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With 11 years of Geotail measurements we construct a model of plasma sheetBy, depending on IMF By, coordinates X,Y andgeodipole tilt angle. At midnight and pre-midnight local timesBy is positively correlated with tilt (positive in summer).Thus in summer By is shifted towards positive valuesand in winter towards negative values, so thatup to several nT could be added to the IMF influence.The dawn side plasma sheet By generally does not exhibit any tiltdependence, but within 15 RE the weaker negative correlation with tilt was revealed.The tilt dependence is just a useful parametrization and several mechanismsactually affecting plasma sheet By were previously suggested.In particular, similar coupling between tilt and IMF Bywas earlier found in the ionospheric convection patterns.Besides this average response, extreme By (|By|>5 nT, By>IMF By) wereoften observed (up to 20–25% of cases during solar maximum and in the pre-midnightsector within 20 RE). They can not be explained by our statistical model and arepreliminary interpreted as an "over-reaction" of the magnetosphere in someindividual events. Large By field radically changes dynamics ofthe current sheet and has to be taken into account during substorm-relatedstudies

Dipole tilt effects in plasma sheet &lt;I&gt;B&lt;sub&gt;y&lt;/sub&gt;&lt;/I&gt;: statistical model and extreme values

Dipole tilt effects in plasma sheet <I>B<sub>y</sub></I>: statistical model and extreme values