, 199034 St. Petersburg, Russia;
- Department of Invertebrate Zoology, St. Petersburg State University, Universitetskaya Naberezhnaya 7/9, 199034 St. Petersburg, Russia
| | - Samuel J. Bolton
- Florida State Collection of Arthropods, Division of Plant Industry, Florida Department of Agriculture and Consumer Services, Gainesville, FL 32608, USA;
| | - Charnie Craemer
- Landcare Research, 231 Morrin Road, Auckland 1072, New Zealand;
| | - Vladimir D. Gankevich
- Zoological Institute of Russian Academy of Sciences, Universitetskaya Naberezhnaya 1, 199034 St. Petersburg, Russia;
| | - Anna S. Zhuk
- Institute of Applied Computer Science, ITMO University, 197101 St. Petersburg, Russia;
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2
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Bolton SJ, Chetverikov PE, Ochoa R, Klimov PB. Where Eriophyoidea (Acariformes) Belong in the Tree of Life. Insects 2023; 14:527. [PMID: 37367343 DOI: 10.3390/insects14060527] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/27/2023] [Revised: 05/24/2023] [Accepted: 05/26/2023] [Indexed: 06/28/2023]
Abstract
Over the past century and a half, the taxonomic placement of Eriophyoidea has been in flux. For much of this period, this group has been treated as a subtaxon within Trombidiformes. However, the vast majority of recent phylogenetic analyses, including almost all phylogenomic analyses, place this group outside Trombidiformes. The few studies that still place Eriophyoidea within Trombidiformes are likely to be biased by incomplete taxon/gene sampling, long branch attraction, the omission of RNA secondary structure in sequence alignment, and the inclusion of hypervariable expansion-contraction rRNA regions. Based on the agreement among a number of independent analyses that use a range of different datasets (morphology; multiple genes; mitochondrial/whole genomes), Eriophyoidea are almost certain to be closely related to Nematalycidae, a family of vermiform mites within Endeostigmata, a basal acariform grade. Much of the morphological evidence in support of this relationship was apparent after the discovery of Nematalycidae in the middle of the 20th century. However, this evidence has largely been disregarded until very recently, perhaps because of overconfidence in the placement of Eriophyoidea within Trombidiformes. Here, we briefly review and identify a number of biases, both molecular- and morphology-based, that can lead to erroneous reconstructions of the position of Eriophyoidea in the tree of life.
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Affiliation(s)
- Samuel J Bolton
- Florida State Collection of Arthropods, Division of Plant Industry, Florida Department of Agriculture and Consumer Services, Gainesville, FL 32608, USA
| | - Philipp E Chetverikov
- Zoological Institute of Russian Academy of Sciences, Universitetskaya nab., 1, St. Petersburg 199034, Russia
| | - Ronald Ochoa
- Agricultural Research Service, Systematic Entomology Laboratory, United States Department of Agriculture, Beltsville, MD 20705, USA
| | - Pavel B Klimov
- Department of Biological Sciences, Purdue University, West Lafayette, IN 47907, USA
- Institute of Environmental and Agricultural Biology (X-BIO), University of Tyumen, Tyumen 625003, Russia
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3
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Klimov PB, Chetverikov PE, Dodueva IE, Vishnyakov AE, Bolton SJ, Paponova SS, Lutova LA, Tolstikov AV. Symbiotic bacteria of the gall-inducing mite Fragariocoptes setiger (Eriophyoidea) and phylogenomic resolution of the eriophyoid position among Acari. Sci Rep 2022; 12:3811. [PMID: 35264574 PMCID: PMC8907322 DOI: 10.1038/s41598-022-07535-3] [Citation(s) in RCA: 15] [Impact Index Per Article: 7.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/17/2021] [Accepted: 02/17/2022] [Indexed: 12/13/2022] Open
Abstract
Eriophyoid mites represent a hyperdiverse, phytophagous lineage with an unclear phylogenetic position. These mites have succeeded in colonizing nearly every seed plant species, and this evolutionary success was in part due to the mites' ability to induce galls in plants. A gall is a unique niche that provides the inducer of this modification with vital resources. The exact mechanism of gall formation is still not understood, even as to whether it is endogenic (mites directly cause galls) or exogenic (symbiotic microorganisms are involved). Here we (i) investigate the phylogenetic affinities of eriophyoids and (ii) use comparative metagenomics to test the hypothesis that the endosymbionts of eriophyoid mites are involved in gall formation. Our phylogenomic analysis robustly inferred eriophyoids as closely related to Nematalycidae, a group of deep-soil mites belonging to Endeostigmata. Our comparative metagenomics, fluorescence in situ hybridization, and electron microscopy experiments identified two candidate endosymbiotic bacteria shared across samples, however, it is unlikely that they are gall inducers (morphotype1: novel Wolbachia, morphotype2: possibly Agrobacterium tumefaciens). We also detected an array of plant pathogens associated with galls that may be vectored by the mites, and we determined a mite pathogenic virus (Betabaculovirus) that could be tested for using in biocontrol of agricultural pest mites.
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Affiliation(s)
- Pavel B Klimov
- X-BIO Institute, Tyumen State University, Tyumen, Russia, 625003.
| | | | - Irina E Dodueva
- Saint-Petersburg State University, St. Petersburg, Russia, 199034
| | | | - Samuel J Bolton
- Florida Department of Agriculture and Consumer Services, Gainesville, FL, USA
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4
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Abstract
It is generally thought that the anterior border of the opisthosoma of acariform mites is delineated by the disjugal furrow, but there is no evidence to support this other than the superficial appearance of tagmosis in some oribatids. It is proposed herein that the disjugal furrow is an apomorphic feature that does not correspond with any segmental borders. Although the disjugal furrow is absent from Proteonematalycus wagneri Kethley, the visible body segments of this species indicate that this furrow, when present, intersects the metapodosoma. Therefore, the disjugal furrow does not delineate the anterior border of the opisthosoma. Instead, this border is between segments D and E (segments VI and VII for all arachnids). This hypothesis can be accommodated by a new model in which the proterosoma warps upwards relative to the main body axis. This model, which is applicable to all Acariformes, if not all arachnids, explains the following phenomena: 1) the location of the gnathosomal neuromeres within the idiosoma; 2) the relatively posterior position of the paired eyes; 3) the shape of the synganglion; 4) the uneven distribution of legs in most species of acariform mites with elongate bodies.
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Affiliation(s)
- Samuel J. Bolton
- Florida State Collection of Arthropods, Division of Plant Industry, Florida Department of Agriculture and Consumer Services, Gainesville, Florida, United States of America
- * E-mail:
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5
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Bolton SJ, Levin SM, Guillot T, Li C, Kaspi Y, Orton G, Wong MH, Oyafuso F, Allison M, Arballo J, Atreya S, Becker HN, Bloxham J, Brown ST, Fletcher LN, Galanti E, Gulkis S, Janssen M, Ingersoll A, Lunine JL, Misra S, Steffes P, Stevenson D, Waite JH, Yadav RK, Zhang Z. Microwave observations reveal the deep extent and structure of Jupiter's atmospheric vortices. Science 2021; 374:968-972. [PMID: 34709937 DOI: 10.1126/science.abf1015] [Citation(s) in RCA: 4] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
[Figure: see text].
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Affiliation(s)
- S J Bolton
- Southwest Research Institute, San Antonio, TX, USA
| | - S M Levin
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - T Guillot
- Université Côte d'Azur, Observatoire de la Côte d'Azur, Centre National de la Recherche Scientifique, Laboratoire Lagrange, Nice, France
| | - C Li
- Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA
| | - Y Kaspi
- Weizmann Institute of Science, Rehovot, 76100, Israel
| | - G Orton
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - M H Wong
- Carl Sagan Center for Research, SETI Institute, Mountain View, CA, USA
| | - F Oyafuso
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - M Allison
- Goddard Institute for Space Studies, New York, NY, USA.,Department of Astronomy, Columbia University, New York, NY 10027, USA
| | - J Arballo
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - S Atreya
- Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA
| | - H N Becker
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - J Bloxham
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138, USA
| | - S T Brown
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - L N Fletcher
- School of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
| | - E Galanti
- Weizmann Institute of Science, Rehovot, 76100, Israel
| | - S Gulkis
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - M Janssen
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - A Ingersoll
- Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - J L Lunine
- Department of Astronomy, Cornell University, Ithaca, NY, USA
| | - S Misra
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - P Steffes
- Department of Electrical and Computer Engineering, Georgia Institute of Technology, Atlanta, GA, USA
| | - D Stevenson
- Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - J H Waite
- Southwest Research Institute, San Antonio, TX, USA
| | - R K Yadav
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138, USA
| | - Z Zhang
- Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
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6
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Ebert RW, Greathouse TK, Clark G, Allegrini F, Bagenal F, Bolton SJ, Connerney JEP, Gladstone GR, Imai M, Hue V, Kurth WS, Levin S, Louarn P, Mauk BH, McComas DJ, Paranicas C, Szalay JR, Thomsen MF, Valek PW, Wilson RJ. Comparing Electron Energetics and UV Brightness in Jupiter's Northern Polar Region During Juno Perijove 5. Geophys Res Lett 2019; 46:19-27. [PMID: 30828110 DOI: 10.1029/2019gl084146] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/29/2018] [Revised: 12/14/2018] [Accepted: 12/20/2018] [Indexed: 05/24/2023]
Abstract
We compare electron and UV observations mapping to the same location in Jupiter's northern polar region, poleward of the main aurora, during Juno perijove 5. Simultaneous peaks in UV brightness and electron energy flux are identified when observations map to the same location at the same time. The downward energy flux during these simultaneous observations was not sufficient to generate the observed UV brightness; the upward energy flux was. We propose that the primary acceleration region is below Juno's altitude, from which the more intense upward electrons originate. For the complete interval, the UV brightness peaked at ~240 kilorayleigh (kR); the downward and upward energy fluxes peaked at 60 and 700 mW/m2, respectively. Increased downward energy fluxes are associated with increased contributions from tens of keV electrons. These observations provide evidence that bidirectional electron beams with broad energy distributions can produce tens to hundreds of kilorayleigh polar UV emissions.
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Affiliation(s)
- R W Ebert
- Southwest Research Institute San Antonio TX USA
- Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA
| | | | - G Clark
- Johns Hopkins University Applied Physics Lab Laurel MD USA
| | - F Allegrini
- Southwest Research Institute San Antonio TX USA
- Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA
| | - F Bagenal
- Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA
| | - S J Bolton
- Southwest Research Institute San Antonio TX USA
| | | | - G R Gladstone
- Southwest Research Institute San Antonio TX USA
- Department of Physics and Astronomy University of Texas at San Antonio San Antonio TX USA
| | - M Imai
- Department of Physics and Astronomy University of Iowa Iowa City IA USA
| | - V Hue
- Southwest Research Institute San Antonio TX USA
| | - W S Kurth
- Department of Physics and Astronomy University of Iowa Iowa City IA USA
| | - S Levin
- Jet Propulsion Laboratory Pasadena CA USA
| | - P Louarn
- Institut de Recherche en Astrophysique et Planétologie Toulouse France
| | - B H Mauk
- Johns Hopkins University Applied Physics Lab Laurel MD USA
| | - D J McComas
- Southwest Research Institute San Antonio TX USA
- Department of Astrophysical Sciences Princeton University Princeton NJ USA
| | - C Paranicas
- Johns Hopkins University Applied Physics Lab Laurel MD USA
| | - J R Szalay
- Department of Astrophysical Sciences Princeton University Princeton NJ USA
| | | | - P W Valek
- Southwest Research Institute San Antonio TX USA
| | - R J Wilson
- Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA
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7
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Kaspi Y, Galanti E, Hubbard WB, Stevenson DJ, Bolton SJ, Iess L, Guillot T, Bloxham J, Connerney JEP, Cao H, Durante D, Folkner WM, Helled R, Ingersoll AP, Levin SM, Lunine JI, Miguel Y, Militzer B, Parisi M, Wahl SM. Jupiter's atmospheric jet streams extend thousands of kilometres deep. Nature 2018. [PMID: 29516995 DOI: 10.1038/nature25793] [Citation(s) in RCA: 30] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
The depth to which Jupiter's observed east-west jet streams extend has been a long-standing question. Resolving this puzzle has been a primary goal for the Juno spacecraft, which has been in orbit around the gas giant since July 2016. Juno's gravitational measurements have revealed that Jupiter's gravitational field is north-south asymmetric, which is a signature of the planet's atmospheric and interior flows. Here we report that the measured odd gravitational harmonics J3, J5, J7 and J9 indicate that the observed jet streams, as they appear at the cloud level, extend down to depths of thousands of kilometres beneath the cloud level, probably to the region of magnetic dissipation at a depth of about 3,000 kilometres. By inverting the measured gravity values into a wind field, we calculate the most likely vertical profile of the deep atmospheric and interior flow, and the latitudinal dependence of its depth. Furthermore, the even gravity harmonics J8 and J10 resulting from this flow profile also match the measurements, when taking into account the contribution of the interior structure. These results indicate that the mass of the dynamical atmosphere is about one per cent of Jupiter's total mass.
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Affiliation(s)
- Y Kaspi
- Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel
| | - E Galanti
- Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel
| | - W B Hubbard
- Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721, USA
| | - D J Stevenson
- Divison of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA
| | - S J Bolton
- Southwest Research Institute, San Antonio, Texas 78238, USA
| | - L Iess
- Department of Mechanical and Aerospace Engineering, Sapienza Universita di Roma, 00184 Rome, Italy
| | - T Guillot
- Université Côte d'Azur, OCA, Lagrange CNRS, 06304 Nice, France
| | - J Bloxham
- Department of Earth and Planetary Sciences, Harvard University, Cambridge, Massachusetts 02138, USA
| | - J E P Connerney
- Space Research Corporation, Annapolis, Maryland 21403, USA.,NASA/GSFC, Greenbelt, Maryland 20771, USA
| | - H Cao
- Divison of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA.,Department of Earth and Planetary Sciences, Harvard University, Cambridge, Massachusetts 02138, USA
| | - D Durante
- Department of Mechanical and Aerospace Engineering, Sapienza Universita di Roma, 00184 Rome, Italy
| | - W M Folkner
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA
| | - R Helled
- Institute for Computational Science, Center for Theoretical Astrophysics and Cosmology, University of Zurich, 8057 Zurich, Switzerland
| | - A P Ingersoll
- Divison of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA
| | - S M Levin
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA
| | - J I Lunine
- Department of Astronomy, Cornell University, Ithaca, New York 14853, USA
| | - Y Miguel
- Université Côte d'Azur, OCA, Lagrange CNRS, 06304 Nice, France.,Leiden Observatory, University of Leiden, Leiden, The Netherlands
| | - B Militzer
- Department of Earth and Planetray Science, University of California, Berkeley, California 94720, USA
| | - M Parisi
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA
| | - S M Wahl
- Department of Earth and Planetray Science, University of California, Berkeley, California 94720, USA
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8
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Connerney JEP, Adriani A, Allegrini F, Bagenal F, Bolton SJ, Bonfond B, Cowley SWH, Gerard JC, Gladstone GR, Grodent D, Hospodarsky G, Jorgensen JL, Kurth WS, Levin SM, Mauk B, McComas DJ, Mura A, Paranicas C, Smith EJ, Thorne RM, Valek P, Waite J. Jupiter's magnetosphere and aurorae observed by the Juno spacecraft during its first polar orbits. Science 2018; 356:826-832. [PMID: 28546207 DOI: 10.1126/science.aam5928] [Citation(s) in RCA: 94] [Impact Index Per Article: 15.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/13/2016] [Accepted: 04/20/2017] [Indexed: 11/02/2022]
Abstract
The Juno spacecraft acquired direct observations of the jovian magnetosphere and auroral emissions from a vantage point above the poles. Juno's capture orbit spanned the jovian magnetosphere from bow shock to the planet, providing magnetic field, charged particle, and wave phenomena context for Juno's passage over the poles and traverse of Jupiter's hazardous inner radiation belts. Juno's energetic particle and plasma detectors measured electrons precipitating in the polar regions, exciting intense aurorae, observed simultaneously by the ultraviolet and infrared imaging spectrographs. Juno transited beneath the most intense parts of the radiation belts, passed about 4000 kilometers above the cloud tops at closest approach, well inside the jovian rings, and recorded the electrical signatures of high-velocity impacts with small particles as it traversed the equator.
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Affiliation(s)
- J E P Connerney
- Space Research Corporation, Annapolis, MD 21403, USA. .,NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - A Adriani
- Institute for Space Astrophysics and Planetology, National Institute for Astrophysics, Rome, 00133, Italy
| | - F Allegrini
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - F Bagenal
- Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA
| | - S J Bolton
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - B Bonfond
- Institut d'Astrophysique et de Geophysique, Universite de Liege, Liege, B-4000 Belgium
| | | | - J-C Gerard
- Institut d'Astrophysique et de Geophysique, Universite de Liege, Liege, B-4000 Belgium
| | - G R Gladstone
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - D Grodent
- Institut d'Astrophysique et de Geophysique, Universite de Liege, Liege, B-4000 Belgium
| | | | - J L Jorgensen
- National Space Institute, Technical University of Denmark, Kongens Lyngby, 2800, Denmark
| | - W S Kurth
- University of Iowa, Iowa City, IA 52242, USA
| | - S M Levin
- Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA 91109, USA
| | - B Mauk
- Johns Hopkins University, Applied Physics Laboratory, Laurel, MD 20723, USA
| | - D J McComas
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08544, USA
| | - A Mura
- Institute for Space Astrophysics and Planetology, National Institute for Astrophysics, Rome, 00133, Italy
| | - C Paranicas
- Johns Hopkins University, Applied Physics Laboratory, Laurel, MD 20723, USA
| | - E J Smith
- Jet Propulsion Laboratory/California Institute of Technology, Pasadena, CA 91109, USA
| | - R M Thorne
- Department of Atmospheric and Oceanic Sciences, University of California-Los Angeles, Los Angeles, CA 90095, USA
| | - P Valek
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - J Waite
- Southwest Research Institute, San Antonio, TX 78238, USA
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9
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Bolton SJ, Adriani A, Adumitroaie V, Allison M, Anderson J, Atreya S, Bloxham J, Brown S, Connerney JEP, DeJong E, Folkner W, Gautier D, Grassi D, Gulkis S, Guillot T, Hansen C, Hubbard WB, Iess L, Ingersoll A, Janssen M, Jorgensen J, Kaspi Y, Levin SM, Li C, Lunine J, Miguel Y, Mura A, Orton G, Owen T, Ravine M, Smith E, Steffes P, Stone E, Stevenson D, Thorne R, Waite J, Durante D, Ebert RW, Greathouse TK, Hue V, Parisi M, Szalay JR, Wilson R. Jupiter's interior and deep atmosphere: The initial pole-to-pole passes with the Juno spacecraft. Science 2018; 356:821-825. [PMID: 28546206 DOI: 10.1126/science.aal2108] [Citation(s) in RCA: 186] [Impact Index Per Article: 31.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/13/2016] [Accepted: 05/01/2017] [Indexed: 11/02/2022]
Abstract
On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, passing less than 5000 kilometers above the equatorial cloud tops. Images of Jupiter's poles show a chaotic scene, unlike Saturn's poles. Microwave sounding reveals weather features at pressures deeper than 100 bars, dominated by an ammonia-rich, narrow low-latitude plume resembling a deeper, wider version of Earth's Hadley cell. Near-infrared mapping reveals the relative humidity within prominent downwelling regions. Juno's measured gravity field differs substantially from the last available estimate and is one order of magnitude more precise. This has implications for the distribution of heavy elements in the interior, including the existence and mass of Jupiter's core. The observed magnetic field exhibits smaller spatial variations than expected, indicative of a rich harmonic content.
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Affiliation(s)
- S J Bolton
- Southwest Research Institute, San Antonio, TX 78238, USA.
| | - A Adriani
- Institute for Space Astrophysics and Planetology, National Institute for Astrophysics, 00133 Rome, Italy
| | - V Adumitroaie
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - M Allison
- Goddard Institute for Space Studies, New York, NY 10025, USA
| | - J Anderson
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - S Atreya
- University of Michigan, Ann Arbor, MI 48109, USA
| | - J Bloxham
- Harvard University, Cambridge, MA 02138, USA
| | - S Brown
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - J E P Connerney
- Space Research Corporation, Annapolis, MD 21403, USA.,NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
| | - E DeJong
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - W Folkner
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - D Gautier
- Laboratoire d'Études Spatiales et d'Instrumentation en Astrophysique, Observatoire de Paris, 92195 Meudon, France
| | - D Grassi
- Institute for Space Astrophysics and Planetology, National Institute for Astrophysics, 00133 Rome, Italy
| | - S Gulkis
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - T Guillot
- Université Côte d'Azur, Observatoire de la Côte d'Azur, Laboratoire Lagrange CNRS, 06304 Nice, France
| | - C Hansen
- Planetary Science Institute, Tucson, AZ 85719, USA
| | - W B Hubbard
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
| | - L Iess
- Sapienza University of Rome, 00185 Rome, Italy
| | - A Ingersoll
- California Institute of Technology, Pasadena, CA 91125, USA
| | - M Janssen
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - J Jorgensen
- National Space Institute, Technical University of Denmark, 2800 Kongens Lyngby, Denmark
| | - Y Kaspi
- Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel
| | - S M Levin
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - C Li
- California Institute of Technology, Pasadena, CA 91125, USA
| | - J Lunine
- Cornell University, Ithaca, NY 14853, USA
| | - Y Miguel
- Université Côte d'Azur, Observatoire de la Côte d'Azur, Laboratoire Lagrange CNRS, 06304 Nice, France
| | - A Mura
- Institute for Space Astrophysics and Planetology, National Institute for Astrophysics, 00133 Rome, Italy
| | - G Orton
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - T Owen
- Institute for Astronomy, University of Hawaii at Manoa, Honolulu, HI 96822, USA
| | - M Ravine
- Malin Space Science Systems, San Diego, CA 92121, USA
| | - E Smith
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - P Steffes
- Center for Space Technology and Research, Georgia Institute of Technology, Atlanta, GA 30332, USA
| | - E Stone
- California Institute of Technology, Pasadena, CA 91125, USA
| | - D Stevenson
- California Institute of Technology, Pasadena, CA 91125, USA
| | - R Thorne
- Department of Atmospheric and Oceanic Sciences, University of California, Los Angeles, CA 90095, USA
| | - J Waite
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - D Durante
- Sapienza University of Rome, 00185 Rome, Italy
| | - R W Ebert
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - T K Greathouse
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - V Hue
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - M Parisi
- Jet Propulsion Laboratory/Caltech, Pasadena, CA 91109, USA
| | - J R Szalay
- Southwest Research Institute, San Antonio, TX 78238, USA
| | - R Wilson
- Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA
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Bolton SJ, Bauchan GR, Ochoa R, Klompen H. A novel fluid-feeding mechanism for microbivory in the Acariformes (Arachnida: Acari). Arthropod Struct Dev 2015; 44:313-325. [PMID: 25958124 DOI: 10.1016/j.asd.2015.04.009] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/07/2014] [Revised: 04/27/2015] [Accepted: 04/27/2015] [Indexed: 06/04/2023]
Abstract
Low temperature scanning electron microscopy (LT-SEM) has revealed anatomical details suggesting that Osperalycus and Gordialycus (Acariformes: Nematalycidae) have an unusual feeding apparatus that is hypothesized to be specialized for feeding on the fluid contents of small microorganisms (diameter<5 μm). Both mite genera have a feeding strategy that appears to involve picking up small microorganisms and placing them onto the subcapitulum for puncturing. However, they have slightly different variants of the same basic rupturing mechanism. Whereas Gordialycus has evolved expansive and convergent rutella to hold the microorganisms in place while pushing chelicerae into them, Osperalycus has evolved a pouch into which a microorganism is inserted. The rutella reinforce this pouch while the chelicerae break up the microorganism. Both types of mouthpart apparatus seem to be adapted to minimize waste, an appropriate specialization given the organically impoverished habitats in which these mites live.
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Affiliation(s)
- Samuel J Bolton
- Acarology Laboratory, Department of Evolution, Ecology and Organismal Biology, The Ohio State University, 1315 Kinnear Rd., Columbus, OH 43212, USA.
| | - Gary R Bauchan
- Electron and Confocal Microscopy Unit, USDA, ARS, BARC-West, Bldg. 012, 10300 Baltimore Ave., Beltsville, MD 20705-2350, USA
| | - Ronald Ochoa
- Systematic Entomology Laboratory, USDA, ARS, BARC-West, Bldg. 005, 10300 Baltimore Ave., Beltsville, MD 20705-2350, USA
| | - Hans Klompen
- Acarology Laboratory, Department of Evolution, Ecology and Organismal Biology, The Ohio State University, 1315 Kinnear Rd., Columbus, OH 43212, USA
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Bolton SJ, Bauchan GR, Ochoa R, Pooley C, Klompen H. The role of the integument with respect to different modes of locomotion in the Nematalycidae (Endeostigmata). Exp Appl Acarol 2015; 65:149-161. [PMID: 25355075 PMCID: PMC4274376 DOI: 10.1007/s10493-014-9857-0] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 08/04/2014] [Accepted: 10/06/2014] [Indexed: 06/04/2023]
Abstract
Previous research on the locomotion of the Nematalycidae has only been undertaken on Gordialycus, which is by far the most elongated genus of the family. Gordialycus is dependent on an unusual form of peristalsis to move around. It was not known whether the genera of Nematalycidae with shorter bodies also used this mode of locomotion. Our videographic recordings of Osperalycus did not reveal peristalsis. Instead, this mite appears to move around the mineral regolith via the expansion and constriction of the metapodosomal and genital region, allowing greater versatility in the way that the annular regions contract and extend. This type of locomotion would enable relatively short bodied nematalycids to anchor themselves into secure positions before extending their anterior regions through tight spaces. Low-temperature scanning electron micrographs show that the short bodied genera have integumental features that appear to be associated with this mode of locomotion. Peristalsis is almost certainly a more derived form of locomotion that is an adaptation to the unusually long body form of Gordialycus.
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Affiliation(s)
- Samuel J Bolton
- Acarology Laboratory, Department of Evolution, Ecology and Organismal Biology, The Ohio State University, 1315 Kinnear Rd., Columbus, OH, 43212, USA,
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13
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Bolton SJ, Pinnion K, Marshall CV, Wilson E, Barker JE, Oreffo V, Foster ML. Changes in Clara cell 10 kDa protein (CC10)-positive cell distribution in acute lung injury following repeated lipopolysaccharide challenge in the rat. Toxicol Pathol 2008; 36:440-8. [PMID: 18420837 DOI: 10.1177/0192623308315357] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/04/2023]
Abstract
Clara cell 10 kDa protein (CC10) is the major secretory protein of Clara cells and is thought to play a protective role in the lung owing to its anti-inflammatory properties. There is little information on the anatomical distribution of CC10-positive cells in rat lung following lipopolysaccharide (LPS) challenge. We have determined the expression of CC10 along the tracheobronchial tree in saline-treated and LPS-treated rats. Saline-treated rats showed sporadic CC10 staining in central airways and abundant staining in bronchioles. In transitional airways, most cells were positive except for squamous cells. Following LPS challenge, there was a reduction in staining in the upper airways but little change within bronchioles. Squamous epithelia within the transitional airways now showed positive staining. These cells also co-stained for pancytokeratin and appeared to co-localize with surfactant D- and Ki67-positive cells, indicating the presence of a dedifferentiated cell type with both epithelial and pneumocyte phenotypes. These data show that diffuse inflammatory injury results in generalized loss of CC10 in central airways. Conversely, the transitional airways showed evidence of a dedifferentiated population of squamous cells that now stained for CC10. We hypothesize that this is an attempt by peripheral lung to maintain alveolar sac integrity during an inflammatory episode.
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Affiliation(s)
- S J Bolton
- Department of Pathology, Safety Assessment UK, AstraZeneca R&D Charnwood, Loughborough, Leicestershire LE11 5RH, United Kingdom.
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Thomas RA, Norman JC, Huynh TT, Williams B, Bolton SJ, Wardlaw AJ. Mechanical stretch has contrasting effects on mediator release from bronchial epithelial cells, with a rho-kinase-dependent component to the mechanotransduction pathway. Respir Med 2006; 100:1588-97. [PMID: 16469490 DOI: 10.1016/j.rmed.2005.12.008] [Citation(s) in RCA: 22] [Impact Index Per Article: 1.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 10/12/2005] [Accepted: 12/21/2005] [Indexed: 10/25/2022]
Abstract
INTRODUCTION In vivo, the airway epithelium stretches and relaxes with each respiratory cycle, but little is known about the effect this pattern of elongation and relaxation has on bronchial epithelial cells. We have used a model of cell deformation to measure the effect of stretch on inflammatory cytokine release by the BEAS 2B cell line, and to examine the method of mechanotransduction in these cells. METHODS BEAS 2B cells were cyclically stretched using the Flexercell system. IL-8 and RANTES protein and RNA levels were measured after different elongations, rates and duration of stretch. An inhibitor of Rho (Ras Homologous)-associated kinases was used, to assess the effect of blocking downstream of integrin signalling. Immunofluorescent staining of paxillin was used to study the effect of stretch on the distribution of focal contacts and the organisation of the actin cytoskeleton. RESULTS IL-8 release by BEAS 2B cells was increased by cytokine stimulation and stretch, whereas RANTES levels in the cell supernatant decreased after stretch in a dose-, time- and rate-dependent manner. Thirty percent elongation at 20 cycles/min for 24h increased IL-8 levels by over 100% (P < 0.01). Blocking rho kinase using Y-27632 inhibited the effect of stretch on IL-8 release by the BEAS 2B cells. Immunofluorescent staining demonstrated that stretch caused dramatic disassembly of focal adhesions and resulted in the redistribution of paxillin to the peri-nuclear region. CONCLUSION This study demonstrates a marked effect of stretch on bronchial epithelial cell function. We propose that stretch modulates epithelial cell function via the activation of rho kinases. The observation that stretch promotes focal adhesion disassembly suggests a mechanism whereby focal adhesion turnover (coordination of assembly and disassembly) is essential for mechanotransduction in bronchial epithelial cells.
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Affiliation(s)
- R A Thomas
- Institute for Lung Health, University of Leicester, UK
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Bolton SJ, Janssen M, Thorne R, Levin S, Klein M, Gulkis S, Bastian T, Sault R, Elachi C, Hofstadter M, Bunker A, Dulk G, Gudim E, Hamilton G, Johnson WTK, Leblanc Y, Liepack O, McLeod R, Roller J, Roth L, West R. Ultra-relativistic electrons in Jupiter's radiation belts. Nature 2002; 415:987-91. [PMID: 11875557 DOI: 10.1038/415987a] [Citation(s) in RCA: 97] [Impact Index Per Article: 4.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
Ground-based observations have shown that Jupiter is a two-component source of microwave radio emission: thermal atmospheric emission and synchrotron emission from energetic electrons spiralling in Jupiter's magnetic field. Later in situ measurements confirmed the existence of Jupiter's high-energy electron-radiation belts, with evidence for electrons at energies up to 20[?]MeV. Although most radiation belt models predict electrons at higher energies, adiabatic diffusion theory can account only for energies up to around 20[?]MeV. Unambiguous evidence for more energetic electrons is lacking. Here we report observations of 13.8[?]GHz synchrotron emission that confirm the presence of electrons with energies up to 50[?]MeV; the data were collected during the Cassini fly-by of Jupiter. These energetic electrons may be repeatedly accelerated through an interaction with plasma waves, which can transfer energy into the electrons. Preliminary comparison of our data with model results suggests that electrons with energies of less than 20[?]MeV are more numerous than previously believed.
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Affiliation(s)
- S J Bolton
- Jet Propulsion Laboratory/Caltech, Pasadena, California 91109, USA.
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Gurnett DA, Kurth WS, Hospodarsky GB, Persoon AM, Zarka P, Lecacheux A, Bolton SJ, Desch MD, Farrell WM, Kaiser ML, Ladreiter HP, Rucker HO, Galopeau P, Louarn P, Young DT, Pryor WR, Dougherty MK. Control of Jupiter's radio emission and aurorae by the solar wind. Nature 2002; 415:985-7. [PMID: 11875556 DOI: 10.1038/415985a] [Citation(s) in RCA: 151] [Impact Index Per Article: 6.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
Radio emissions from Jupiter provided the first evidence that this giant planet has a strong magnetic field and a large magnetosphere. Jupiter also has polar aurorae, which are similar in many respects to Earth's aurorae. The radio emissions are believed to be generated along the high-latitude magnetic field lines by the same electrons that produce the aurorae, and both the radio emission in the hectometric frequency range and the aurorae vary considerably. The origin of the variability, however, has been poorly understood. Here we report simultaneous observations using the Cassini and Galileo spacecraft of hectometric radio emissions and extreme ultraviolet auroral emissions from Jupiter. Our results show that both of these emissions are triggered by interplanetary shocks propagating outward from the Sun. When such a shock arrives at Jupiter, it seems to cause a major compression and reconfiguration of the magnetosphere, which produces strong electric fields and therefore electron acceleration along the auroral field lines, similar to the processes that occur during geomagnetic storms at the Earth.
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Affiliation(s)
- D A Gurnett
- Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242, USA.
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Bolton SJ, Jones DN, Darker JG, Eggleston DS, Hunter AJ, Walsh FS. Cellular uptake and spread of the cell-permeable peptide penetratin in adult rat brain. Eur J Neurosci 2000; 12:2847-55. [PMID: 10971627 DOI: 10.1046/j.1460-9568.2000.00171.x] [Citation(s) in RCA: 39] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022]
Abstract
Investigation of normal and pathological diseases of the central nervous system (CNS) has been hampered by the inability to effectively manipulate protein function in vivo. In order to address this important topic, we have evaluated the ability of penetratin, a novel cell-permeable peptide consisting of a 16-amino acid sequence derived from a Drosophila homeodomain protein, to act as a carrier system to introduce a cargo into brain cells. Fluorescently tagged penetratin was injected directly into rat brain, either into the striatum or the lateral ventricles, and rats were perfusion-fixed 24 h later in order to assess the brain response to the peptide. Immunohistochemistry following intrastriatal injection showed that injection of 10 microg penetratin caused neurotoxic cell death and triggered recruitment of inflammatory cells in a dose-dependent fashion. Doses of 1 microg or less resulted in reduced toxicity and recruitment of inflammatory cells, but interestingly, there was some spread of the penetratin. Injections of an inactive peptide sequence, derived from the same homeodomain, caused little toxicity but could still, however, trigger an inflammatory response. Intraventricular injections showed extensive inflammatory cell recruitment but minimal spread of either peptide. These results suggest that a dose of 1 microg of penetratin peptide is suitable for directing agents to small, discrete areas of the brain and as such is an interesting new system for analysing CNS function.
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Affiliation(s)
- S J Bolton
- Department of Neuroscience Research, SmithKline Beecham Pharmaceuticals plc, New Frontiers Science Park, Third Avenue, Harlow, Essex CM19 5AW, UK.
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Bolton SJ, Barry ST, Mosley H, Patel B, Jockusch BM, Wilkinson JM, Critchley DR. Monoclonal antibodies recognizing the N- and C-terminal regions of talin disrupt actin stress fibers when microinjected into human fibroblasts. Cell Motil Cytoskeleton 2000; 36:363-76. [PMID: 9096958 DOI: 10.1002/(sici)1097-0169(1997)36:4<363::aid-cm6>3.0.co;2-6] [Citation(s) in RCA: 34] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 02/04/2023]
Abstract
We have characterized a panel of 6 monoclonal antibodies raised against human platelet talin by Western blotting, immune precipitation, and immunofluorescence, and shown that antibodies TA205 and TD77 disrupt actin stress fibers and focal adhesions, and inhibit cell motility when microinjected into human fibroblasts. Using a series of chick talin fusion proteins spanning the entire length of the molecule, we have mapped the epitopes recognized by these antibodies to the conserved N- and C-terminal regions of the protein. TA205 bound to an epitope contained within residues 139-433, a region which overlaps an F-actin binding site, and which shows homology with the ezrin/radixin/moesin family of cytoskeletal proteins. The epitope recognized by TD77 was located within the C-terminal region of the protein (residues 2269-2541) which also contains an F-actin binding site homologous to that in the yeast actin-binding protein SIa2p. To investigate the possibility that TD77 disrupts actin stress fibers by binding directly to the C-terminal actin binding site, additional talin fusion proteins were generated and analyzed for TD77 and actin binding. Fusion proteins containing residues 2269-2541, 2304-2541, and 2304-2463 all cosedimented with F-actin, whereas TD77 did not recognize the latter fusion protein. These results show that the C-terminal actin-binding site is distinct from the region recognized by the anti-functional antibody TD77, raising the possibility that it binds to a novel functionally important ligand-binding site in the talin molecule.
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Affiliation(s)
- S J Bolton
- Department of Biochemistry, University of Leicester, United Kingdom
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Bolton SJ, Russelakis-Carneiro M, Betmouni S, Perry VH. Non-nuclear histone H1 is upregulated in neurones and astrocytes in prion and Alzheimer's diseases but not in acute neurodegeneration. Neuropathol Appl Neurobiol 1999; 25:425-32. [PMID: 10564533 DOI: 10.1046/j.1365-2990.1999.00171.x] [Citation(s) in RCA: 25] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022]
Abstract
A non-nuclear isoform of histone H1 is constitutively expressed in neurones. This protein is the major lipopolysaccharide (LPS)-binding protein in the brain. Since the major systemic LPS-binding protein is released in the liver and is an acute phase reactant, we were interested to learn whether this novel CNS histone showed altered expression following neuronal injury. We have therefore examined the changes in the expression of this molecule in acute neuronal injury and in two neurodegenerative pathologies, murine scrapie and Alzheimer's disease. No upregulation or change in H1 staining was observed in acute neurodegeneration induced by the intrastriatal injection of the glutamate antagonist N-methyl d-aspartic acid. In contrast, Western blotting indicated that histone H1 is upregulated in the brains of mice with clinical signs of scrapie. Immunohistochemistry revealed that in the regions of pathology there was increased staining for histone H1 in the neurones and the surrounding neuropil. Cells with an astrocytic appearance were also seen to stain positively for H1 but only in the regions of pathology. Immunofluorescent double staining for glial fibrillary acid protein (GFAP) and histone H1 confirmed that these cells were indeed astrocytes. Alzheimer's disease brain also showed an increase in the neuronal and astrocytic staining but only in regions of pathology. The function of histone in the CNS is unknown but the data presented here demonstrate an upregulation in areas of neuronal degeneration, which indicates that it may be involved in disease pathogenesis.
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Affiliation(s)
- S J Bolton
- CNS Inflammation Group, School of Biological Sciences, University of Southampton, Southampton, UK
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Bolton SJ, Perry VH. Differential blood-brain barrier breakdown and leucocyte recruitment following excitotoxic lesions in juvenile and adult rats. Exp Neurol 1998; 154:231-40. [PMID: 9875284 DOI: 10.1006/exnr.1998.6927] [Citation(s) in RCA: 78] [Impact Index Per Article: 3.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/24/2022]
Abstract
Acute neuronal degeneration can be induced by intracerebral injections of the glutamate receptor agonists kainic acid (KA) and NMDA (N-methyl-D-aspartate). It is accompanied by an inflammatory response that has not yet been fully investigated. We have previously demonstrated that the juvenile rat brain is more susceptible to an inflammatory challenge when compared to adult rat brain. This study set out to investigate whether this also applied to the inflammatory response associated with acute neuronal degeneration. NMDA and kainic acid were injected into the rat striatum and lesion size, leucocyte recruitment, and blood-brain barrier (BBB) breakdown were assessed after 4, 8, 12, 24, 72, and 168 h. Both NMDA and KA induced lesions of similar volume at either age and apoptotic and necrotic nuclei could be detected. NMDA induced cellular loss by 4 h, whereas KA-injected rats did not show signs of neuronal loss until 8-12 h. The inflammatory response was characterized by an infiltration of neutrophils followed by macrophages. Juvenile rats showed a greater susceptibility to leucocyte recruitment compared to adult rats. BBB breakdown in response to NMDA injection occurred in the absence of cellular recruitment at 4 h in juveniles and was significantly greater in juvenile compared to adult rats at 8 h. BBB breakdown was minimal in KA-injected animals while at 7 days an influx of serum IgG coincided with a loss of astrocytic GFAP staining within the lesion.
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Affiliation(s)
- S J Bolton
- Department of Pharmacology, University of Oxford, United Kingdom
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Bolton SJ, Anthony DC, Perry VH. Loss of the tight junction proteins occludin and zonula occludens-1 from cerebral vascular endothelium during neutrophil-induced blood-brain barrier breakdown in vivo. Neuroscience 1998; 86:1245-57. [PMID: 9697130 DOI: 10.1016/s0306-4522(98)00058-x] [Citation(s) in RCA: 271] [Impact Index Per Article: 10.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/08/2023]
Abstract
The tight junctions found between cerebral vascular endothelial cells form the basis of the blood-brain barrier. Breakdown of the blood-brain barrier is a feature of a variety of CNS pathologies that are characterized by extensive leucocyte recruitment, such as multiple sclerosis and stroke. The molecular mechanisms associated with opening of the blood-brain barrier and leucocyte recruitment in vivo are currently poorly understood. We have used an in vivo rat model to investigate the molecular response of the CNS endothelium to neutrophil adhesion and migration. Injection of interleukin-1 beta into the striatum of juvenile brains results in a neutrophil-dependent increase in vessel permeability at 4 h. Only a subset of blood vessels were associated with neutrophil recruitment. These particular vessels displayed an increase in phosphotyrosine staining, loss of the tight junctional proteins, occludin and zonula occludens-1, and apparent redistribution of the adherens junction protein vinculin. Examination of these vessels under the electron microscope indicated that the cell-cell adhesions in such vessels are morphologically different from normal junctions. This study provides the first direct evidence in vivo that leucocyte recruitment can trigger signal transduction cascades leading to junctional disorganization and blood-brain barrier breakdown. Our results have established an endothelial cell molecular profile associated with leucocyte-induced blood-brain barrier breakdown in vivo, and the relevance of different in vitro cell culture models may now be viewed more objectively.
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Affiliation(s)
- S J Bolton
- Department of Pharmacology, University of Oxford, U.K
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22
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Affiliation(s)
- V H Perry
- CNS Inflammation Group, School of Biological Sciences, University of Southampton, Bassett Crescent East, Great Britain
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23
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Abstract
Bacterial lipopolysaccharide (LPS) is a potent inflammogen following systemic infection. Macrophages express a number of surface molecules including CD14, CD18 and the scavenger receptor that are capable of recognizing and binding LPS. Injection of the CNS with LPS produces an atypical inflammatory response including a delay in the recruitment of macrophages to the brain parenchyma. We have shown using a ligand blot overlay approach, that LPS is capable of binding to histone H1 present in brain homogenate. The ability of LPS to bind to H1 has only been previously shown for monocytes. Subsequent immunohistochemistry revealed that the anti-H1 antibody, ANA-108, stained neuronal cell bodies and was located in the membrane, possibly at the cell surface. Further experiments revealed that the H1 antigen recognized by the ANA-108 antibody was not a histone wholly restricted to the nucleus but may represent a novel CNS form of the protein. This observation has implications for the autoimmune disease systemic lupus erythematosus (SLE) due to the presence of auto-antibodies, particularly against DNA and nuclear proteins, in serum. The formation of immune complexes in various organs leads to severe dysfunction. Anti-histone antibodies are typical of the auto-antibodies found in SLE serum and the presence of the H1 antigen on the surface of neurons could provide an insight into biology underlying the neurological problems associated with SLE.
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Affiliation(s)
- S J Bolton
- CNS Inflammation Group, University Department of Pharmacology, Oxford, UK
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24
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Abstract
Bacterial lipopolysaccharide (LPS) is a potent inflammogen following systemic infection. Macrophages express a number of surface molecules including CD14, CD18 and the scavenger receptor that are capable of recognizing and binding LPS. Injection of the CNS with LPS produces an atypical inflammatory response including a delay in the recruitment of macrophages to the brain parenchyma. We have shown using a ligand blot overlay approach, that LPS is capable of binding to histone H1 present in brain homogenate. The ability of LPS to bind to H1 has only been previously shown for monocytes. Subsequent immunohistochemistry revealed that the anti-H1 antibody, ANA-108, stained neuronal cell bodies and was located in the membrane, possibly at the cell surface. Further experiments revealed that the H1 antigen recognized by the ANA-108 antibody was not a histone wholly restricted to the nucleus but may represent a novel CNS form of the protein. This observation has implications for the autoimmune disease systemic lupus erythematosus (SLE) due to the presence of auto-antibodies, particularly against DNA and nuclear proteins, in serum. The formation of immune complexes in various organs leads to severe dysfunction. Anti-histone antibodies are typical of the auto-antibodies found in SLE serum and the presence of the H1 antigen on the surface of neurons could provide an insight into biology underlying the neurological problems associated with SLE.
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Affiliation(s)
- S J Bolton
- CNS Inflammation Group, University Department of Pharmacology, Oxford, UK
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25
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Abstract
The environment of the brain is controlled by a sophisticated endothelial barrier that prevents the free entry of solutes from the blood. It is commonly assumed that this blood-brain barrier (BBB) also prevents the entry of leukocytes into the central nervous system. However, recent evidence in animal models shows that this is not the case, and leukocytes can cross an intact BBB during health and disease. Indeed, in many neurological diseases, including Alzheimer's disease, prion diseases and AIDS-related dementia, leukocytes enter the brain parenchyma without concomitant BBB breakdown. Current research is concentrating on factors that control the integrity of the BBB and the mechanisms that leukocytes use to enter the brain.
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Affiliation(s)
- V H Perry
- Dept. of Pharmacology, University of Oxford U.K.
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Anthony DC, Bolton SJ, Fearn S, Perry VH. Age-related effects of interleukin-1 beta on polymorphonuclear neutrophil-dependent increases in blood-brain barrier permeability in rats. Brain 1997; 120 ( Pt 3):435-44. [PMID: 9126055 DOI: 10.1093/brain/120.3.435] [Citation(s) in RCA: 207] [Impact Index Per Article: 7.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/04/2023] Open
Abstract
In adult rats, 50,000 units of recombinant interleukin-1 beta (IL-1 beta) injected into the brain parenchyma produced an intense meningitis and disruption of the blood-CSF barrier by 4 h. No increase in vascular permeability to horseradish peroxidase or leukocyte recruitment was observed at the site of injection. By contrast, in juvenile rats, 100 units of IL-1 beta injected into the striatum gave rise to a large increase in blood-brain barrier permeability and recruitment of polymorphonuclear neutrophils into the tissue around the injection site by 4 h. This effect was also accompanied by a marked meningitis. The injection of 100 units of IL-1 beta into neonatal (2-h-old) rats gave rise to an increase in permeability of vessels to serum proteins in the meninges, but no increase in vascular permeability was observed at the injection site. The IL-1 beta-induced increases in vessel permeability in the meninges, parenchyma, and choroid plexus were polymorphonuclear neutrophil dependent, since leukocyte depletion by irradiation or polymorphonuclear neutrophil anti-serum pre-treatment eliminated the response in the juvenile animals and in the adults. Seventy-five thousand units of murine tumour necrosis factor-alpha injected into the parenchyma of both adults and juvenile animals failed to induce an increase in blood-brain barrier permeability or polymorphonuclear neutrophil recruitment, but did give rise to a mild meningitis. These findings demonstrate clear differences in the responsiveness of different CNS compartments to IL-1 beta. Furthermore, while tumour necrosis factor-alpha and IL-1 beta might have been expected to exhibit similar proinflammatory effects in the CNS, this is not the case. We also show, for the first time, that age has a significant effect on the response to a cytokine. The "window of susceptibility' to an inflammatory stimulus in juvenile rats, if paralleled in humans, may be a major factor in the increased susceptibility of children to trauma or to infectious insults to the CNS.
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Affiliation(s)
- D C Anthony
- Department of Pharmacology, University of Oxford, UK
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Hemmings L, Rees DJ, Ohanian V, Bolton SJ, Gilmore AP, Patel B, Priddle H, Trevithick JE, Hynes RO, Critchley DR. Talin contains three actin-binding sites each of which is adjacent to a vinculin-binding site. J Cell Sci 1996; 109 ( Pt 11):2715-26. [PMID: 8937989 DOI: 10.1242/jcs.109.11.2715] [Citation(s) in RCA: 171] [Impact Index Per Article: 6.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022] Open
Abstract
We have determined the sequence of chicken talin (2,541 amino acids, M(r) 271,881) which is very similar (89% identity) to that of the mouse protein. Alignments with the Caenorhabditis elegans and Dictyostelium discoideum talin sequences show that the N- and C-terminal regions of the protein are conserved whereas the central part of the molecule is more divergent. By expressing overlapping talin polypeptides as fusion proteins, we have identified at least three regions of the protein which can bind F-actin: residues 102–497, 951–1,327 and 2,269-2,541. The N-terminal binding site contains a region with homology to the ERM family of actin-binding proteins, and the C-terminal site is homologous to the yeast actin-binding protein Sla2p. Each of the actin-binding sites is close to, but distinct from a binding site for vinculin, a protein which also binds actin. The Pro1176 to Thr substitution found in talin from Wistar-Furth rats does not destroy the capacity of this region of the protein to bind actin or vinculin. Microinjection studies showed that a fusion protein containing the N-terminal actin-binding site localised weakly to stress fibres, whereas one containing the C-terminal site initially localised predominantly to focal adhesions. The former was readily solubilised, and the latter was resistant to Triton extraction. The N-terminal talin polypeptide eventually disrupted actin stress fibres whereas the C-terminal polypeptide was without effect. However, a larger C-terminal fusion protein also containing a vinculin-binding site did disrupt stress fibres and focal adhesions. The results suggest that, although both the N- and C-terminal regions of talin bind actin, the properties of these two regions of the protein are distinct.
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Affiliation(s)
- L Hemmings
- Department of Biochemistry, University of Leicester, UK
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Abstract
Plasma measurements made during the flyby of Io on 7 December 1995 with the Galileo spacecraft plasma analyzers reveal that the spacecraft unexpectedly passed directly through the ionosphere of Io. The ionosphere is identified by a dense plasma that is at rest with respect to Io. This plasma is cool relative to those encountered outside the ionosphere. The composition of the ionospheric plasmas includes O++, O+ and S++, S+, and SO2+ ions. The plasma conditions at Io appear to account for the decrease in the magnetic field, without the need to assume that Io has a magnetized interior.
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Affiliation(s)
- L A Frank
- Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242, USA
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Winder SJ, Hemmings L, Bolton SJ, Maciver SK, Tinsley JM, Davies KE, Critchley DR, Kendrick-Jones J. Calmodulin regulation of utrophin actin binding. Biochem Soc Trans 1995; 23:397S. [PMID: 8566285 DOI: 10.1042/bst023397s] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/31/2023]
Affiliation(s)
- S J Winder
- MRC Laboratory of Molecular Biology, Cambridge, UK
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30
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de Pater I, Heiles C, Wong M, Maddalena RJ, Bird MK, Funke O, Neidhoefer J, Price RM, Kesteven M, Calabretta M, Klein MJ, Gulkis S, Bolton SJ, Foster RS, Sukumar S, Strom RG, LePoole RS, Spoelstra T, Robison M, Hunstead RW, Campbell-Wilson D, Ye T, Dulk G, Leblanc Y, Lecacheux A. Outburst of Jupiter's synchrotron radiation after the impact of comet Shoemaker-Levy 9. Science 1995; 268:1879-83. [PMID: 11536723 DOI: 10.1126/science.11536723] [Citation(s) in RCA: 38] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/02/2022]
Abstract
Jupiter's nonthermal microwave emission, as measured by a global network of 11 radio telescopes, increased dramatically during the Shoemaker-Levy 9 impacts. The increase was wavelength-dependent, varying from approximately 10 percent at 70 to 90 centimeters to approximately 45 percent at 6 and 36 centimeters. The radio spectrum hardened (flattened toward shorter wavelengths) considerably during the week of impacts and continued to harden afterward. After the week of cometary impacts, the flux density began to subside at all wavelengths and was still declining 3 months later. Very Large Array and Australia Telescope images of the brightness distribution showed the enhancement to be localized in longitude and concentrated near the magnetic equator. The evidence therefore suggests that the increase in flux density was caused by a change in the resident particle population, for example, through an energization or spatial redistribution of the emitting particles.
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Affiliation(s)
- I de Pater
- Astronomy Department, University of California, Berkeley 94720, USA
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31
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Winder SJ, Hemmings L, Maciver SK, Bolton SJ, Tinsley JM, Davies KE, Critchley DR, Kendrick-Jones J. Utrophin actin binding domain: analysis of actin binding and cellular targeting. J Cell Sci 1995; 108 ( Pt 1):63-71. [PMID: 7738117 DOI: 10.1242/jcs.108.1.63] [Citation(s) in RCA: 154] [Impact Index Per Article: 5.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022] Open
Abstract
Utrophin, or dystrophin-related protein, is an autosomal homologue of dystrophin. The protein is apparently ubiquitously expressed and in muscle tissues the expression is developmentally regulated. Since utrophin has a similar domain structure to dystrophin it has been suggested that it could substitute for dystrophin in dystrophic muscle. Like dystrophin, utrophin has been shown to be associated with a membrane-bound glycoprotein complex. Here we demonstrate that expressed regions of the predicted actin binding domain in the NH2 terminus of utrophin are able to bind to F-actin in vitro, but do not interact with G-actin. The utrophin actin binding domain was also able to associate with actin-containing structures, stress fibres and focal contacts, when microinjected into chick embryo fibroblasts. The expressed NH2-terminal 261 amino acid domain of utrophin has an affinity for skeletal F-action (Kd 19 +/- 2.8 microM), midway between that of the corresponding domains of alpha-actinin (Kd 4 microM) and dystrophin (Kd 44 microM). Moreover, this utrophin domain binds to non-muscle actin with a approximately 4-fold higher affinity than to skeletal muscle actin. These data (together with those of Matsumura et al. (1992) Nature, 360, 588–591) demonstrate for the first time that utrophin is capable of performing a functionally equivalent role to that of dystrophin. The NH2 terminus of utrophin binds to actin and the COOH terminus binds to the membrane associated glycoprotein complex, thus in non-muscle and developing muscle utrophin performs the same predicted ‘spacer’ or ‘shock absorber’ role as dystrophin in mature muscle tissues. These data suggest that utrophin could replace dystrophin functionally in dystrophic muscle.
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Affiliation(s)
- S J Winder
- Medical Research Council Laboratory of Molecular Biology, Cambridge, UK
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32
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Abstract
During the Galileo flyby of Venus the plasma wave instrument was used to search for impulsive radio signals from lightning and to investigate locally generated plasma waves. A total of nine events were detected in the frequency range from 100 kilohertz to 5.6 megahertz. Although the signals are weak, lightning is the only known source of these signals. Near the bow shock two types of locally generated plasma waves were observed, low-frequency electromagnetic waves from about 5 to 50 hertz and electron plasma oscillation at about 45 kilohertz. The plasma oscillations have considerable fine structure, possibly because of the formation of soliton-like wave packets.
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Abstract
Icosahedral viral particles were found in the cytoplasm of erythrocytes and splenic reticular cells of a marine toad (Bufo marinus) collected from Costa Rica. Capsids had a maximum diameter of 312 nm and a spherical core with biphasic electron density. Viruses in erythrocytes were associated with cytoplasmic assembly areas and vacuoles in cytoplasm. Nuclei had finely granular material of decreased electron density located centrally, but contained no viral particles. A group of unenveloped viral particles was seen extracellularly in a splenic vessel. The virus was consistent with an iridovirus. In a blood smear stained with Giemsa round basophilic bodies with average diameters of 1.70 microns and morphologically similar to Pirhemocyton sp. were seen in the cytoplasm of erythrocytes and occasionally in the cytoplasm of monocytes or extracellularly. Erythrocytes containing these bodies had vacuoles and irregular pale-staining areas in the cytoplasm and pale-staining areas in the nucleus. These changes corresponded to the viral particles, assembly areas, vacuoles and nuclear changes at the ultrastructural level.
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Affiliation(s)
- R Speare
- Graduate School of Tropical Veterinary Science and Agriculture, James Cook University of North Queensland, Townsville, Australia
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