Dst (Disturbance Storm Time) is an index designed to measure the intensity of geomagnetic activity over the Atlantic region.
Original attempts for defining Dst were made by Kertz (1958 and 1964) and Sugiura (1964) with a derivation scheme first proposed by Sugiura and Hendricks (1967) and further improved by Sugiura and coworkers (1969) when it was adopted by the International Association for Geomagnetism and Aeronomy (IAGA). The definitive values of Dst are published by Data Analysis Center for Geomagnetism and Space Magnetism, Kyoto, Japan on behalf of the International Service for Geomagnetic Indices (ISGI), a service of IAGA.
The version presented here is an estimate, derived from measurements made at the near-equatorial magnetic observatory on Ascension Island (ASC), in the Atlantic. Dst (ASC) index is derived from the ASC one-minute horizontal magnetic field variations.
Following the method deployed for the derivation of the official Dst, the secular variation trend and solar quiet (Sq) diurnal variations are estimated and removed from the observatory measurements. The data are then transformed to the dipole equator equivalent, giving Dst (ASC).
About the data:
Data supplied here are real-time estimates derived by BGS and, unlike the definitive Dst, which is an hourly index, Dst (ASC) is computed for every one-minute.
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