Plasma Astrophysics, Part II

Available
0
StarStarStarStarStar
0Reviews
Magnetic ?elds are easily generated in astrophysical plasma owing to its ?6 high conductivity. Magnetic ?elds, having strengths of order few 10 G, correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to ampli?cation of a small seed ?eld by a turbulent galactic dynamo. In several galaxies, like the famous M51, magnetic ?elds are well correlated (or anti-cor...
Read more
product_type_E-book
pdf
Price
135.00 £
Magnetic ?elds are easily generated in astrophysical plasma owing to its ?6 high conductivity. Magnetic ?elds, having strengths of order few 10 G, correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to ampli?cation of a small seed ?eld by a turbulent galactic dynamo. In several galaxies, like the famous M51, magnetic ?elds are well correlated (or anti-cor...
Read more
Follow the Author

Options

  • Formats: pdf
  • ISBN: 9780387688947
  • Publication Date: 31 Dec 2007
  • Publisher: Springer New York
  • Product language: English
  • Drm Setting: DRM