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PHY1033C/HIS3931/IDH 3931 : Discovering Physics
PHY1033C/HIS3931/IDH 3931 : Discovering Physics

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... • The field has direction so we will need to orient probe properly  In this case parallel to the field lines (see Diagram) • If the field is negative field line is moving away from the probe  Not Important we are only interested in |B| ...
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... for rocks of different ages from North America and Eurasia produces two curves, the so-called “polar wandering curves”. Note that as the curves get younger they converge. Fitting the continents back together results in a single curve. Nonetheless, the positions still do not correspond with the curre ...
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Document
Document

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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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