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Thomas Stroman (2)and Ken-Ichi Nishikawa (3) ((1) Institute of Nuclear Physics PAN

Identifiers

  • name variant Thomas Stroman (2)and Ken-Ichi Nishikawa (3) ((1) Institute of Nuclear Physics PAN 0.60 · backfill

Papers (1)

  1. Production of Magnetic Turbulence by Cosmic Rays Drifting Upstream of Supernova Remnant Shocks astro-ph · 2008 · author #3

Mentions

  • 0802.2185 #3 · backfill · confidence 0.70 Thomas Stroman (2)and Ken-Ichi Nishikawa (3) ((1) Institute of Nuclear Physics PAN

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