The top documents tagged [fluid core]

Advanced Fluid
Documents Advanced Fluid

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Slabby pahoehoe from the western Deccan Volcanic Province: evidence for incipient pahoehoe^aa transitions
Documents Slabby pahoehoe from the western Deccan Volcanic Province: evidence for incipient pahoehoe^aa transitions

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Jurnal geomagnet mitchell johnson
Engineering Jurnal geomagnet mitchell johnson

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The Fluid Core: How Technology Is Creating a New Hierarchy of Need, and How Smart Companies Are Responding
Business The Fluid Core: How Technology Is Creating a New Hierarchy of Need, and How Smart Companies Are Responding

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HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics,
Documents HIGH-QUALITY FAST QPOs FROM MAGNETARS: AN ELECTRIC CIRCUIT MODEL A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics,

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Possible excitation of the Chandler wobble by the geophysical annual cycle Kosek Wiesław Space Research Centre, Polish Academy of Sciences Seminar at
Documents Possible excitation of the Chandler wobble by the geophysical annual cycle Kosek Wiesław Space Research Centre, Polish Academy of Sciences Seminar at

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VieVS User Workshop 7 – 9 September, 2010 Vienna Hana Spicakova Results obtained using VieVS: Love numbers and FCN period presented at IVS General Meeting
Documents VieVS User Workshop 7 – 9 September, 2010 Vienna Hana Spicakova Results obtained using VieVS: Love numbers and FCN period presented at IVS General Meeting

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Solidified iron 20004000 km6000800010,00012,000 solid mantle Mg(Fe) silicates crust Rapidly convecting, electrically conducting, fluid iron The outer core:
Documents Solidified iron 20004000 km6000800010,00012,000 solid mantle Mg(Fe) silicates crust Rapidly convecting, electrically conducting, fluid iron The outer core:

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9 Planetary Geology Planets Rock!. 9 Goals What determines why planets look the way they do. What are the 4 main process that affect a planet’s surface
Documents 9 Planetary Geology Planets Rock!. 9 Goals What determines why planets look the way they do. What are the 4 main process that affect a planet’s surface

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Reversals of the Geomagnetic Field Secular variations- historic to modern changes in the field Archaeomagnetism: changes during the Holocene Reversals
Documents Reversals of the Geomagnetic Field Secular variations- historic to modern changes in the field Archaeomagnetism: changes during the Holocene Reversals

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6 Planetary Geology Planets Rock!. 6 Goals What determines why planets look the way they do. What are the 4 main process that affect a planet’s surface
Documents 6 Planetary Geology Planets Rock!. 6 Goals What determines why planets look the way they do. What are the 4 main process that affect a planet’s surface

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ON THE ORIGIN OF HIGH-QUALITY FAST QPOs FROM MAGNETARS A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)
Documents ON THE ORIGIN OF HIGH-QUALITY FAST QPOs FROM MAGNETARS A.Stepanov (Pulkovo Observatory, St.Petersburg) V.Zaitsev (Institute of Applied Physics, N.Novgorod)

224 views