A new Method for Determining the Interplanetary Current-Sheet Local Orientation

Details A new Method for Determining the Interplanetary Current-Sheet Local Orientation A new Method for Determining the Interplanetary Current-Sheet Local Orientation

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003soph..213..147b&link_type=abstract

Solar Physics, v. 213, Issue 1, p. 147-172 (2003).

Physics

1

Scientific paper

In this work we have developed a new method for determining the interplanetary current sheet local parameters. The method, called `HYTARO' (from Hyperbolic Tangent Rotation), is based on a modified Harris magnetic field. This method has been applied to a pool of 57 events, all of them recorded during solar minimum conditions. The model performance has been tested by comparing both, its outputs and noise response, with these of the `classic MVM' (from Minimum Variance Method). The results suggest that, despite the fact that in many cases they behave in a similar way, there are specific crossing conditions that produce an erroneous MVM response. Moreover, our method shows a lower noise level sensitivity than that of MVM.

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