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Science (New York, N.Y.), 1963
© 1963 American Association for the Advancement of Science. 25 February 1963. The three-axis flux gate magnetometer electronics were designed and built by Marshall Laboratories of Torrance, Calif., under the supervision of the Jet Propulsion Laboratory, represented by Benjamin V. Connor, the magnetometer project engineer. The experiment is supported by
Smith, E. J. +3 more
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© 1963 American Association for the Advancement of Science. 25 February 1963. The three-axis flux gate magnetometer electronics were designed and built by Marshall Laboratories of Torrance, Calif., under the supervision of the Jet Propulsion Laboratory, represented by Benjamin V. Connor, the magnetometer project engineer. The experiment is supported by
Smith, E. J. +3 more
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Accounts of Chemical Research, 2011
Aromaticity is indispensable for explaining a variety of chemical behaviors, including reactivity, structural features, relative energetic stabilities, and spectroscopic properties. When interpreted as the spatial delocalization of π-electrons, it represents the driving force for the stabilization of many planar molecular structures.
Rafael, Islas +2 more
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Aromaticity is indispensable for explaining a variety of chemical behaviors, including reactivity, structural features, relative energetic stabilities, and spectroscopic properties. When interpreted as the spatial delocalization of π-electrons, it represents the driving force for the stabilization of many planar molecular structures.
Rafael, Islas +2 more
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2012
The study of magnetism and magnetic fields readily follows the study of electricity and is normally a second-semester topic in a first-year physics course. One of the difficulties that a teacher may encounter is that students often confuse magnetic poles with electric charges.
Jan Mader, Mary Winn
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The study of magnetism and magnetic fields readily follows the study of electricity and is normally a second-semester topic in a first-year physics course. One of the difficulties that a teacher may encounter is that students often confuse magnetic poles with electric charges.
Jan Mader, Mary Winn
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Physical Review E, 2012
A vertically draining thin ferrofilm under the influence of gravity and a nonuniform magnetic field is considered. It is observed experimentally that the presence of the magnetic field greatly alters the drainage of the film. A mathematical model is developed to describe the behavior. Experiments are conducted for multiple magnetic field configurations.
Randy, Back, J Regan, Beckham
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A vertically draining thin ferrofilm under the influence of gravity and a nonuniform magnetic field is considered. It is observed experimentally that the presence of the magnetic field greatly alters the drainage of the film. A mathematical model is developed to describe the behavior. Experiments are conducted for multiple magnetic field configurations.
Randy, Back, J Regan, Beckham
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Science, 1986
The magnetic field experiment on the Voyager 2 spacecraft revealed a strong planetary magnetic field of Uranus and an associated magnetosphere and fully developed bipolar magnetic tail. The detached bow shock wave in the solar wind supersonic flow was observed upstream at 23.7 Uranus radii (1 R U = 25 ...
N F, Ness +6 more
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The magnetic field experiment on the Voyager 2 spacecraft revealed a strong planetary magnetic field of Uranus and an associated magnetosphere and fully developed bipolar magnetic tail. The detached bow shock wave in the solar wind supersonic flow was observed upstream at 23.7 Uranus radii (1 R U = 25 ...
N F, Ness +6 more
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Fusion Technology, 1998
Plasmas and magnetic fields are inseparably related in numerous physical circumstances. This is not only the case in natural occurring plasmas like the solar corona and the earth magnetic tail, but also in laboratory plasmas like tokamaks and stellarators.
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Plasmas and magnetic fields are inseparably related in numerous physical circumstances. This is not only the case in natural occurring plasmas like the solar corona and the earth magnetic tail, but also in laboratory plasmas like tokamaks and stellarators.
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Magnetic Resonance in Medicine, 1988
AbstractHomogeneous radiofrequency magnetic fields are necessary for production of high‐quality magnetic images and for most forms of magnetic resonance spectroscopy. It is often convenient to map the radiofrequency homogeneity associated with a resonant device by measuring the magnetic image intensity of an aqueous phantom placed within the resonator.
J P, Hornak, J, Szumowski, R G, Bryant
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AbstractHomogeneous radiofrequency magnetic fields are necessary for production of high‐quality magnetic images and for most forms of magnetic resonance spectroscopy. It is often convenient to map the radiofrequency homogeneity associated with a resonant device by measuring the magnetic image intensity of an aqueous phantom placed within the resonator.
J P, Hornak, J, Szumowski, R G, Bryant
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Geophysical & Astrophysical Fluid Dynamics, 1987
The observations of the optical polarization of starlight [1,2] showed large-scale alignment of the vectors which was interpreted to be due to galactic magnetic fields which align interstellar grains [3]. The data on star polarization accumulated over many years (e.g. [4,5,6]) giving in the end a large sample of objects at known distances.
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The observations of the optical polarization of starlight [1,2] showed large-scale alignment of the vectors which was interpreted to be due to galactic magnetic fields which align interstellar grains [3]. The data on star polarization accumulated over many years (e.g. [4,5,6]) giving in the end a large sample of objects at known distances.
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