Double flux rope structure of magnetic clouds?

Details Double flux rope structure of magnetic clouds? Double flux rope structure of magnetic clouds?

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471..127v&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 127-130 (1999).

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Interplanetary Magnetic Fields

Scientific paper

Vandas et al. (1) reported that some observations of magnetic clouds exhibit features characteristic of spheroidal clouds (spheromaks) rather than of a simple flux rope, namely specific full sinusoidal profiles of magnetic field components or double-peak magnetic field magnitude profiles. On the other hand, numerous other facts stress a flux rope structure of magnetic clouds (energetic particle observations, multi-spacecraft measurements, association with eruptive prominences) over a detached plasmoid (spheromak). We analyze several cases of magnetic clouds and suggest that a double flux rope structure of these objects is common and solves this puzzle.

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