Prediction of magnetic orientation in driver gas associated -Bz events

Details Prediction of magnetic orientation in driver gas associated -Bz events Prediction of magnetic orientation in driver gas associated -Bz events

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....97.3151h&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. A3, March 1, 1992, p. 3151-3157.

Physics

14

Earth Magnetosphere, Flux Transfer Events, Interplanetary Magnetic Fields, Solar Corona, Solar Wind, Stellar Mass Ejection, International Sun Earth Explorers, Interplanetary Medium, Magnetic Field Reconnection, Prominences, Solar Flares, Solar Terrestrial Interactions

Scientific paper

The source regions of five strong -Bz events detected at 1 AU for which solar sources were identified by Tang et al. (1989) and Tsurutani et al. (1992) are investigated in order to determine whether the magnetic orientation of driver gas in the interplanetary medium observed at the earth can be predicted when its solar source is identified. Three -Bz events were traced to flare-associated coronal mass ejections (CMEs), one to an eruptive prominence associated CME, and one to three possible solar sources. The computed magnetic orientations at the candidate 'release height' (the height where the front of a CME ceases to accelerate) above the flare sites associated with CMEs show the existence of the expected southward field component. It is concluded that the magnetic orientation in flare-associated CME generated driver gas may be predictable.

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