Magnetic flux ropes: Would we know one if we saw one?

S. E. Gibson, B. C. Low, K. D. Leka, Y. Fan, L. Fletcher

Research output: Contribution to journalConference articlepeer-review

2 Scopus citations

Abstract

There has been much debate lately about whether twisted magnetic flux ropes exist in the corona. When asked for observational evidence of them, the temptation is to show images of apparently twisted structures (e.g. see Figure 1). However, we must be very careful of projection effects in interpreting these observations. Two critical aspects of understanding how we might observe flux ropes are 1) the 3D nature of the flux rope, and 2) physically, which bits are visible and for what reasons? In this paper we will use a simple but physically reasonable 3D analytic model to address, these two issues, and develop techniques that can in future be used on more general models, both analytic and numerical.

Original languageEnglish
Pages (from-to)265-268
Number of pages4
JournalEuropean Space Agency, (Special Publication) ESA SP
Issue number505
StatePublished - Oct 2002
EventProceedings of the Magnetic Coupling of the solar Atmosphere Euroconference and IAU Colloquium 188 - Santorini, Greece
Duration: Jun 11 2002Jun 15 2002

Keywords

  • CMEs
  • Magnetic flux ropes
  • Solar corona

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