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Polar wind

High-altitude atmospheric effect

  • 3 min read
  • 3 chapters

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Through Solar wind, Electric field and Ionosphere

History

In 1966 Bauer and, separately, Dessler and Michel noted that since the Earth's geomagnetic field above the poles forms a long tail away from the Sun out beyond the Moon's orbit, ions should flow from the higher pressure region in the ionosphere out into space. The term "polar wind" was coined in 1968 in a pair of articles by Banks and Holzer and by Ian Axford. Since the process by which the ionospheric plasma flows away from the Earth along magnetic field lines, is similar to the flow of solar plasma away from the Sun's corona (the solar wind), Axford suggested the term "polar wind."

The earliest experimental characterization of the polar wind came from the 1966 Explorer 33 and especially the 1974 ISIS-2 satellite projects. Additional data from the 1981 Dynamics Explorer led to some uncertainty in the theoretical models about the role of cool O+ ions. This issue was cleared up with the more comprehensive data from 1989 Akebono satellite, and the 1996 Polar satellite.

The idea for the polar wind originated with the desire to solve the paradox of the terrestrial helium budget. This paradox consists of the fact that helium in the Earth's atmosphere seems to be produced (via radioactive decay of uranium and thorium) faster than it is lost by escaping from the upper atmosphere. The realization that some helium could be ionized, and therefore escape the Earth along open magnetic field lines near the magnetic poles (the 'polar wind'), is one possible solution to the paradox.

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