Low-dimensionality and predictability of solar wind and global magnetosphere during magnetic storms

Article, Preprint English OPEN
Zivkovic, Tatjana ; Rypdal, Kristoffer (2011)
  • Publisher: American Geopgysical Union (AGU)
  • Related identifiers: doi: 10.1029/2011JA016547
  • Subject: Physics - Space Physics | VDP::Mathematics and natural science: 400::Physics: 430::Space and plasma physics: 437 | VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437
    arxiv: Physics::Atmospheric and Oceanic Physics | Physics::Space Physics | Astrophysics::Solar and Stellar Astrophysics

This article is part of Tatjana Živkovics' doctoral thesis. Available in Munin at <a href=http://hdl.handle.net/10037/3231>http://hdl.handle.net/10037/3231</a> The storm index SYM-H, the solar wind velocity v, and interplanetary magnetic field Bz show no signatures o... View more
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