Journal articles: 'Ionien'

1

Gürler, Binnur. ""Ephesos-Lampen" aus Metropolis/Ionien." Jahreshefte des Österreichischen Archäologischen Institutes in Wien 1, no. 71 (2003): 133. http://dx.doi.org/10.1553/oejh71s133.

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2

Blanc, Alain. "L’adjectif ionien ἀντίξοος et la résistance active." Revue des Études Grecques 123, no. 1 (2010): 1–27. http://dx.doi.org/10.3406/reg.2010.8000.

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3

BYVANCK-QUARLES VAN UFFORD, L. "'Achämenidischer Becher' ou 'bol ionien à panse arrondie'?" BABESCH - Bulletin Antieke Beschaving 66 (January 1, 1991): 159–63. http://dx.doi.org/10.2143/bab.66.0.2005986.

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4

Ruzé, Françoise. "Le style ionien dans la vie politique archaïque." Revue des Études Anciennes 87, no. 1 (1985): 157–67. http://dx.doi.org/10.3406/rea.1985.4200.

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5

Dubois, Laurent. "Le nom d’une taxe portuaire en grec ionien." Revue des Études Grecques 127, no. 2 (2014): 603–8. http://dx.doi.org/10.3406/reg.2014.8358.

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6

Masson, Olivier. "Le culte ionien d'Apollon Oulios, d'après des données onomastiques nouvelles." Journal des savants 3, no. 1 (1988): 173–83. http://dx.doi.org/10.3406/jds.1988.1514.

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7

Lejeune, Michel, Jean Pouilloux, and Yves Solier. "Etrusque et ionien archaïques sur un plomb de Pech Maho (Aude)." Revue archéologique de Narbonnaise 21, no. 1 (1988): 19–59. http://dx.doi.org/10.3406/ran.1988.1323.

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8

Lorenzi, Marianne. "L’Uscoque de George Sand : les réécritures vénitiennes d’un pirate ionien du." Cahiers d’études italiennes, no. 21 (November 5, 2015): 197–207. http://dx.doi.org/10.4000/cei.2764.

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9

Minon, Sophie. "De Babylone à l’Occident méditerranéen : le nom d’homme hellénisé sous la forme Ζώπυρος." Cahiers du Centre de Linguistique et des Sciences du Langage, no. 60 (February 24, 2020): 225–38. http://dx.doi.org/10.26034/la.cdclsl.2020.197.

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En amical hommage à Rudolf Wachter, ces quelques réflexions ont pour point de départ la base Zωπυρ°, créatrice d’anthroponymes fort à la mode aux époques tardo-hellénistique et impériale : au total, près de mille individus répertoriés dans la base de données en ligne lgpn2 du Lexicon of Greek Personal Names d’Oxford,1 qui portent en majorité le nom masculin Ζώπυρος (719), au féminin, Ζωπύρᾱ (65x,2 sans attestation de l’équivalent ionien *Ζωπύρη), Ζωπυρίων venant en deuxième en terme de fréquence (100+, ≥ 4a).3 Il s’agira de tenter d’élucider quelques-unes des motivations de la popularité du premier de ces noms.

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10

Jones, C. P. "ἕθνος and γνος in Herodotus." Classical Quarterly 46, no. 2 (December 1996): 315–20. http://dx.doi.org/10.1093/cq/46.2.315.

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Herodotus has often been considered the Father of Ethnography no less than the Father of History. It comes as a paradox, then, that he has been taxed with confusion in his use of two terms that recur over and over in his discussion of peoples, ἕθνος and γνος. Here is the formulation of Raymond Weil:Hérodote definit mal l‘ethnos’. C'est pour lui tantôot une subdivision du ‘génos’, tantôt au contraire un ensemble de ‘géné’. Ainsi 1' ‘ethnos’ des Médes, comme celui des Scythes, groupe plusieurs γνεα. Mais cet ‘ethnos’ scythe porte aussi le nom de ‘génos’, et comprend des ἕθνεα. Les Athéniens sont un ‘ethnos’ hellénique qui fait partie du ‘génos’ ionien, les Lacédémoniens un ‘ethnos’ pélasgique à rattacher au ‘génos’ dorien.

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11

MÜLLER, Lukas, Christina Erika SPONSEL, and Boris DREYER. "Die Einwohner der Stadt Metropolis in Ionien ehren Stadthalter der Provinz oder Mitglieder ihrer Familien." Gephyra 24 (November 15, 2022): 33–37. http://dx.doi.org/10.37095/gephyra.1141261.

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Zwei Funde aus Metropolis im Jahr 2022 bieten Einblicke in die Beziehung der Kleinstadt zu ihren Provinzstatthaltern aus der späten Republik und der frühen Kaiserzeit. Die Stadt gelangte trotz erheblicher Zerstörungen in den mithridatischen Kriegen (s. Inschrift 1) zu neuerlicher Prosperität und stattete den neuen Machthabern dafür reichlich Dank ab. Dabei hat in der ersten Inschrift der Prokonsul Gaius Fabius, soweit erkennbar, mit seinen Wohltaten die gesamte Provinz beglückt. In der zweiten Inschrift ist es ein Mitglied der Familie (die Tochter) des Stadthalters, die sich der Stadt gegenüber als wohltätig erweist und dafür geehrt wird.

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12

Del Favero, C. "Effetti secondari comparati dei mezzi di contrasto ionici e non ionici." Rivista di Neuroradiologia 1, no. 2 (August 1988): 161–64. http://dx.doi.org/10.1177/197140098800100206.

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Vengono presentati i risultati relativi alle reazioni avverse dei mezzi di contrasto ionici e non ionici introdotti per via venosa in 34.928 pazienti. L'incidenza delle reazioni avverse è stata dell '11.47% con il mezzo di contrasto ionico e 2.1% con il mezzo di contrasto non ionico. Si è notato un incremento di rischio per i soggetti con anamnesi allergica. Le reazioni avverse sono state prevalentemente minori e moderate mentre le gravi sono state più frequenti con il mezzo di contrasto ionico. Complessivamente i mezzi di contrasto non ionici diminuiscono l'incidenza delle reazioni avverse da 1 a 5–8 volte rispetto ai contrasti ionici.

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13

Escarmed, Groupe, S. Charier, B. Biju-Duval, Y. Morel, and S. Rossi. "L'escarpement Apulien et le promontoire de Céphalonie : marge septentrionale du bassin Ionien (synthèse des données des campagnes à la mer Escarmed)." Revue de l'Institut Français du Pétrole 43, no. 4 (July 1988): 485–515. http://dx.doi.org/10.2516/ogst:1988030.

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14

Glushkova, Svetla. "The Septinsular Republic: The First Greek State in Revolutionary Europe." Epohi 30, no. 2 (December 19, 2022): 230–41. http://dx.doi.org/10.54664/bdcv9978.

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The Greek-inhabited Ionian islands were key in Mediterranean trade. They came under Venetian rule at the end of the 14th century. The Ionians lived in a stratified society enjoying personal freedoms, brought together by their Orthodox religion. At the end of the 18th century, the Ionian islands were dragged into the complex political relations between the big countries in Europe and the Ottoman Empire. In June 1797, the islands were occupied by the French army, but soon after that, they came under Russo-Ottoman protection. A republic with a moderate constitution was established, which was later replaced by one after a Venetian model, retaining noble titles and privileges.

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15

Weidlich, Michael. "Zur Schmetterlingsfauna der Ionischen Inseln Griechenlands mit der Beschreibung neuer Psychiden-Taxa sowie ein Beitrag zu ihrer Köcherfliegenfauna (Lepidoptera, Trichoptera)." Beiträge zur Entomologie = Contributions to Entomology 66, no. 2 (December 20, 2016): 265–320. http://dx.doi.org/10.21248/contrib.entomol.66.2.265-320.

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Der Autor führte insgesamt 8 Exkursionen zu den Ionischen Inseln in Griechenland durch. Zwei neue Psychidenarten, Bankesia cephalonica spec. nov. und Reisseronia ionica spec. nov. sowie zwei neue Unterarten Reisseronia ionica odysseus subspec. nov. und Reisseronia ionica lefkadensis subspec. nov. werden beschrieben und mit verwandten Arten verglichen. Das erste Taxon wurde im Nationalpark „Enos“ auf Kefalonia auf 1600 m NN entdeckt, R. ionica spec. nov. kommt auf Kefalonia, odysseus subspec. nov. auf Ithaka und lefkadensis subspec. nov auf Lefkada vor. Die Taxa von Reisseronia sind auf den Inseln weit verbreitet und stellenweise häufig. Während der Jahre 1993, 2000, 2001, 2002, 2003, 2005, 2012 und 2015 wurde ihre Biologie und Ökologie studiert. Weiterhin wird der Kenntnisstand zur Lepidopterenfauna der Ionischen Inseln recherchiert und umfassend diskutiert. Im Ergebnis werden 638 Lepidopterenarten bekanntgegeben. Darunter befindet sich eine Art, deren Erstnachweis für Europa mitgeteilt wird und zwei Arten als neu für Griechenland genannt. Für weitere 105 Arten wird deren Erstnachweis für die Ionischen Inseln bekannt gemacht. Ausserdem werden die Beifänge zur Köcherfliegenfauna veröffentlicht.StichwörterGreece, Ionian Islands, Bankesia cephalonica spec. nov., Reisseronia ionica spec. nov., Reisseronia ionica odysseus subspec. nov., Reisseronia ionica lefkadensis subspec. nov., Psychidae, Lepidoptera, Trichoptera.

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16

Baliousis, Evagelos. "Flora and Vegetation of the Island of Kalamos (Ionian Sea, Greece) – Floristic Analysis and Phytogeographical Aspects." Hacquetia 14, no. 2 (December 1, 2015): 307–18. http://dx.doi.org/10.1515/hacq-2015-0002.

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Abstract The floristic investigation of the Ionian island of Kalamos resulted in the addition of 275 specific and infraspecific taxa, which are reported here, to a present total of 502 taxa. For each newly recorded taxon local distribution and habitat types are presented. Convolvulus pentapetaloides and Malcolmia graeca subsp. hydraea are reported for the first time from the Ionian islands. Some of the new records concern rare taxa in Greece or regional endemics, which are, therefore, chorologically significant, such as Alkanna corcyrensis, Stachys ionica, Heptaptera colladonioides. A brief description of some of the vegetation types of the island is given. The results of floristic analysis and phytogeographical aspects demonstrate the pronounced Mediterranean character of the island’s flora.

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17

Groupe, Escarmed, S. Charier, Y. Morel, B. Biju-Duval, and V. Renard. "L'Escarpement de Malte, le mont Alfeo et les monts de Médine: marges anciennes du bassin Ionien (synthèse des données des campagnes a la mer Escarmed)." Revue de l'Institut Français du Pétrole 42, no. 6 (November 1987): 695–745. http://dx.doi.org/10.2516/ogst:1987041.

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18

Greaves, Alan M. "Frühes Ionien: Eine Bestandsaufnahme. Panionion-Symposium Güzelçamli, 26 September-1 Oktober 1999. By Justus Cobet, Volkmar von Graeve, Wolf-Dietrich Niemeier, and Konrad Zimmerman." American Journal of Archaeology 112, no. 3 (July 1, 2008): 552–53. http://dx.doi.org/10.1086/ajs20627498.

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19

McIntyre, V. J. "Neutral and Ionised Hydrogen in NGC 4214." Publications of the Astronomical Society of Australia 15, no. 1 (1998): 157–58. http://dx.doi.org/10.1071/as98157.

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AbstractIt is not clear at present how the diffuse ionised gas (DIG) component in galaxies is ionised. The leading hypothesis is that ultraviolet photons from star clusters are responsible, but this requires a rather porous interstellar medium if the photons are to travel the large distances (≥ 1 kpc) between the bright clusters and diffuse-emission regions. To examine this hypothesis, we present high-resolution VLA observations of the neutral hydrogen in the Magellanic galaxy NGC 4214, and compare them with an Hα image. The data appear consistent with the idea that enough UV photons escape from supergiant H II regions to ionise the DIG.

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20

Ivanov, Igor, and Oksana Ivanova. "Mathematical Modeling of Charge Transfer Processes in Polymeric Ionites During the Water Vapor Sorption." EPJ Web of Conferences 224 (2019): 03001. http://dx.doi.org/10.1051/epjconf/201922403001.

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Based on a thermodynamic approach, a mathematical model of charge transfer processes in the polymeric ionites (ion-exchange materials) during the water vapor sorption was developed. Theoretical dependences of the resistance of a polymeric ionite on the relative air humidity over the range 10-100% at physically reasonable values of the parameters of the system were obtained. The comparison of theoretical and experimental dependences has been performed. Possible reasons for and criteria of the phase transitions that lead to stepwise change of ionite resistance were discussed. The developed mathematical model adequately describes the available experimental data and allows formulating practical recommendations on selecting optimal polymeric coatings for the electrode units of molecular-electronic humidity gauges.

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21

Givi Papava, Marina Gurgenishvili, Ia Chitrekashvili, Eter Gavashelidze, and Gelashvili Nazi. "IONITES ON THE BASIS OF CLINOPTILOLITE." International Academy Journal Web of Scholar, no. 10(40) (October 31, 2019): 39–41. http://dx.doi.org/10.31435/rsglobal_wos/31102019/6740.

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Organomineral ionites have been synthesized, in which natural mineral sorbent is chemically bound to organic part of a molecsule, containing ionogen groups. Ionogen groups of these ionites contribute to efficient exchange in water solutions. They might be used for cleaning drainage waters and technical solutions, as well as for purification of medicinal preparations from various admixes. Hydrogen forms of natural zeolite - clinoptilolite and bromoacetic acid were used to resolve this problem. Chemical modification of clinoptilolite, by inculcation of ionogen groups into zeolite skeleton, enables us to increase significantly ionite exchange capacity. Static exchange capacity of a cationite with carboxyl ionogen groups increases from 0,1 - 0,9 (for chemically unmodified zeolite) to 5- 6 мg.equiv./g.

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22

Sarropoulou, Virginia, and Eleni Maloupa. "Asexual Propagation of Four Medicinal Greek Endemic Plants of Lamiaceae Family With Conservation Priority From The Collection of The Balkan Botanic Garden of Kroussia, N. Greece." JOURNAL OF ADVANCES IN AGRICULTURE 10 (January 31, 2019): 1611–22. http://dx.doi.org/10.24297/jaa.v10i0.8039.

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Conservation of endemic rare-threatened plants and sustainable exploitation of biodiversity with emphasis on medicinal-aromatic plants and plants with horticultural/ornamental value can be achieved through ex situ conservation activities. For this purpose, propagation experiments with cuttings were performed on four local Ionian endemic species with conservation priority, Stachys ionica Halácsy, Teucrium halascyanum, Thymus holosericeus Celak and Thymus plasonii Adamovic (all Lamiaceae). For propagation, softwood tip cuttings (3-5 cm) were cut at early autumn from mother plants collected from the wild and maintained in open-air mother plantations. For experimentation, the base of cuttings was immersed for 1 min in solutions of four concentrations of IBA (0, 1000, 2000 and 4000 ppm). Cuttings were placed on a peat:perlite (1:3) substrate in the bench of greenhouse heated mist system. Most suitable treatment for T. halascyanum (3 ½ weeks) proved to be 1000 ppm IBA (32.13 roots 1.72 cm long, 100% rooting). Accordingly, 2000 ppm IBA gave 100% rooting for both S. ionica (28.5 roots 1.56 cm long,) (3 weeks) and Th. holosericeus (4.4 roots 1.76 cm long) (7 weeks). T. plasonii cuttings treated with 2000 ppm IBA gave 85.71% optimum rooting with 8.67 roots 1.78 cm long.

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Walterbos, René A. M. "The Warm Ionised Medium in Spiral Galaxies: A View from Above." Publications of the Astronomical Society of Australia 15, no. 1 (1998): 99–102. http://dx.doi.org/10.1071/as98099.

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AbstractThe warm ionised medium (WIM), also referred to as diffuse ionised gas (DIG), contains most of the mass of interstellar medium in ionised form, contributing as much as 30% of the total atomic gas mass in the solar neighborhood. The advent of CCDs has enabled unprecedented study of this medium in external galaxies, probing a variety of environments. In particular, we can derive the morphology of the WIM, its distribution across disks, and the correlation with other Population I material. Spectroscopy of the WIM makes it possible to test various ionisation models. I will review here our current understanding of the properties of the WIM in spiral galaxies. A perhaps unexpected result is that the Hα emission from the WIM contributes about 40% of the total observed Hα luminosity from spirals. This places severe constraints on possible sources of ionisation, since only photoionisation by OB stars meets this requirement. Spectroscopic measurements of forbidden line strengths appear in reasonable agreement with photoionisation models. It is not yet clear if the Lyman continuum photons that ionise the WIM are mostly from OB stars located inside traditional HII regions, or from field OB stars.

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Bareka, Pepy, Georgia Kamari, and Dimitrios Phitos. "Acis ionica (Amaryllidaceae), a new species from the Ionian area (W Greece, S Albania)." Willdenowia 36, no. 1 (February 27, 2006): 357–66. http://dx.doi.org/10.3372/wi.36.36131.

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25

Oey, M. S., and R. C. Kennicutt. "LMC HII Region Luminosities versus Observed Ionising Stars." Publications of the Astronomical Society of Australia 15, no. 1 (1998): 141–43. http://dx.doi.org/10.1071/as98141.

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AbstractWe use the stellar census of OB associations in the Large Magellanic Cloud (LMC) to predict the Hα luminosities of the host HII regions, based on results from stellar atmosphere models. These values are compared to the observed HII region luminosities, yielding an estimate for the mean fraction of H-ionising photons that escape the local nebulae in this sample. We formally estimate that, overall, 0–51% of the ionising radiation escapes the local HII regions and is available to ionise the warm, ionised medium in the LMC. We find both nebulae that appear to be density-bounded and ones that appear to be radiation-bounded.

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26

Stankevič, Jolita, Aistė Audickaitė, Simona Šilovė, Valdas Šimčikas, Henrikas Cesiulis, Grita Skujienė, Virginija Bukelskienė, Violeta Žalgevičienė, and Janina Tutkuvienė. "EFFECT OF IONISED (ELECTROLYSED) WATER ON THE RAT EMBRYO DEVELOPMENT." Journal of Environmental Engineering and Landscape Management 28, no. 1 (January 24, 2020): 28–35. http://dx.doi.org/10.3846/jeelm.2020.11831.

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The aim of this study was to investigate the effects ionised water has on embryonic development using Wistar rat animal model. For that purpose, alkaline and acidic water was prepared with a domestic water ioniser. It was found that the concentrations of Cl–, SO42– ions increased in acidic water, while in alkaline water, Ca2+ concentration decreased and halogenated hydrocarbon concentrations exceeded permitted levels. The animals were given test alkaline and acidic water, as well as tap water as control. After three months, female rats were mated. On the 21st day of gestation, they were euthanized and subjected to Caesarean sections; the number of live and dead fetuses was recorded. The fetuses were examined for external or visceral malformations and skeletal abnormalities. The data showed that embryo death was higher in acidic and alkaline experimental groups in comparison to the control group. The fetuses in both test groups were significantly shorter than in the control group. Long bones of fetal hind and front limbs were shorter in the acidic group in comparison to the control group. Retardation of limb osteogenesis was expressed in the acidic group fetuses. Therefore, in our model, ionised water had a negative effect on the embryonic development.

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Ciaranfi, Neri. "The GSSP of “Ionian” Stage (Early-Middle Pleistocene boundary) at the Montalbano Ionico section (Southern Italy)." Quaternary International 279-280 (November 2012): 90. http://dx.doi.org/10.1016/j.quaint.2012.07.394.

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Karakitsios, V., M. Roveri, S. Lugli, V. Manzi, R. Gennari, A. Antonarakou, M. Triantaphyllou, K. Agiadi, and G. Kontakiotis. "Remarks on the Messinian evaporites of Zakynthos Island (Io- nian Sea, Eastern Mediterranean)." Bulletin of the Geological Society of Greece 47, no. 1 (December 21, 2016): 146. http://dx.doi.org/10.12681/bgsg.10915.

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Detailed mapping of the Neogene deposits on Zakynthos Island shows that the Messinian primary evaporite basins, formed over Ionian basement, are delimited by the westernmost outcrop of the Triassic evaporitic diapirs, located west of the Kalamaki-Argasi Messinian gypsum unit. The post-Miocene external Ionian thrust is emplaced west of the Triassic diapirs. Planktonic foraminifera biostratigraphy indicates that primary evaporite accumulation took place probably during the first stage of the Messinian salinity crisis (5.96-5.60 Ma), in shallower parts of a foreland basin, formed over the Pre-Apulian and the Ionian zone basement. Establishment of these depositional environments, before the Ionian thrust emplacement, was probably due to the particularities of the foreland basin, which extended from the external Ionian to the internal Pre-Apulian zone. Field observations, borehole data and an onshore seismic profile show that the Neogene sediments over the Pre-Apulian basement correspond to the foredeep through forebulge domain of the foreland basin, as it is documented from their spatial thickness distribution. In contrast, the Neogene sediments over the Ionian basement correspond to the wedge top of the foreland basin, which was less subsiding, as it is deduced by their reduced thickness. This lower subsidence rate was the result of the concurrent diapiric movements of the Ionian Triassic evaporites. In Agios Sostis area, located over Pre-Apulian basement, the Neogene sequence is intercalated by decametre-thick resedimented blocks consisting of shallow water selenite. To the southeast, this mass-wasting Messinian gypsum passes to mainly gypsum turbidite. In Kalamaki-Argasi area, located over Ionian basement, the shallow water environment led to the deposition of the observed primary gypsum. Erosion of the primary gypsum of both forebulge and wedge top supplied the foreland basin’s depocenter with gypsum turbidites.

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Ciocan, B. I., B. L. Ziegler, M. Verdugo, P. Papaderos, K. Fogarty, M. Donahue, and M. Postman. "The VLT-MUSE and ALMA view of the MACS 1931.8-2635 brightest cluster galaxy." Astronomy & Astrophysics 649 (May 2021): A23. http://dx.doi.org/10.1051/0004-6361/202040010.

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We reveal the importance of ongoing in situ star formation in the brightest cluster galaxy (BCG) in the massive cool-core CLASH cluster MACS 1931.8-2635 at a redshift of z = 0.35 by analysing archival VLT-MUSE optical integral field spectroscopy. Using a multi-wavelength approach, we assessed the stellar and warm ionised medium components, which were spatially resolved by the VLT-MUSE spectroscopy, and linked them to the molecular gas by incorporating sub-mm ALMA observations. We measured the fluxes of strong emission lines such as: [O II] λ3727, Hβ, [O III] λ5007, Hα, [N II] λ 6584, and [S II] λ6718, 6732, which allowed us to determine the physical conditions of the warm ionised gas, such as electron temperature, electron density, extinction, ionisation parameter, (O/H) gas metallicities, star formation rates, and gas kinematics, as well as the star formation history of the system. Our analysis reveals the ionising sources in different regions of the galaxy. The ionised gas flux brightness peak corresponds to the location of the supermassive black hole in the BCG and the system shows a diffuse warm ionised gas tail extending 30 kpc in the north-east direction. The ionised and molecular gas are co-spatial and co-moving, with the gaseous component in the tail likely falling inward, providing fuel for star formation and accretion-powered nuclear activity. The gas is ionised by a mix of star formation and other energetic processes which give rise to LINER-like emission, with active galactic nuclei emission dominant only in the BCG core. We measured a star formation rate of ∼97 M⊙ yr−1, with its peak at the BCG core. However, star formation accounts for only 50–60% of the energetics needed to ionise the warm gas. The stellar mass growth of the BCG at z < 0.5 is dominated either by in situ star formation generated by thermally unstable intracluster medium cooling or by dry mergers, with these mechanisms accounting for the build-up of 20% of the stellar mass of the system. Our measurements reveal that the most central regions of the BCG contain the lowest gas-phase oxygen abundance, whereas the Hα arm exhibits slightly more elevated values, suggesting the transport of gas out to large distances from the centre as a result of active galactic nuclei outbursts. The galaxy is a dispersion-dominated system that is typical for massive, elliptical galaxies. The gas and stellar kinematics are decoupled, with the gaseous velocity fields being more closely related to the bulk motions of the intracluster medium.

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Gačić, M., G. Civitarese, V. Kovačević, L. Ursella, M. Bensi, M. Menna, V. Cardin, et al. "Extreme winter 2012 in the Adriatic: an example of climatic effect on the BiOS rhythm." Ocean Science 10, no. 3 (June 23, 2014): 513–22. http://dx.doi.org/10.5194/os-10-513-2014.

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Abstract. Adriatic and Ionian seas are Mediterranean sub-basins linked through the Bimodal Oscillating System mechanism responsible for decadal reversals of the Ionian basin-wide circulation. Altimetric maps showed that the last cyclonic mode started in 2011 but unexpectedly in 2012 reversed to anticyclonic. We related this "premature" inversion to the extremely strong winter in 2012, which caused the formation of very dense Adriatic waters, flooding Ionian flanks in May and inverting the bottom pressure gradient. Using Lagrangian float measurements, the linear regression between the sea surface height and three isopycnal depths suggests that the southward deep-layer flow coincided with the surface northward geostrophic current and the anticyclonic circulation regime. Density variations at depth in the northwestern Ionian revealed the arrival of Adriatic dense waters in May and maximum density in September. Comparison between the sea level height in the northwestern Ionian and in the basin centre showed that in coincidence with the arrival of the newly formed Adriatic dense waters the sea level was lowered in the northwestern flank, inverting the surface pressure gradient. Toward the end of 2012, the density gradient between the basin flanks and its centre went to zero, coinciding with the weakening of the anticyclonic circulation and eventually with its return to the cyclonic pattern. Thus, the premature and transient reversal of Ionian surface circulation originated from the extremely harsh winter in the Adriatic, resulting in the formation and spreading of highly dense bottom waters. The present study highlights the remarkable sensitiveness of the Adriatic–Ionian BiOS to climatic forcing.

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Gačić, M., G. Civitarese, V. Kovačević, L. Ursella, M. Bensi, M. Menna, V. Cardin, et al. "Extreme winter 2012 in the Adriatic: an example of climatic effect on the BiOS rhythm." Ocean Science Discussions 11, no. 1 (February 3, 2014): 425–52. http://dx.doi.org/10.5194/osd-11-425-2014.

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Abstract. Adriatic and Ionian Seas are Mediterranean sub-basins linked through the Bimodal Oscillating System mechanism responsible for decadal reversals of the Ionian basin-wide circulation. Altimetric maps showed that the last cyclonic mode started in 2011 but unexpectedly in 2012 reversed to anticyclone. We related this "premature" inversion to extremely strong winter in 2012, which caused the formation of very dense Adriatic waters, flooding Ionian flanks in May and inverting the bottom pressure gradient. Using Lagrangian float measurements, the linear regression between the sea surface height and three isopycnal depths suggests that the southward deep-layer flow coincided with the surface northward geostrophic current and the anti-cyclonic circulation regime. Density variations at depth in the north-western Ionian revealed the arrival of Adriatic dense waters in May and maximum density in September. Comparison between the sea level height in the north-western Ionian and in the basin centre showed that in coincidence with the arrival of the newly formed Adriatic dense waters the sea level lowered in the north-western flank inverting the surface pressure gradient. Toward the end of 2012, the density gradient between the basin flanks and its centre went to zero, coinciding with the weakening of the anticyclonic circulation and eventually with its return to the cyclonic pattern. Thus, the premature and transient reversal of Ionian surface circulation originated from the extremely harsh winter in the Adriatic, resulting in the formation and spreading of highly dense bottom waters. The present study highlights the remarkable sensitiveness of the Adriatic–Ionian BiOS to climatic forcing.

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Hill, David S., Stuart B. Kamenetsky, and Sandra E. Trehub. "Relations among Text, Mode, and Medium: Historical and Empirical Perspectives." Music Perception 14, no. 1 (1996): 3–21. http://dx.doi.org/10.2307/40285707.

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We examined, by historical and empirical means, relations among text (positive, negative), mode (Ionian, Phrygian), and medium (organ, vocal) in settings of a popular Christian melody from the baroque era. A descriptive analysis of 51 representative settings indicated that baroque composers tended to link Ionian settings of the melody to a "salvation" text and Phrygian settings to a "condemnation" text. They also set vocal pieces more frequently in the Ionian mode and organ pieces in the Phrygian mode. A series of experiments confirmed that contemporary adult and child listeners linked reward texts to the Ionian mode and punishment texts to the Phrygian mode, with the internal cadence structure of the settings affecting such links. Moreover, adult listeners associated these texts differentially with organ and vocal settings.

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Civitarese, G., M. Gačić, M. Lipizer, and G. L. E. Borzelli. "On the impact of the Bimodal Oscillating System (BiOS) on the biogeochemistry and biology of the Adriatic and Ionian Seas (Eastern Mediterranean)." Biogeosciences Discussions 7, no. 5 (September 14, 2010): 6971–95. http://dx.doi.org/10.5194/bgd-7-6971-2010.

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Abstract. Analysis of 20-year time-series of the vertically averaged salinity and nutrient data in the South Adriatic shows that the two parameters are subject to strong decadal variability. In addition, nutrient and salinity variations are out of phase. Nutrients in the Ionian and in the Adriatic vary in parallel except that often the nutrient content in the Adriatic is lower than in the Ionian, a fact that has been attributed to primary producer consumption following the winter convective mixing. Horizontal distribution of the nitracline depth in the Ionian suggests that nutrient content in the Adriatic is a function of the circulation pattern in the Ionian that wells up or wells down the nitracline: cyclonic circulation causes a downwelling of the nitracline along the borders of the Northern Ionian Gyre (NIG) and a decrease in the nutrient content of the water flowing into the Adriatic across the Otranto Strait, and vice versa. The circulation variations are due to the Bimodal Oscillating System, i.e. the feedback mechanism between the Adriatic and Ionian. Inversion of the sense of the NIG results in the advection of Modified Atlantic Water or of the Levantine/Eastern Mediterranean (EMed) waters in the Adriatic. Here, we show that the presence of allochtonous organisms from Atlantic/Western Mediterranean (WMed) and EMed/temperate zone in the Adriatic are concomitant with the anticyclonic and cyclonic circulations, respectively, of the NIG. As a consequence of the NIG inversions, in the Ionian, this highly oligotrophic zone shows annual blooms in its central area only during cyclonic circulation. On the basis of the results presented, a revision of the theory of Adriatic ingressions formulated in the early 1950s is proposed.

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Minas, Adamantios Dionysios. "The Suppression of the Music of Ionian Islands by the Modern Greek State: Culture that did not Fit the Political Agenda." Public Voices 9, no. 1 (January 5, 2017): 125. http://dx.doi.org/10.22140/pv.207.

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Music plays an important role in social integration, often providing the vehicle for how one culture reinterprets itself in another. However, as in the case of the Ionian Islands, a peoples’ ability to incorporate outside influences and produce local culture may find itself at odds with the more nationalistic purposes of the state. The Ionian Islands came to be part of the Greek state without enduring the yoke of occupation by the Ottoman Empire or suffering in the wars that preceded the Greek free state. Therefore, the Ionian culture, in particular its popular music, has been made obscure by political elites who defined Greece as the benevolent opposite of its enemies, as the center of civilization and therefore without cultural influences – a definition that Ionian music, influenced by Italian settlers, did not meet.

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Noll, Thomas. "Ionian theorem." Journal of Mathematics and Music 3, no. 3 (November 2009): 137–51. http://dx.doi.org/10.1080/17459730903309815.

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Temperley, David, and Daphne Tan. "Emotional Connotations of Diatonic Modes." Music Perception 30, no. 3 (December 2012): 237–57. http://dx.doi.org/10.1525/mp.2012.30.3.237.

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In this experiment, participants (nonmusicians) heard pairs of melodies and had to judge which of the two melodies was happier. Each pair consisted of a single melody presented in two different diatonic modes (Lydian, Ionian, Mixolydian, Dorian, Aeolian, or Phrygian) with a constant tonic of C; all pairs of modes were used. The results suggest that modes imply increasing happiness as scale-degrees are raised, with the exception of Lydian, which is less happy than Ionian. Overall, the results are best explained by familiarity: Ionian (major mode), the most common mode in both classical and popular music, is the happiest, and happiness declines with increasing distance from Ionian. However, familiarity does not entirely explain our results. Familiarity predicts that Mixolydian would be happier than Lydian (since they are equally similar to Ionian, and Mixolydian is much more common in popular music); but for almost half of our participants, the reverse was true. This suggests that the “sharpness” of a mode also affects its perceived happiness, either due to pitch height or to the position of the scale relative to the tonic on the “line of fifths”; we favor the latter explanation.

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KARAKITSIOS, V., N. RIGAKIS, and I. BAKOPOULOS. "Migration and trapping of the Ionian series hydrocarbons (Epirus, NW Greece)." Bulletin of the Geological Society of Greece 34, no. 3 (January 1, 2001): 1237. http://dx.doi.org/10.12681/bgsg.17200.

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Surface oil shows in the Ionian zone of NW Greece are mainly linked to the organic matter rich Lower Posidonia beds of Toarcian age and shale fragments within the Triassic breccias. The calcareous formations of the Ionian series are characterized by insignificant primary porosity-permeability. Only fractured carbonates might comprise potential reservoir rocks capped on top by the detrital series. Other prospective traps, with the evaporites playing the role of cap-rocks, are related to the degree of basement involvement in the structural evolution of the Ionian basin.

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Mangira, O., E. Papadimitriou, G. Tsaklidis, and G. Vasiliadis. "SEISMIC HAZARD ASSESSMENT FOR THE CORINTH GULF AND CENTRAL IONIAN ISLANDS BY MEANS OF THE LINKED STRESS RELEASE MODEL." Bulletin of the Geological Society of Greece 50, no. 3 (July 27, 2017): 1369. http://dx.doi.org/10.12681/bgsg.11850.

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Εarthquake generation causes spatio-temporal stress changes on adjacent fault segments that can alter the occurrence probability of subsequent earthquakes onto them. The interaction is investigated with the Linked Stress Release Model, applied to fit historical data from two areas that accommodate high seismicity, the Corinth Gulf and the Central Ionian Islands. These two areas are divided in two subareas, based on seismotectonic features; Corinth Gulf is divided in the western and eastern part, whereas the area of Central Ionian Islands is divided in Kefalonia and Lefkada subareas. The results establish interactions between the subareas, especially in the Central Ionian Islands, and underline the differences in tectonic structures and earthquake mechanisms between these areas. Particularly, the seismicity in the Central Ionian Islands is proved to be more complex and active and yet more difficult to be examined, whereas the LSRM fits the Corinth Gulf data more easily.

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BARE, V., P. BAKO, V. NGRESl, V. BARE, L. NGRESl, and M. BAKO. "Geological construction of southern part of Ionian zone based on interpretation of seismic data." Bulletin of the Geological Society of Greece 34, no. 4 (January 1, 2001): 1479. http://dx.doi.org/10.12681/bgsg.17246.

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The Ionian zone is the main object of seismic interpretation for a long time. Within this framework, we shall analyze the new seismic intrpretation methods used in oil and gas exploration in the western part of Ionian zone. The Ionian zone is very complex involving certain tectonic faults. In the central part, we can see the duplex tectonic style. Anticline belts from east to west can be interpreted.The Ionian zone comprises three anticline belts:Berati belt, Kurveleshi belt and Cika belt. By application of SeisWork2D in the eastern part of the belt, we have evidenced some perscpective structures, meanwhile in the western part, the seismic quality is very chaotic. Kurveleshi belt is constructed by structures of various forms and dimensions associated with developed tectonics up to thrusting. Cika anticline belt is constructed mainly by prolonged structures of considerable dimensions associated with evaporate outcrops as in Xara, Fterra, Cika etc.

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Tucker, Emily, Jamie Gerlach, Azais Curtean, Kent Passingham, Lisa Murphy, and Gregory Lewbart. "Copper and zinc generated by the Aquascape IonGen pond clarifier system can be detrimental to koi (Cyprinus carpio) health." Veterinary Record Open 7, no. 1 (August 2020): e000396. http://dx.doi.org/10.1136/vetreco-2020-000396.

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BackgroundCopper is frequently used as an algicide, and copper ion generators such as the Aquascape IonGen claim to be safe for use in systems containing fish. In 2012, a die-off of koi (Cyprinus carpio) in a pond in Raleigh, North Carolina, occurred after the IonGen was added to the system.MethodsPhysical and postmortem examinations suggested that heavy metal toxicity was the likely cause of morbidity and mortality. This was supported by a heavy metal screening of the owners’ pond. Additional experiments were performed to determine if the IonGen produced toxic levels of copper and zinc.ResultsThe tank containing the IonGen had higher concentrations of copper and zinc, and copper levels exceeded those associated with toxicity in both hard and soft water.ConclusionThe results of this study indicate that ion generators might not be safe for fish, and copper should only be used as an algicide if concentrations are closely monitored.

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Getsos, K., F. Pomoni-Papaioannou, and A. Zelilidis. "A CARBONATE RAMP EVOLUTION IN THE TRANSITION FROM THE APULIA PLATFORM TO THE IONIAN BASIN DURING EARLY TO LATE CRETACEOUS (NW GREECE)." Bulletin of the Geological Society of Greece 40, no. 1 (June 8, 2018): 53. http://dx.doi.org/10.12681/bgsg.16335.

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Facies analysis of Cretaceous carbonate sequences from the external and central Ionian zone revealed a homoclinal ramp model of evolution. During Berriasian to Valanginian, the carbonate ramp was differentiated to an inner-mid and outer ramp environment, which corresponded to the external and central Ionian zone, respectively, while the main inner ramp environment is assumed that was located in the Pre-Apulian zone. The external Ionian zone (inner-mid ramp) is characterized by muds tones-wackes tones with fragmented echinoderms, bivalves, radiolarians and rare aptychus considered to be deposited below the fairweather wave base (FWWB). Locally, thin graded storm deposits intervene, indicating deposition above the storm weather wave base (SWB). Minor occurrences of packs tonesgrainstones, with fragmented echinoderms, calcareous algae, tubiphytes, lagenid foraminifera and rare ooids occur, as well, considered to be deposited at the lowermost part of the inner ramp, near the constantly agitated fairweather wave base (FWWB). The central Ionian zone (outer ramp) is mainly characterized by mudstones-wackestones with abundant radiolarians and rare calpionellids and calcispheres, considered to be deposited below the storm wave base (SWB). No talus or breccias deposits were observed, during the mentioned time interval, in any part of the studied area. From Hauterivian to Turonian, continual sea-level rise, led to establishment of outer ramp environment in the external Ionian zone, over the previous inner-mid ramp, and outer ramp-basin environment, over the previous outer ramp, in the central Ionian zone. The transition from shallower to deeper conditions is characterized by an overall deposition of mudstones-wackestones with abundant radiolarians rooted in pure micrite.

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De Caro, Mariagrazia, Caterina Montuori, Francesco Frugoni, Stephen Monna, Fabio Cammarano, and Laura Beranzoli. "T-Phases Observed at the Ionian Seafloor: Seismic Source and Bathymetric Effects." Seismological Research Letters 92, no. 1 (September 30, 2020): 481–93. http://dx.doi.org/10.1785/0220200096.

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Abstract T-waves are acoustic waves generated by earthquakes at the land–water interface. They can propagate efficiently for thousands of kilometers within the ocean’s low-velocity waveguide—the SOund Fixing And Ranging (SOFAR) channel. In the present work, we studied T-waves that propagate in the Ionian basin and are generated by regional earthquakes (epicentral distance <1000 km) located in the Hellenic Arc (Greece). The Ionian Sea is a small basin that has strong bathymetric variations and is limited at its western edge by a steep continental slope—the Malta escarpment. T-waves from Greece were recorded by a broadband seismometer onboard one of seafloor-observing units of the Western Ionian Regional Facility of EMSO—European Multidisciplinary Seafloor and water column Observatory Research Infrastructure (see Data and Resources) deployed in the western Ionian Sea (Italy) at about 2100 m water depth. By studying the particle motion and T-phase energy flux (TPEF) of the T-waves recorded at the observatory, we find that the western Ionian Sea bathymetry is an efficient reflector for T-waves within the SOFAR channel. To investigate whether factors other than T-wave path effects drive TPEF levels, we also study the source part of the T-wave generation process.

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Sakkas, Vassilis, Vasilis Kapetanidis, George Kaviris, Ioannis Spingos, Spyridon Mavroulis, Michalis Diakakis, John D. Alexopoulos, et al. "Seismological and Ground Deformation Study of the Ionian Islands (W. Greece) during 2014–2018, a Period of Intense Seismic Activity." Applied Sciences 12, no. 5 (February 23, 2022): 2331. http://dx.doi.org/10.3390/app12052331.

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Seismicity in the Ionian Sea (W. Greece) is mainly generated along the Cephalonia–Lefkada Transform Fault Zone (CLTFZ) in the central Ionian, and on the northwestern termination of the Hellenic subduction margin in the south. Joint pre-, co- and post-seismic ground deformation and seismological analysis is performed at the broad Ionian area, aiming to homogeneously study the spatiotemporal evolution of the activity prior to and after the occurrence of strong (M > 6) earthquakes during the period of 2014–2018. The 2014 Cephalonia earthquakes (Mw6.1 and Mw5.9) were generated on a faulting system adjacent to CLTFZ, causing local ground deformation. The post-seismic sequence is coupled in space and time with the 2015 Lefkada earthquake (Mw6.4), which occurred on the Lefkada segment of the CLTFZ. Co-seismic displacement was recorded in the broader area. Seismicity was concentrated along the CLTFZ, while its temporal evolution lasted for several months. The 2018 Zakynthos earthquake (Mw6.7) caused regional deformation and alterations on the near-velocity field, with the seismicity rate remaining above background levels until the end of 2021. In the northern Ionian, convergence between the Apulian platform and the Hellenic foreland occurs, exhibiting low seismicity. Seismic hazard assessment revealed high PGA and PGV expected values in the central Ionian.

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Kouria, Aphrodite. "Secular painting in the Ionian islands and Italian art: Aspects of a multi-faceted relationship." Historical Review/La Revue Historique 13 (February 24, 2017): 29. http://dx.doi.org/10.12681/hr.11555.

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The contribution of Italian art, especially Venetian, was decisive to the secularisation of art in the Ionian Islands and the shaping of the so-called Ionian School, in the context of a broader Western influence affecting all aspects of life and culture, especially on the islands of Zakynthos and Corfu. Italian influences, mainly of Renaissance, Mannerism and Baroque art, can be identified both on the iconographic and the stylistic level of artworks, with theoretical support. This article explores facets of the dialogue of secular painting in the Ionian with Italian art in the eighteenth and nineteenth centuries, focussing on works and artists that highlight significant aspects of this multilayered phenomenon and also through secondary channels that expand the horizon of analysis. Procession paintings, with their various connotations, and portraiture, which flourished in secular Ionian art, offer the most interesting material as regards the selection, reception and management of Italian models and points of reference.

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Tselentis, G.-A., G. Stavrakakis, E. Sokos, F. Gkika, and A. Serpetsidaki. "Tsunami hazard assessment in the Ionian Sea due to potential tsunamogenic sources – results from numerical simulations." Natural Hazards and Earth System Sciences 10, no. 5 (May 12, 2010): 1021–30. http://dx.doi.org/10.5194/nhess-10-1021-2010.

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Abstract. In spite of the fact that the great majority of seismic tsunami is generated in ocean domains, smaller basins like the Ionian Sea sometimes experience this phenomenon. In this investigation, we study the tsunami hazard associated with the Ionian Sea fault system. A scenario-based method is used to provide an estimation of the tsunami hazard in this region for the first time. Realistic faulting parameters related to four probable seismic sources, with tsunami potential, are used to model expected coseismic deformation, which is translated directly to the water surface and used as an initial condition for the tsunami propagation. We calculate tsunami propagation snapshots and mareograms for the four seismic sources in order to estimate the expected values of tsunami maximum amplitudes and arrival times at eleven tourist resorts along the Ionian shorelines. The results indicate that, from the four examined sources, only one possesses a seismic threat causing wave amplitudes up to 4 m at some tourist resorts along the Ionian shoreline.

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Gambino, Salvatore, Giovanni Barreca, Valentina Bruno, Giorgio De Guidi, Carmelo Ferlito, Felix Gross, Mario Mattia, Luciano Scarfì, and Carmelo Monaco. "Transtension at the Northern Termination of the Alfeo-Etna Fault System (Western Ionian Sea, Italy): Seismotectonic Implications and Relation with Mt. Etna Volcanism." Geosciences 12, no. 3 (March 10, 2022): 128. http://dx.doi.org/10.3390/geosciences12030128.

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Offshore data in the western Ionian Sea indicate that the NW–SE-trending dextral shear zone of the Alfeo-Etna Fault System turns to the N–S direction near the Ionian coastline, where the extensional Timpe Fault System is located. Morpho-structural data show that NW–SE-trending right-lateral strike-slip faults connect the Timpe Fault System with the upper slope of the volcano, where the eruptive activity mainly occurs along the N–S to NE–SW-trending fissures. Fault systems are related to the ~E–W-trending extension and they are seismically active having given rise to shallow and low-moderate magnitude earthquakes in the last 150 years. As a whole, morpho-structural, geodetic and seismological data, seismic profiles and bathymetric maps suggest that similar geometric and kinematic features characterize the shear zone both on the eastern flank of the volcano and in the Ionian offshore. The Alfeo-Etna Fault System probably represents a major kinematic boundary in the western Ionian Sea associated with the Africa–Europe plate convergence since it accommodates, by right-lateral kinematics, the differential motion of adjacent western Ionian compartments. Along this major tectonic alignment, crustal structures such as releasing bends, pull-apart basins and extensional horsetails occur both offshore and on-land, where they probably represent the pathway for magma uprising from depth.

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Marquart, T., G. Östlin, N. Bergvall, P. Masegosa, P. Amram, and I. Márquez. "The Kinematics of Extended Hα Emission in Blue Compact Galaxies." Proceedings of the International Astronomical Union 2, S235 (August 2006): 321. http://dx.doi.org/10.1017/s1743921306006867.

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AbstractBlue Compact Galaxies (BCGs) have received interest mainly because they comprise the best available test-beds for studies of low-metallicity star formation (SF) and allow the study of relatively unevolved systems at low redshift. Their ongoing phase of intense star formation is a transient phenomenon and the best candidates for its trigger are interactions and mergers. Studies of the kinematics are important for the understanding of this process.We present spatially resolved kinematics from the Hα line in five BCGs that show an extended region of ionised emission around the central starburst. We find this region to have near-spherical isophotes at large radii and to be dynamically decoupled from a central disturbance. A scenario where the strong triggered star formation in the center ionises the surrounding gas cloud, still following its original motions, can qualitatively explain these common features. The poster, including the figures, can be found at http://kern-2pt/thomasmarquart.net/pspdf/prague-marquart.pdf.

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Shabrang, L., M. Menna, C. Pizzi, H. Lavigne, G. Civitarese, and M. Gačić. "Long-term variability of the southern Adriatic circulation in relation to North Atlantic Oscillation." Ocean Science 12, no. 1 (February 12, 2016): 233–41. http://dx.doi.org/10.5194/os-12-233-2016.

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Abstract. The interannual variability of the South Adriatic Gyre and its relation to the wind vorticity and the large-scale climatic pattern (North Atlantic Oscillation – NAO) was studied using the time series of satellite altimetric data and ocean surface wind products. The cyclonic circulation observed in the southern Adriatic area was partly sustained by the local wind forcing, as suggested by the positive correlation between the rate of change of the current vorticity and the wind-stress vorticity. Nevertheless, the influence of vorticity advection from the adjacent area (northern Ionian Sea) cannot be ignored and it is more significant during the anticyclonic phase of Adriatic–Ionian Bimodal Oscillation System. The geostrophic current vorticities of the southern Adriatic and northern Ionian seas are correlated with a time lag of 14 months, which approximately corresponds to an advection speed of ∼ 1 cm s−1. The different wind patterns observed during two NAO phases in the winter revealed a stronger positive vorticity during the negative NAO phase. Conversely, during the wintertime positive NAO phase the wind vorticity is characterized by lower positive or slightly negative values. Despite a statistically significant negative correlation between the NAO index and the wind vorticity, no unequivocal relationship between large climatic system and the interannual variability of the South Adriatic Gyre intensity was found due to additional effects of the vorticity advection from the Ionian. This can be explained by the fact that the Ionian circulation mode does not depend on the NAO variations. Therefore, the main result of this study is that the interannual variability of the southern Adriatic cyclonic circulation is a result of the combined influence of the vorticity advection from the Ionian and the local wind-curl effect.

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ANASTASOPOULOU, A., F. BIANDOLINO, A. CHATZISPYROU, F. HEMIDA, B. GUIJARRO, V. KOUSTENI, CH MYTILINEOU, P. PATTOURA, and E. PRATO. "New Fisheries-related data from the Mediterranean Sea (November, 2016)." Mediterranean Marine Science 17, no. 3 (November 30, 2016): 822. http://dx.doi.org/10.12681/mms.1909.

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In this fourth Collective Article, with fisheries-related data from the Mediterranean, we present weight-length relationships for eight deep-sea fish species (Brama brama, Conger conger, Etmopterus spinax, Molva macrophthalma, Mora moro, Pagellus bogaraveo, Phycis blennoides) from the Eastern Ionian Sea; Scyliorhinus canicula from various locations in the Mediterranean Sea and weight-length relationships and condition factor of five Mugilidae species (Liza aurata, Liza saliens, Liza ramada, Mugil cephalus, Chelon labrosus) from a Mediterranean lagoon in the Ionian Sea. Moreover, we present otolith weight, fish length and otolith length relationships of the red mullet (Mullus barbatus) in the Aegean and Ionian Sea and otolith weight relationships in European hake (Merluccius merluccius) from the Greek Seas.

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Galanidou, Nena, Giorgos Iliopoulos, and Christina Papoulia. "The Palaeolithic settlement of Lefkas. Archaeological evidence in a palaeogeographic context." Journal of Greek Archaeology 1 (January 1, 2016): 1–33. http://dx.doi.org/10.32028/jga.v1i.642.

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The chain of islands emerging from the Ionian Sea constitutes the western part of the active Hellenic Arc and is separated from the European landmass by the shaping forces of eustasy and tectonism. As part of the Ionian Margin, the islands share the same geological and climate regimes with their counterpart, the coastal zone of the west Greek mainland extending from Epirus to the Peloponnese. The Ionian setting consists of limestone geology and karst, rocks containing abundant cherts, high tectonic activity, tsunamis, and high rainfall rates. The pioneering work conducted by A. Sordinas on Corfu, Zakynthos and other islands in the 1960s, later by Cubuk on Kefalonia, and in the 1990s by A. Dousougli and C. Zachos on Lefkas, established the earliest component of Ionian prehistory and laid the foundations for further fieldwork with an explicit Palaeolithic focus. Surface surveys exploring the diachronic history of individual islands or the coastal zone of west Greece have added new points to the Palaeolithic map. Today, early Ionian prehistory is an independent research objective, going hand-in-hand with a shift of interest to early island and coastal archaeology. It is pursued through two interconnected lines of investigation: systematic fieldwork to enlarge the archaeological sample and explore the variation of hominin settlement in time and space, and re-appraisal of published material to fine-tune the archaeology, compare it, and place it in a palaeogeographic context.

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Journal articles on the topic 'Ionien'

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