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  • 1
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1996
    In:  Journal of Geophysical Research: Solid Earth Vol. 101, No. B10 ( 1996-10-10), p. 21973-21973
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 101, No. B10 ( 1996-10-10), p. 21973-21973
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1996
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    detail.hit.zdb_id: 2969341-X
    detail.hit.zdb_id: 161665-1
    detail.hit.zdb_id: 3094268-8
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    detail.hit.zdb_id: 3094181-7
    detail.hit.zdb_id: 3094219-6
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    SSG: 16,13
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  • 2
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1994
    In:  Journal of Geophysical Research: Solid Earth Vol. 99, No. B6 ( 1994-06-10), p. 12031-12032
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 99, No. B6 ( 1994-06-10), p. 12031-12032
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1994
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    detail.hit.zdb_id: 3094104-0
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    detail.hit.zdb_id: 3094268-8
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    SSG: 16,13
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  • 3
    Online Resource
    Online Resource
    Elsevier BV ; 2001
    In:  Earth and Planetary Science Letters Vol. 185, No. 3-4 ( 2001-2), p. 237-252
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 185, No. 3-4 ( 2001-2), p. 237-252
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2001
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  • 4
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1988
    In:  Eos, Transactions American Geophysical Union Vol. 69, No. 8 ( 1988-02-23), p. 115-115
    In: Eos, Transactions American Geophysical Union, American Geophysical Union (AGU), Vol. 69, No. 8 ( 1988-02-23), p. 115-115
    Abstract: William Jason Morgan, Jr., entered geophysics through a lucky break — for both him and geophysics. He was a graduate student in physics at Princeton University, looking for evidence of gravity waves and possible changes in the gravitational constant, when Walter Elsasser came over from the Geology Department looking for a post doc who wished to explore some mantle convection problems. Since he enjoyed living in Princeton, and Elsasser's problems sounded interesting, he accepted. The few small steps from the Physics Building to the neighboring Geology Department turned out to be the longest move so far in his professional career, as he is now a professor of geophysics at Princeton. In any case, his mind has made giant leaps since then
    Type of Medium: Online Resource
    ISSN: 0096-3941 , 2324-9250
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1988
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  • 5
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1992
    In:  Geophysical Research Letters Vol. 19, No. 1 ( 1992-01-03), p. 13-16
    In: Geophysical Research Letters, American Geophysical Union (AGU), Vol. 19, No. 1 ( 1992-01-03), p. 13-16
    Abstract: We analyze over 1300 km of high resolution along‐axis gravity profiles at ridges with half‐spreading rates ranging from 1.2 to 5.5 cm/yr. The results show consistently higher along‐axis gradients of mantle Bouguer anomaly at the slow‐spreading Mid‐Atlantic Ridge (MAR) (0.3–1.2 mgal/km) than at the intermediate‐ to fast‐spreading Cocos‐Nazca Ridge and East Pacific Rise (EPR) (0.1–0.2 mgal/km). The regional peak‐to‐trough amplitude of mantle Bouguer anomaly is also greater along the MAR (30–60 mgal) than the Cocos‐Nazca Ridge and the EPR (10–20 mgal). With increasing spreading rate, the regional peak‐to‐trough amplitude of axial seafloor depth decreases from 1000–1700 m to 200–700 m. 3‐D numerical experiments suggest that mantle contributions to the gravity can be significant only near large‐offset transforms. At the more commonly observed non‐transform offsets, gravity anomalies will reflect crustal thickness variations. The along‐axis gravity data thus indicate that the amplitude of along‐axis crustal thickness variation decreases with increasing spreading rate. We propose that this spreading rate dependent crustal accretion style may originate in the mantle: finite‐amplitude mantle upwelling is intrinsically plume‐like (3‐D) beneath a slow‐spreading ridge but more sheet‐like (2‐D) beneath a fast‐spreading ridge. Such a transition in mantle upwelling may occur if the relative importance of passive upwelling over buoyant upwelling increases with increasing spreading rate. Small amplitude 3‐D upwellings may occur at a fast‐spreading ridge, but their effects on crustal thickness variations will be significantly reduced by along‐axis melt flows along a persistent low‐viscosity crustal magma chamber. In contrast, the large crustal thickness variations due to 3‐D mantle upwellings will be maintained at a slow‐spreading ridge because less along‐axis melt flows can occur in the colder and more rigid crust there.
    Type of Medium: Online Resource
    ISSN: 0094-8276 , 1944-8007
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1992
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  • 6
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 1993
    In:  Journal of Geophysical Research: Solid Earth Vol. 98, No. B12 ( 1993-12-10), p. 21977-21995
    In: Journal of Geophysical Research: Solid Earth, American Geophysical Union (AGU), Vol. 98, No. B12 ( 1993-12-10), p. 21977-21995
    Abstract: Segmentation and along‐axis variations within individual segments indicate the inherently three‐dimensional nature of mantle up welling and melting beneath oceanic spreading centers. Numerical convection experiments are used to explore the effects of local buoyancy forces on upwelling and melt production beneath a segmented spreading center. The experiments are conducted in a region consisting of a thermally defined rigid lithosphere and a uniform viscosity asthenosphere overlying a higher‐viscosity mantle half‐space. A periodic plate boundary geometry is imposed consisting of spreading segments and transform offsets. Buoyancy forces are caused by thermal expansion and the compositional density reduction due to the extraction of partial melt. The relative magnitudes of the buoyant and plate‐driven components of mantle flow are controlled by the spreading rate and mantle viscosity, with buoyant flow more important at lower spreading rates and viscosities. Buoyant flow beneath the spreading axis amplifies along‐axis variations in upwelling near a ridge‐transform intersection, and distributes the variations along the entire spreading axis. Buoyant flow may thus be responsible for the more three‐dimensional character of slow spreading centers. Away from the spreading axis, thermal buoyancy drives convective rolls that align with the direction of plate motion and which have an along‐axis wavelength controlled by the prescribed thickness of the asthenosphere. However, the position and stability of rolls are influenced by the segmentation geometry. In cases where the spreading center geometry does not allow a stable configuration of rolls, the flow is time‐dependent. Along‐axis variations in upwelling cause variations in melt production, which imply large variations in crustal thickness that dominate the surface gravity signal. The crustal thickness distributions implied by these numerical experiments produce bulls‐eye‐shaped negative mantle Bouguer anomalies centered over spreading segments, as observed at several spreading centers. The amplitude of the anomaly increases with decreasing spreading rate.
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 1993
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  • 7
    Online Resource
    Online Resource
    American Geophysical Union (AGU) ; 2010
    In:  Journal of Geophysical Research Vol. 115, No. B7 ( 2010-07-24)
    In: Journal of Geophysical Research, American Geophysical Union (AGU), Vol. 115, No. B7 ( 2010-07-24)
    Type of Medium: Online Resource
    ISSN: 0148-0227
    Language: English
    Publisher: American Geophysical Union (AGU)
    Publication Date: 2010
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    SSG: 16,13
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  • 8
    Online Resource
    Online Resource
    Elsevier BV ; 2010
    In:  Earth and Planetary Science Letters Vol. 296, No. 1-2 ( 2010-7), p. 34-44
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 296, No. 1-2 ( 2010-7), p. 34-44
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 2010
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  • 9
    Online Resource
    Online Resource
    Elsevier BV ; 1995
    In:  Earth and Planetary Science Letters Vol. 129, No. 1-4 ( 1995-1), p. 73-84
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 129, No. 1-4 ( 1995-1), p. 73-84
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 1995
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  • 10
    Online Resource
    Online Resource
    Elsevier BV ; 1992
    In:  Earth and Planetary Science Letters Vol. 111, No. 2-4 ( 1992-7), p. 493-516
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 111, No. 2-4 ( 1992-7), p. 493-516
    Type of Medium: Online Resource
    ISSN: 0012-821X
    RVK:
    Language: English
    Publisher: Elsevier BV
    Publication Date: 1992
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    SSG: 16,13
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