article: Mar 29 2010 - More slow-slip events in the Gisborne region
Following a dearth of slow-slip events in 2009, the GeoNet continuous GPS network has recorded new slow-slip events off the east coast of the North Island between January and March of this year.
Normally the interface between the subducting Pacific Plate and the overlying New Zealand crust is locked, which causes the Gisborne region to be pushed slowly westwards (at a few millimetres per year) due to the westward motion of the Pacific Plate. But during slow-slip events the locking is temporarily released, allowing the overlying crust to move back eastwards at rates of a few millimetres per day. GNS Science geodesists have modelled the surface movements at a number of GPS stations in the region and have determined how much movement must have taken place at the interface in order to get the surface observations. The modelling has revealed three events over the past three months. The first two events occurred during a similar time period:
The third event is currently under way:
Maps of the inferred subduction interface slips are shown at right:
| ![]() The two areas of slow-slip occurring during mid-January to mid-February (dashed contours show the depth to the interface of the two plates). | ![]() The area of slow-slip occurring during March. |

Locations of the four GPS stations shown on the plot.

A plot showing the daily positions of four of the continuous GPS sites in the Hawke's Bay to East Cape region. The usual motion of these sites is slowly towards the west. But when a slow-slip event occurs on the plate interface it causes nearby GPS stations to shift as much as 30 millimetres to the east over a period of days or weeks. The first (northernmost) event starts in mid-January as shown by the change in motion of site CNST. This event takes place over a time period of about 3 weeks. While this event is still happening the second (southernmost) event starts at the end of January and lasts for a few days. This event can be seen on station MAHI. Then, in mid March, a bigger event takes place in between the first two. The third event shows especially strongly at sites PARI and GISB, but is also detected at MAHI and CNST.



