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Department of Physics and Astronomy, Michigan State University National Superconducting Cyclotron Laboratory

project1-group9

This is an old revision of the document!

HAℓF

Roles

  • Analysis: Alexander Dombos
  • Code: Fei Yuan
  • Parameter: Heiko Möller

Topic

(Preliminary)

Simulate the effects of a near-Earth supernova explosion at 10 parsec (the “kill radius”) and the resulting collision of the blast with solar wind. Will the supernova reach 1 AU? How does the answer depend on the:

  • supernova explosion energy,
  • distance, and
  • interstellar density?
project1-group9.1401516216.txt.gz · Last modified: 2014/05/31 02:03 by yuan

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