Abstract
Although this chapter is a continuation of the discussion of solar coronal loops of Chapter 15, it can be read independently. As we shall see, the channeling of loops is even more astonishing than what we found in the previous chapter. The huge size of the phenomenon makes loop Physics totally inaccessible to laboratory experiments.1
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References
See P. Lorrain, D. Redžić, S. Koutchmy, J. McTavish, O. Koutchmy, Solar coronal loops as self-channeled proton beams, Solar Physics, submitted (2005).
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(2006). Case Study: Solar Coronal Loops as Self-Channeled Proton Beams II. In: Magneto-Fluid Dynamics. Astronomy and Astrophysics Library. Springer, New York, NY. https://doi.org/10.1007/978-0-387-47290-4_16
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DOI: https://doi.org/10.1007/978-0-387-47290-4_16
Publisher Name: Springer, New York, NY
Print ISBN: 978-0-387-33542-1
Online ISBN: 978-0-387-47290-4
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