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  • 1
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 50, No. 13 ( 2023-07-16)
    Abstract: Valdivia Bank is characterized by quasi‐linear magnetic anomalies that are parallel to the inferred paleo‐Mid‐Atlantic Ridge Magnetic anomalies imply that the plateau becomes younger E‐W consistent with formation via seafloor spreading during anomalies C34n‐C33r Rift valleys, division of C33r, and anomaly curvature imply complex ridge tectonics and a ridge jump
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2023
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    SSG: 16,13
    Location Call Number Limitation Availability
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  • 2
    Online Resource
    Online Resource
    Springer Science and Business Media LLC ; 1998
    In:  Geo-Marine Letters Vol. 18, No. 4 ( 1998-12), p. 267-276
    In: Geo-Marine Letters, Springer Science and Business Media LLC, Vol. 18, No. 4 ( 1998-12), p. 267-276
    Type of Medium: Online Resource
    ISSN: 0276-0460 , 1432-1157
    Language: English
    Publisher: Springer Science and Business Media LLC
    Publication Date: 1998
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    detail.hit.zdb_id: 381526-2
    SSG: 13
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2022
    In:  Journal of Geophysical Research: Solid Earth Vol. 127, No. 11 ( 2022-11)
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 127, No. 11 ( 2022-11)
    Abstract: We present a high‐resolution bathymetry map of southern Shatsky Rise with greater multibeam coverage revealing small‐scale surface features Tamu Massif is subtly segmented into 5 smaller rises consistent with formation by series of ridge eruptions along a jumping triple junction Secondary volcanic cones are distributed mainly over the southern and eastern flanks, and many have trends implying spreading ridge control
    Type of Medium: Online Resource
    ISSN: 2169-9313 , 2169-9356
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2022
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    SSG: 16,13
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2019
    In:  Geophysical Research Letters Vol. 46, No. 16 ( 2019-08-28), p. 9474-9482
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 46, No. 16 ( 2019-08-28), p. 9474-9482
    Abstract: We identified Late Cretaceous magnetic anomalies C33n‐C34n along Walvis Ridge where these anomalies were not previously identified Anomaly patterns infer that Valdivia Bank has an E‐W trending age progression in contrast with the N‐S age progression implied by the hot spot models Uneven anomaly width and spacing indicate complex tectonics between Walvis Ridge and Rio Grande Rise between anomalies C34n and C30n
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2019
    detail.hit.zdb_id: 2021599-X
    detail.hit.zdb_id: 7403-2
    SSG: 16,13
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  • 5
    Online Resource
    Online Resource
    American Association for the Advancement of Science (AAAS) ; 2001
    In:  Science Vol. 294, No. 5551 ( 2001-12-21), p. 2505-2505
    In: Science, American Association for the Advancement of Science (AAAS), Vol. 294, No. 5551 ( 2001-12-21), p. 2505-2505
    Type of Medium: Online Resource
    ISSN: 0036-8075 , 1095-9203
    RVK:
    RVK:
    Language: English
    Publisher: American Association for the Advancement of Science (AAAS)
    Publication Date: 2001
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    detail.hit.zdb_id: 2066996-3
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  • 6
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1984
    In:  Journal of Geophysical Research: Solid Earth Vol. 89, No. B13 ( 1984-12-10), p. 11135-11151
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 89, No. B13 ( 1984-12-10), p. 11135-11151
    Abstract: Seamount magnetic anomaly studies have been conducted on eight volcanoes in the Line Islands seamount chain. The magnetic anomalies of these seamounts were inverted to obtain paleomagnetic information. Four of these gave paleomagnetic pole positions consistent with other Pacific Cretaceous pole positions. Of these, three have reliable radiometric ages ranging from 72 to 85 Ma. The remaining four seamounts gave geomagnetic poles that agree with other Eocene‐Early Oligocene Pacific paleomagnetic data, and one has a reliable radiometric age of 39 Ma. All of the apparently Eocene volcanoes occur in the central Line Islands between 8°N and 3°S. We suggest that the Eocene volcanic event was approximately coincident with the profound change in Pacific plate motion, recorded by the bend in the Hawaiian‐Emperor seamount chain, that occurred at approximately 43 Ma. This volcanism may have resulted from the large change in intraplate stress accompanying the change of plate motion. The change in stress might have pulled apart a zone of weakness caused by the original formation of the Line Islands. Detailed paleomagnetic modeling of the Line Islands seamounts was necessary to obtain good results, as seven of the eight seamounts appear to be inhomogeneously magnetized to some extent. Despite these inhomogeneities the high goodness‐of‐fit parameters and the excellent agreement of these results with other Pacific paleomagnetic data suggest that the paleopoles derived from these seamounts are reliably determined.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1984
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    detail.hit.zdb_id: 2969341-X
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    detail.hit.zdb_id: 3094268-8
    detail.hit.zdb_id: 710256-2
    detail.hit.zdb_id: 2016804-4
    detail.hit.zdb_id: 3094181-7
    detail.hit.zdb_id: 3094219-6
    detail.hit.zdb_id: 3094167-2
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    SSG: 16,13
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1984
    In:  Journal of Geophysical Research: Solid Earth Vol. 89, No. B13 ( 1984-12-10), p. 11261-11272
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 89, No. B13 ( 1984-12-10), p. 11261-11272
    Abstract: Geological and geophysical studies along the entire length of the Line Islands were undertaken in order to test the hot spot model for the origin of this major linear island chain. Volcanic rocks were recovered in 21 dredge hauls and fossiliferous sedimentary rocks were recovered in 19 dredge hauls. Volcanic rocks from the Line Islands are alkalic basalts and hawaiites. In addition, a tholeiitic basalt and a phonolite have been recovered from the central part of the Line chain. Microprobe analyses of groundmass augite in the alkalic basalts indicate that they contain high TiO 2 (1.0–4.0 wt %) and Al 2 O 3 (3.4–9.1 wt %) and are of alkaline to peralkaline affinities. Major element compositions of the Line Islands volcanic rocks are very comparable to Hawaiian volcanic rocks. Trace element and rare earth element analyses also indicate that the rocks are typical of oceanic island alkalic lavas; the Line Islands lavas are very much unlike typical mid‐ocean ridge or fracture zone basalts. Dating of these rocks by 40 Ar‐ 39 Ar, K‐Ar, and paleontological methods, combined with Deep Sea Drilling Project data from sites 165, 315, and 316 and previously dated dredged rocks, provide ages of volcanic events at 20 localities along the chain from 18°N to 9°S, a distance of almost 4000 km. All of these dates define mid‐Cretaceous to late Eocene edifice or ridge‐building volcanic events. Eocene volcanic events took place from 15°N to 9°S, and Late Cretaceous events took place from 18°N to 9°S. In the southern Line Islands both Cretaceous and Eocene events took place on the same edifice or ridge, indicating recurrent volcanism at a single locality. The irregular distribution of atolls in the chain, the fact that Late Cretaceous reefs flourished along a distance of approximately 2500 km in the central and southern Line Islands, and the observation that spatially closely related seamounts exhibit different subsidence histories are interpreted as indicating that large segments of the chain have not followed a t 1/2 related subsidence path. Magnetic surveys of 11 seamounts show that four of the seamounts, from the central Line chain, give virtual geomagnetic poles which fall well to the north of virtual geomagnetic poles of Cretaceous seamounts. These four poles agree with other paleomagnetic data of middle‐late Eocene‐early Oligocene age from the Pacific. One of these four seamounts yielded a 40 Ar‐ 39 Ar total fusion age of 39 Ma. Because the poles of all four seamounts fall into a tight group we infer that they are probably of middle‐late Eocene age to early Oligocene age. The other three seamounts as well as one seamont from the Line Islands analyzed previously all give virtual geomagnetic poles which agree with Late Cretaceous paleomagnetic data from the Pacific. Of these four seamounts, three give Late Cretaceous 40 Ar‐ 39 Ar ages ranging from 71 to 85 Ma; another, in the southern Line Islands, is interpreted, on paleontological evidence, to be of Late Cretaceous age. The origin of the Line Islands has been ascribed by previous workers to the effects of a single hot spot and to the action of four hot spots. The single hot spot model cannot account for all of the volcanic edifices in the Line Islands, although it does explain a general age progression of 9.6±0.4 cm/yr from north to south along the chain derived from a number of dated edifices. The four hot spot model accounts for more of the dated volcanic edifices but still does not explain all of the available data. The petrologic data argue against a mid‐ocean ridge or transform fault origin proposed by earlier workers. The complex volcanic province represented by the Line Islands remains a challenge to existing models for the origin of midplate volcanism in the Pacific. An atoll drilling program which could determine edifice building histories, paleolatitudes of seamount formation, and subsidence rates and patterns in the Line Islands is needed.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1984
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    detail.hit.zdb_id: 3094104-0
    detail.hit.zdb_id: 2130824-X
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    detail.hit.zdb_id: 2403298-0
    detail.hit.zdb_id: 2016800-7
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    detail.hit.zdb_id: 161667-5
    detail.hit.zdb_id: 2969341-X
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094268-8
    detail.hit.zdb_id: 710256-2
    detail.hit.zdb_id: 2016804-4
    detail.hit.zdb_id: 3094181-7
    detail.hit.zdb_id: 3094219-6
    detail.hit.zdb_id: 3094167-2
    detail.hit.zdb_id: 2220777-6
    detail.hit.zdb_id: 3094197-0
    SSG: 16,13
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  • 8
    Online Resource
    Online Resource
    Oxford University Press (OUP) ; 2013
    In:  Geophysical Journal International Vol. 194, No. 1 ( 2013-07-01), p. 18-29
    In: Geophysical Journal International, Oxford University Press (OUP), Vol. 194, No. 1 ( 2013-07-01), p. 18-29
    Type of Medium: Online Resource
    ISSN: 0956-540X , 1365-246X
    Language: English
    Publisher: Oxford University Press (OUP)
    Publication Date: 2013
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    detail.hit.zdb_id: 2006420-2
    detail.hit.zdb_id: 1002799-3
    SSG: 16,13
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  • 9
    Online Resource
    Online Resource
    JSTOR ; 1990
    In:  Journal of Biogeography Vol. 17, No. 6 ( 1990-11), p. 702-
    In: Journal of Biogeography, JSTOR, Vol. 17, No. 6 ( 1990-11), p. 702-
    Type of Medium: Online Resource
    ISSN: 0305-0270
    Language: Unknown
    Publisher: JSTOR
    Publication Date: 1990
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    detail.hit.zdb_id: 188963-1
    SSG: 12
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  • 10
    In: Doklady Earth Sciences, Pleiades Publishing Ltd, Vol. 434, No. 1 ( 2010-9), p. 1208-1213
    Type of Medium: Online Resource
    ISSN: 1028-334X , 1531-8354
    Language: English
    Publisher: Pleiades Publishing Ltd
    Publication Date: 2010
    detail.hit.zdb_id: 2227421-2
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