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scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

scostep 2010 (stp12) - Leibniz-Institut für Atmosphärenphysik an der ...

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STP12 Abstracts<br />

Berlin, 12 - 16 July <strong>2010</strong><br />

SCOSTEP Symposium <strong>2010</strong><br />

Local Dst/Dcx indices: New space weather products from the SOTERIA project<br />

Mursula Kalevi, Holappa Lauri, Karinen Arto, Leik<strong>an</strong>ger Tore<br />

The Dst index is one of the most used geomagnetic indices that is constructed to monitor the<br />

most dramatic events in the near-Earth space, the geomagnetic storms. The Dst index is<br />

calculated as <strong>an</strong> average of disturb<strong>an</strong>ces observed at four low-latitude stations, roughly<br />

equally distributed in longitude. However, in addition to the ring current, other current<br />

systems like the tail current, magnetopause current <strong>an</strong>d partial ring current contribute to the<br />

Dst index. Therefore, the local disturb<strong>an</strong>ces at the four stations are very often quite different.<br />

Moreover, because of the problematic Dst recipe, the different Dst stations contribute to the<br />

Dst index with systematically different weights.<br />

We have calculated a revised version of the Dst index, the so called Dcx index, where the<br />

different stations contribute with equal weights. So far, the Dst/Dcx indices have been based<br />

only on four stations. Such a coarse longitudinal accuracy does not allow for a detailed study<br />

of the local time structure of storm time disturb<strong>an</strong>ces due to asymmetric current systems like<br />

the partial ring current <strong>an</strong>d the tail current. Therefore, we have increased the number of<br />

stations used to calculate the Dcx index to 16 stations. This longitudinally enh<strong>an</strong>ced index is<br />

called Dcx16. Within the FP7 SOTERIA project both the Dcx <strong>an</strong>d Dcx16 indices, together<br />

with all the 16 local Dcx indices observed at each contributing station will be made available.<br />

This offers <strong>an</strong> ample r<strong>an</strong>ge of new possibilities for detailed studies of storm time disturb<strong>an</strong>ces<br />

<strong>an</strong>d currents.

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