Irregular Magnetic Pulsations - Generation, Propagation, and Transformation

Details Irregular Magnetic Pulsations - Generation, Propagation, and Transformation Irregular Magnetic Pulsations - Generation, Propagation, and Transformation

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsm43b1323w&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM43B-1323

Physics

2753 Numerical Modeling, 2772 Plasma Waves And Instabilities (2471), 2790 Substorms, 7836 Mhd Waves And Instabilities (2149, 2752, 6050)

Scientific paper

Low frequency magnetic signals are commonly observed during periods of enhanced Magnetospheric activity. Both Pi1B and Pi2 magnetic pulsations have been shown to correlate strongly with the onset of substorms in the magnetotail, and some authors have considered them manifestations of the same phenomena. However, recent analyses [Arnoldy, 1998; Posch 2007] have concluded that Pi1B and Pi2 signals most likely arise from different physical processes. In this paper, we present the results of theoretical and numerical investigations into the Pi1B and Pi2 phenomena and attempt to reconcile certain recent observations [e.g. Kepko, 2002; Lessard, 2006] with the existing theoretical framework.

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