Zobrazeno 1 - 10
of 148
pro vyhledávání: '"Michael D. Fuller"'
Autor:
Michael D. Fuller
Publikováno v:
Geological Society of America Abstracts with Programs.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::582ad0a6e4c20ade64dab1db65305929
https://doi.org/10.1130/abs/2017cd-291993
https://doi.org/10.1130/abs/2017cd-291993
Autor:
William S. Cassata, Sonia M. Tikoo, Michael D Fuller, David L. Shuster, Jérôme Gattacceca, Clément Suavet, Benjamin P. Weiss, Eduardo A. Lima, Francis Nimmo
Publikováno v:
Earth and Planetary Science Letters. 404:89-97
Recent analyses of Apollo samples have demonstrated that a core dynamo existed on the Moon between at least 4.25 and 3.56 billion years ago (Ga) with surface field intensities reaching ∼70 μT. However, it is unknown when the Moon's magnetic field
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::34e683f9c4b84352a27b983cea93a4f4
https://doi.org/10.1016/j.epsl.2014.07.010
https://doi.org/10.1016/j.epsl.2014.07.010
Autor:
Lindsey Chan, William S. Cassata, Clément Suavet, Jérôme Gattacceca, Benjamin P. Weiss, Ian Garrick-Bethell, David L. Shuster, Timothy L. Grove, Michael D Fuller, James W. Head
Publikováno v:
Proceedings of the National Academy of Sciences. 110:8453-8458
The lifetime of the ancient lunar core dynamo has implications for its power source and the mechanism of field generation. Here, we report analyses of two 3.56-Gy-old mare basalts demonstrating that they were magnetized in a stable and surprisingly i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a50e64f487021cfc6765f9dd843e48c6
https://doi.org/10.1073/pnas.1300341110
https://doi.org/10.1073/pnas.1300341110
Publikováno v:
Studia Geophysica et Geodaetica. 52:225-235
The REM(AF) method is a new tool for the analysis of the origin and alternating field demagnetization coercivity spectra of the remanent magnetization. We applied this method on precambrian Gila diabase sheets from Arizona in order to identify the hi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::99ea9201fc834d51222b7933a4e890cd
https://doi.org/10.1007/s11200-008-0015-1
https://doi.org/10.1007/s11200-008-0015-1
Publikováno v:
Geophysical Journal International. 169:91-99
SUMMARY The spatio-temporal variations in the main geomagnetic field are analysed using Maxwell's source representation of the potential function defined by Maxwell's theory of poles. Maxwell sources up to order 4 are obtained for three main geomagne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::88733e35ed25713403bdeca0fa72d1d2
https://doi.org/10.1111/j.1365-246x.2006.03300.x
https://doi.org/10.1111/j.1365-246x.2006.03300.x
Publikováno v:
Physics of the Earth and Planetary Interiors. 156:242-260
Ocean Drilling Program (ODP) Leg 182, to the Great Australian Bight (GAB), Leg 189 around Tasmania, and Leg 194 off the Great Barrier Reef on the Marion Plateau, all sampled thick carbonate sections that tested the coring techniques and the magnetics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f0e152bfdc396839a02306cfd7688a79
https://doi.org/10.1016/j.pepi.2005.08.007
https://doi.org/10.1016/j.pepi.2005.08.007
Autor:
Michael D Fuller
Publikováno v:
Earth and Planetary Science Letters. 245:605-615
The possibility that precession provides power to the geodynamo has been tested by comparing variations in field intensity and the occurrence of excursions and reversals with the obliquity signal. The strongest minima in the paleomagnetic intensity r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3689c6760d823e67c077ab89ebf8466c
https://doi.org/10.1016/j.epsl.2006.03.022
https://doi.org/10.1016/j.epsl.2006.03.022
Autor:
Norman F. Ness, Peter J. Wasilewski, Mario H. Acuña, Tomas Kohout, Michael D Fuller, Emilio Herrero-Bervera, Gunther Kletetschka
Publikováno v:
Physics of the Earth and Planetary Interiors. 154:290-298
Thermally acquired remanent magnetization is important for the estimation of the past magnetic field present at the time of cooling. Rocks that cool slowly commonly contain magnetic grains of millimeter scale. This study investigated 1-mm-sized magne
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a97fc431c904cb587fb1071d883e7672
https://doi.org/10.1016/j.pepi.2005.07.005
https://doi.org/10.1016/j.pepi.2005.07.005
Publikováno v:
Geochimica et Cosmochimica Acta. 68:4963-4969
The δ 13 C values of thirty-four individual amino acids and two pyridine carboxylic acids have been obtained fromthe Murchison meteorite. They were found to range from +4.9 to +52.8‰, with statistically significant differences observed both within
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c9a9ec3da58a33aeafb5cce8a0c7c789
https://doi.org/10.1016/j.gca.2004.05.024
https://doi.org/10.1016/j.gca.2004.05.024
Autor:
Edward Scott, Michael D Fuller
Publikováno v:
Earth and Planetary Science Letters. 220:83-90
The crustal magnetic field of Mars differs markedly from Earth’s as the Martian features are an order of magnitude stronger and are not distributed over the whole globe as on Earth, but are concentrated in a band in the southern highlands. Unless t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a7a3b2e35a48d2aef88c7290332edbcb
https://doi.org/10.1016/s0012-821x(04)00032-9
https://doi.org/10.1016/s0012-821x(04)00032-9