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  • 1
    Online Resource
    Online Resource
    Acoustical Society of America (ASA) ; 1999
    In:  The Journal of the Acoustical Society of America Vol. 105, No. 2_Supplement ( 1999-02-01), p. 1168-1169
    In: The Journal of the Acoustical Society of America, Acoustical Society of America (ASA), Vol. 105, No. 2_Supplement ( 1999-02-01), p. 1168-1169
    Abstract: The basic goal of the Ocean Seismic Network Pilot Experiment (OSNPE) was to learn how to make reliable broadband (0.001–10 Hz) seismic measurements in the deep ocean. This objective addresses both the requirement for long-term, observatory-based measurements at a small number of carefully selected sites (i.e., the Ocean Seismic Network), and for portable arrays of broadband seismographs that can be deployed for about one year to study specific geological features. The OSNPE ran from February to June 1998. The site of the experiment was ODP Hole 843B (site OSN-1) located about 225 km southwest of Oahu, Hawaii. At the OSN-1 site, three broadband seismographs were deployed within 300 m of each other. The seismometers were (i) a Teledyne GeoTech KS54000 deployed in a borehole 240 m beneath the seafloor; (ii) a Guralp CMG-3T deployed on the seafloor; and (iii) a Guralp CMG-3T buried just beneath the seafloor. The latter two systems also carried long-period pressure sensors. Meteorological and oceanographic data were also recorded continuously throughout the experiment. The magnitude and direction of seafloor currents were recorded at the experiment site itself. Four NOAA/NDBC buoys in the vicinity of OSN-1 recorded wind speed, wave-height, and wave-direction. [Work supported by NSF.]
    Type of Medium: Online Resource
    ISSN: 0001-4966 , 1520-8524
    RVK:
    Language: English
    Publisher: Acoustical Society of America (ASA)
    Publication Date: 1999
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  • 2
    Online Resource
    Online Resource
    Acoustical Society of America (ASA) ; 1999
    In:  The Journal of the Acoustical Society of America Vol. 105, No. 2_Supplement ( 1999-02-01), p. 1169-1169
    In: The Journal of the Acoustical Society of America, Acoustical Society of America (ASA), Vol. 105, No. 2_Supplement ( 1999-02-01), p. 1169-1169
    Abstract: The first Ocean Seismic Network Pilot Experiment (OSNPE) took place from January to June of 1998. The site of the experiment was located about 225 km southwest of Oahu, Hawaii, where three broadband seismographs were deployed within 300 m of each other, (i) deployed in a borehole 240-m beneath the seafloor; (ii) on the seafloor; (iii) buried just beneath the seafloor. Each of the seafloor broadband seismograph stations also carried a Cox-Webb long-period, differential pressure gauge (DPG). The OSNPE ran concurrently with PELENET, a temporary deployment of five island broadband stations and SWELL, a temporary deployment of eight DPGs. Over 50 teleseismic earthquakes were observed. The broadband seismograms recorded during the OSNPE are coherent in the frequency band 0.01–0.1 Hz. At higher frequencies (0.1–3 Hz), there is considerably more variation between the borehole, buried, seafloor, and island sites. Careful examination of the waveforms shows significant differences in the frequencies above 0.1 Hz between the buried/surface broadband ocean bottom seismographs and the borehole seismograph. These variations appear to be associated with shear-wave reverberations and/or Stonely wave propagation within the sediment section. The teleseismic earthquakes permit a preliminary evaluation of the long period (0.01–0.07 Hz) detection thresholds.
    Type of Medium: Online Resource
    ISSN: 0001-4966 , 1520-8524
    RVK:
    Language: English
    Publisher: Acoustical Society of America (ASA)
    Publication Date: 1999
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  • 3
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1990
    In:  Journal of Geophysical Research: Solid Earth Vol. 95, No. B4 ( 1990-04-10), p. 4967-4987
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 95, No. B4 ( 1990-04-10), p. 4967-4987
    Abstract: We have used a unique data set collected during the 1985 East Pacific Rise multichannel seismic experiment to reevaluate the constraints that gravity data can place on the crustal structure of the East Pacific Rise (EPR). The close spacing of track lines within the two main survey areas (8°45′N‐9°55′N and 12°20′‐13°30′N) allowed us to perform three‐dimensional analyses of high‐quality gravity data (+/−1 mGal uncertainity) obtained with the Bell Aerospace BGM‐3 gravity meter. our gravity modeling was enhanced by the availability of high‐resolution Sea Beam bathymetric data and by independent structural constraints provided by seismic reflection and refraction data. To model the crustal and upper mantle density structure at the ridge axis, we first calculated the gravity anomalies due to the density contrasts at the water/crust and crust/mantle boundaries and the changes in density caused by the cooling of the lithosphere with age and subtracted these predictable signals from the observed free‐air anomaly. The residual anomalies were then used to place constraints on the magnitude and distribution of anomalous mass at the EPR. Our results show that over 90% of the power in the observed free‐air anomaly can be modeled by these predictable components of the gravity signal. The amplitude and wavelength of the small residual anomaly can be modeled by a broad region (∼20 km wide), centered on the rise axis, of slightly lower‐than‐normal crustal and/or upper mantle densities (−0.03 Mg m −3 ). This region of anomalous mass and density variations in the underlying mantle provide the principle isostatic support for the axial topographic high. The anomalies are consistent with, but do not require, the presence of a low‐density, crustal magma chamber at the rise axis. If a largely molten magma chamber exists, then the gravity data require that it be a narrow, volumetrieally small body. There are first‐order differences in the distribution of anomalous mass between the two survey areas with the 9°N region generally being characterized by lower densities in the axial region. Along‐axis variations in anomalous mass within each of the survey areas correlate with first‐order changes in the depth and cross‐sectional shape of the EPR axial high. We attribute these differences in axial morphology and the amplitude of the associated gravity anomalies to along‐strike changes in the size of the crustal magma chamber, the width of the surrounding zone of cooling crustal rocks, and densities in the uppermost mantle beneath the rise axis.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1990
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    detail.hit.zdb_id: 3094268-8
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    SSG: 16,13
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2009
    In:  Eos, Transactions American Geophysical Union Vol. 90, No. 41 ( 2009-10-13), p. 362-363
    In: Eos, Transactions American Geophysical Union, American Geophysical Union (AGU), Vol. 90, No. 41 ( 2009-10-13), p. 362-363
    Abstract: The Hawaiian hot spot is regarded as the textbook example of the product of a deep‐rooted mantle plume [ Wilson , 1963; Morgan , 1971]. Its isolated location, far from any plate boundary, should provide an opportunity to test most basic hypotheses on the nature of plume‐plate interaction and related magmatism [e.g., Ribe and Christensen , 1999]. Yet the lack of crucial geophysical data has sustained a debate about whether Hawaii's volcanism is plume‐related or is instead the consequence of more shallow processes, such as the progressive fracturing of the plate in response to extensional stresses [ Turcotte and Oxburgh , 1973].
    Type of Medium: Online Resource
    ISSN: 0096-3941 , 2324-9250
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2009
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  • 5
    Online Resource
    Online Resource
    American Association for the Advancement of Science (AAAS) ; 2009
    In:  Science Vol. 326, No. 5958 ( 2009-12-04), p. 1388-1390
    In: Science, American Association for the Advancement of Science (AAAS), Vol. 326, No. 5958 ( 2009-12-04), p. 1388-1390
    Abstract: Defining the mantle structure that lies beneath hot spots is important for revealing their depth of origin. Three-dimensional images of shear-wave velocity beneath the Hawaiian Islands, obtained from a network of sea-floor and land seismometers, show an upper-mantle low-velocity anomaly that is elongated in the direction of the island chain and surrounded by a parabola-shaped high-velocity anomaly. Low velocities continue downward to the mantle transition zone between 410 and 660 kilometers depth, a result that is in agreement with prior observations of transition-zone thinning. The inclusion of SKS observations extends the resolution downward to a depth of 1500 kilometers and reveals a several-hundred-kilometer-wide region of low velocities beneath and southeast of Hawaii. These images suggest that the Hawaiian hot spot is the result of an upwelling high-temperature plume from the lower mantle.
    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: 2009
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  • 6
    In: Geophysical Journal International, Oxford University Press (OUP), Vol. 187, No. 3 ( 2011-12), p. 1725-1742
    Type of Medium: Online Resource
    ISSN: 0956-540X
    URL: Issue
    Language: English
    Publisher: Oxford University Press (OUP)
    Publication Date: 2011
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  • 7
    Online Resource
    Online Resource
    Elsevier BV ; 2011
    In:  Earth and Planetary Science Letters Vol. 303, No. 3-4 ( 2011-03), p. 267-280
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 303, No. 3-4 ( 2011-03), p. 267-280
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2011
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  • 8
    In: Bulletin of the AAS, American Astronomical Society, Vol. 53, No. 4 ( 2021-03-18)
    Type of Medium: Online Resource
    URL: Issue
    Language: English
    Publisher: American Astronomical Society
    Publication Date: 2021
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  • 9
    In: Urologic Oncology: Seminars and Original Investigations, Elsevier BV, Vol. 41, No. 1 ( 2023-01), p. 51.e25-51.e31
    Type of Medium: Online Resource
    ISSN: 1078-1439
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2023
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  • 10
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1994
    In:  Journal of Geophysical Research: Solid Earth Vol. 99, No. B5 ( 1994-05-10), p. 9097-9116
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 99, No. B5 ( 1994-05-10), p. 9097-9116
    Abstract: Using migrated common depth point reflection profiles, we find the structural differences along the ultrafast spreading ( 〉 150 mm/yr) East Pacific Rise south of the Garrett fracture zone are second‐order, suggesting a remarkably uniform process of crustal accretion. The rise axis south of the Garrett transform is underlain by a narrow ( 〈 1.0 km) melt lens which shows great along‐strike continuity. The depth of the axial melt sill is approximately 1200 m beneath the seafloor which is about 400 m shallower than along the slower spreading East Pacific Rise at 9°30′N. This observation strengthens the argument that the depth to the top of the crustal velocity inversion is spreading rate dependent. Melt sill width, however, shows little variation along the East Pacific Rise, suggesting no dependence of magma chamber size on spreading rate. The melt reservoir decreases in width toward/across the 14°27′S ridge axis discontinuity by a modest 250–300 m and appears to be continuous across this feature. Given the small aspect ratio (∼1.0 km by ∼50 m by tens of kilometers) of the axial melt lens, the previously recorded jump in MgO content across the 14°27′S offset is likely the result of a mixing boundary which is sustained through an along‐strike impedance in convection. Wide‐angle reflections originating at the base of seismic layer 2A, assumed to coincide with the extrusive layer, reveal a twofold to threefold increase (200–250 to 500–600 m) in thickness within 1–2 km of the rise axis. The pattern of extrusive thickening imaged south of the Garrett transform is similar to that observed along the slower spreading (110–120 mm/yr) East Pacific Rise at 9°N. Outside of the neovolcanic zone mean extrusive thickness is relatively invariant along a profile and from profile to profile. This implies a degree of temporal stability of the along‐strike magma supply when integrated over the 10 kyr that corresponds to the width of the neovolcanic zone. The inferred uniformity of off‐axis mean extrusive thickness is inconsistent with the conjecture that decreases in axial volume toward the 14°27′S discontinuity are caused by long‐term reductions in magma supply. Second‐order differences in the style of extrusive thickening may be related to structural differences within the low‐velocity zone underlying the rise axis and/or changes within the stress field in the overlying carapace which results in the diffuse emplacement of lavas near the rise axis. Images of Mono on cross‐axis profiles may be traced to within ∼1.0 km of the melt sill edge; this observation is in agreement with rise crest models which generate the lower crustal section through the advection of material down and outward from the axial melt lens rather than through cumulate deposition at the base of a large magma chamber.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1994
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    SSG: 16,13
    Location Call Number Limitation Availability
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