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#19H.     The Magnetopause -- History

  (Files in red–history)


18. Solar Wind

  18H.Solar Wind obs.

18A. Interplan. Field

18B. Heliosphere.

19. Magnetopause

    19H.Chapman, 1930

20.Global Structure

21. Lagrangian pts.

22. "Wind" s/c

23. The Tail

24. Substorms

25. Auroral Currents

  25H. Birkeland Currents
    By the end of the 19th century at least some disturbances of the Earth's magnetic field could be traced to the Sun. Some seemed to follow flares, others showed their solar origin by tending to recur at intervals of 27 days, the Sun's rotation period.

      But how did the Sun exert its influence?

    Early ideas that the Sun sent out streams of electrons (which also produced the aurora) were given up when it was realized that the unbalanced negative electric charge of such electrons would completely disrupt the process.

    The Chapman-Ferraro Cavity

       Then in 1930 a different idea was proposed by Sidney Chapman in England and by his younger associate Vincent Ferraro: that the Sun sent out huge clouds of electrically neutral plasma, and that magnetic storms arose when those clouds enveloped the Earth. Many magnetic storms were observed to begin with a "sudden commencement," a small step-like jump in the magnetic field observed all over the world, taking just a minute or so. Chapman and Ferraro proposed that such jumps marked the cloud's arrival.

   They realized that the strong field of the Earth would hold off the cloud, carving a cavity in the cloud in which the Earth and its magnetic field would be confined (see drawing above, from their 1931 article). They also speculated that a ring current would then be set up, though they had no clear idea of the way it happened.

   The theory of the "Chapman-Ferraro Cavity" proved to be prophetic, except for one important detail: the flow of plasma from the Sun was not confined to isolated clouds, but went on all the time, in the form of the solar wind. Denser and faster clouds, such as arise from coronal mass ejections (see corona), were later identified as the real cause of sudden commencements.

  Explorer 12

       The magnetopause itself was first observed in 1961 by NASA's Explorer 12. Many satellites have since then studied and probed it--notably, Europe's HEOS 1 and 2 (1975-6) above the poles, as well as NASA's ISEE-3 (1983) and Japan's Geotail (1992-4), extended missions which, during the marked years, probed the distant tail region, up to distances

      Further reading:

  • Ferraro, Vincent C.A., "The Birth of a Theory" (an account of the beginnings of the Chapman-Ferraro theory), p. 14-18 in Sidney Chapman, Eighty, by S.-I. Akasofu, B. Fogle and B. Haurwitz, U. of Colorado Press, Boulder, 1969.

  • Cahill, Lawrence J., Jr., "Early study of the boundary of the geomagnetic field" (an account of the Explorer 12 observations), in Physics of the Magnetopause, B.U.Ö.Sonnerup and P. Song, editors, Amer. Geophys. Union, Washington, D.C. 1995.

Questions from Users:
            ***     Does our magnetic field stop the atmosphere from getting blown away?
                  ***     Blocking of the Solar Wind by our Moon?

Next Stop: #20.  Structure of the Earth's Magnetosphere

Last updated 25 November 2001
Re-formatted 3-13-2006