Skip to main content

The Early History

  • Chapter
Magneto-Fluid Dynamics

Part of the book series: Astronomy and Astrophysics Library ((AAL))

  • 1311 Accesses

Abstract

Our story covers two and one half millennia. It starts with Thales of Miletus who wrote in −600 about the mineral magnetite. It ends with Gouy and Larmor who proposed at the beginning of the 20th century the concept of self-excited dy-namo to explain the existence of magnetic fields on the Sun. All this while, the pace was accelerating.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 129.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD 169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. References for this section about China: Haudricourt and Needham (1957, pp. 483–485); Hellemans and Bunch (1988, pp. 19, 37, 39, 75); Macdonald (1957, p. 1508); Needham and Ling (1954–1956, Vol. 1, p. 128, and Vol. 2, p. 576); Needham, Ling, and Robinson (1962, pp. 229–230, 232, 249–250, 279–280, 334); Sarton (1927–1948, Vol. 1, pp. 755–756, 764).

    Google Scholar 

  2. Needham, Ling, and Robinson (1962, p. 231); Sarton (1927–1948, Vol. 1, pp. 65, 71, 72).

    Google Scholar 

  3. Lenoble (1958, p. 325).

    Google Scholar 

  4. See Brothers Arnold and Potamian (1904). The authors provide many references to Latin and medieval writings, with quotations.

    Google Scholar 

  5. Pliny the Elder (1855, Chap. XXXIV, 137).

    Google Scholar 

  6. Beaujouan (1957, p. 573); Hellemans and Bunch (1988, p. 79); Needham, Ling, and Robinson (1962, pp. 230, 279–280); Sarton (1927–1948, Vol. 2, pp. 24, 385, 589, 592–593, 671).

    Google Scholar 

  7. Macdonald (1957, p. 1504); Needham, Ling, and Robinson (1962, pp. 229–230); Sarton (1927–1948, Vol. 2, p. 630).

    Google Scholar 

  8. Needham, Ling, and Robinson (1962, p. 330).

    Google Scholar 

  9. Arnold and Potamian (1904); Beaujouan (1957, p. 542); Hellemans and Bunch (1988, pp. 61, 81); Lenoble (1958, pp. 326–327); Merrill and McElhinny (1983, pp. v, 5); Sarton (1927–1948, Vol. 2, pp. 24, 630).

    Google Scholar 

  10. Fleming (1939, pp. 2–3); Malin (1989, pp. 7–8); Merrill and McElhinny (1983, pp. 6–7, 12). See also Physics Today (June 2000), p. 52. There exists an extensive site on Gilbert’s life and work at www.spof.gsfc.nasa.gov/earthmag/demagint.htm

    Google Scholar 

  11. Beaujouan (1957, p. 573).

    Google Scholar 

  12. Fleming (1939, p. 2); Hellemans and Bunch (1988, p. 99).

    Google Scholar 

  13. Merrill and McElhinny (1983, p. 6).

    Google Scholar 

  14. Malin (1989, p. 35).

    Google Scholar 

  15. Malin (1989, p. 21–22); Merrill and McElhinny (1983, p. 11).

    Google Scholar 

  16. Faraday (1852a,b,c, 1965); Gillispie (1970–1978).

    Google Scholar 

  17. Bork (1963); Domb (1979); Gillispie (1970–1978); Harman (1998); Heaviside (1950); Hunt (1991).

    Google Scholar 

  18. For the origin of the name Maxwell, see Gillispie (1970–1978).

    Google Scholar 

  19. Maxwell (1873).

    Google Scholar 

  20. Hunt (1991).

    Google Scholar 

  21. Gillispie (1970–1978).

    Google Scholar 

  22. Gillispie (1970–1978) attributes the discovery of the vector formulation to Lorentz (1853–1928) in 1895, eleven years after Heaviside.

    Google Scholar 

  23. Heaviside (1950), Sect. 22.6.

    Google Scholar 

  24. See Heaviside (1950).

    Google Scholar 

  25. Zeeman (1897).

    Google Scholar 

  26. Hale (1908).

    Google Scholar 

  27. Gouy (1912).

    Google Scholar 

  28. Larmor (1919).

    Google Scholar 

  29. Larmor (1929, 1934).

    Google Scholar 

  30. Gillispie (1970–1978).

    Google Scholar 

Download references

Rights and permissions

Reprints and permissions

Copyright information

© 2006 Springer Science+Business Media, LLC

About this chapter

Cite this chapter

(2006). The Early History. In: Magneto-Fluid Dynamics. Astronomy and Astrophysics Library. Springer, New York, NY. https://doi.org/10.1007/978-0-387-47290-4_1

Download citation

Publish with us

Policies and ethics