Text: "Orbits in the solar wind -- a mini-research problem." A remarkable motion occurs when a classical inverse-square law orbit is perturbed by a weak uniform force field in the orbital plane. A 3% cause change can lead to colossal effects. Of particular interest is the probability density of the first excited state of hydrogen. If such anomalous effects as these can be obtained in conservation laws (which are statistical laws) so that the local skewing of the statistics occurs, it would make free energy possible. American Journal of Physics. 42(5), May 1974. p. 361-371.

See Also: solar wind, inverse square law, gravitation, electrostatics, angular momentum, free energy, oscillations.

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