The role of CMEs and interplanetary shocks in IMF winding angle statistics

Details The role of CMEs and interplanetary shocks in IMF winding angle statistics The role of CMEs and interplanetary shocks in IMF winding angle statistics

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..382..502s&link_type=abstract

Proceedings of the eigth international solar wind conference: Solar wind eight. AIP Conference Proceedings, Volume 382, pp. 502

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1

Interplanetary Magnetic Fields, Planetary Bow Shocks, Interplanetary Shocks, Particle Emission, Solar Wind

Scientific paper

We examine the possible role of CMEs and interplanetary shocks in past analyses of the large-scale winding of the IMF by extracting CME and shock observations from the ISEE-3 dataset and analyzing periods of the disturbed and undisturbed solar wind separately. We use the full ISEE-3 dataset representing the entire L1 mission (1978-1982). We conclude that CMEs, the shocks upstream of CMEs and other interplanetary shocks are responsible for the apparent overwinding of the IMF spiral relative to the Parker prediction. The IMF winding angle asymmetry appears to be preserved after the removal of the interplanetary disturbances.

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