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understanding electromagnetism: a new approach
understanding electromagnetism: a new approach

Monopoles and Electricity
Monopoles and Electricity

... Fig 5 shows how electricity is generated in a coil of wire. This is accomplished by the atoms that make up the wire; each atom is a small magnetic dipole with its own north and south magnetic monopoles orbiting through its nucleus. When the north pole of a bar magnet passes by the magnetic field of ...
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Solar energetic particle access to distant longitudes through

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Polarimetric evidence of a white dwarf pulsar in

to go to any of the pages listed below, click on its title
to go to any of the pages listed below, click on its title

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Physics 1001 - Introduction to Magnetism VO Magnets are all

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Use the following list to match to the statements below: Seismic
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Energetic particle injection events in the Kronian magnetosphere
Energetic particle injection events in the Kronian magnetosphere

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The title of my PDF

... of seconds instead of milliseconds. The signal is a continuous series of synchrotron emissions from bunches of electrons generated from β-decay, which produce coherent, millisecond duration pulses at each frequency over several seconds (or hundreds of milliseconds for a bandwidth limited observation ...
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web page pre-post test questions

... The following questions are part of a pretest survey we would like you to complete before you participate in the seminar on space weather. We intend to use the answers as a measure of your knowledge about the topics to be discussed in the seminar. You will be asked to retake this survey again after ...
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Chandra HETGS Multiphase Spectroscopy Of The Young

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Sunspots: from small-scale inhomogeneities towards a global theory

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Lenz Law Digital Guide

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3D WHOLE-PROMINENCE FINE STRUCTURE MODELING

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Aurora



An aurora is a natural light display in the sky, predominantly seen in the high latitude (Arctic and Antarctic) regions. Auroras are produced when the magnetosphere is sufficiently disturbed by the solar wind that the trajectories of charged particles in both solar wind and magnetospheric plasma, mainly in the form of electrons and protons, precipitate them into the upper atmosphere (thermosphere/exosphere), where their energy is lost. The resulting ionization and excitation of atmospheric constituents emits light of varying colour and complexity. The form of the aurora, occurring within bands around both polar regions, is also dependent on the amount of acceleration imparted to the precipitating particles. Precipitating protons generally produce optical emissions as incident hydrogen atoms after gaining electrons from the atmosphere. Proton auroras are usually observed at lower latitudes. Different aspects of an aurora are elaborated in various sections below.
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