Comparative analysis of geomagnetic events identified by various indices

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Аннотация

We presented the results of comparative analysis of geomagnetic events identified by various indices. A previously developed technique is used to identify magnetic storms by the Dst index. As a basis for identification, we chose the previously developed method for identifying geomagnetic storms based on the Dst index. A similar method was implemented to identify geomagnetic events by the ap and AE indices. Comparative analysis includes: (1) identification of common geomagnetic events identified by various indices; (2) identification of cases when an event is a strong geomagnetic disturbance by one of the indices (Dst, ap, AE) and is not a geomagnetic event by at least one of the two remaining indices; and (3) a comparative analysis of the diurnal and seasonal distribution of the number of geomagnetic events identified by different indices.

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Авторлар туралы

K. Ratovsky

Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences

Хат алмасуға жауапты Автор.
Email: ratovsky@iszf.irk.ru
Ресей, Irkutsk

M. Klimenko

Kaliningrad Branch of the Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation of the Russian Academy of Sciences

Email: ratovsky@iszf.irk.ru
Ресей, Kaliningrad

A. Vesnin

Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences

Email: ratovsky@iszf.irk.ru
Ресей, Irkutsk

K. Belyuchenko

Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences

Email: ratovsky@iszf.irk.ru
Ресей, Irkutsk

Yu. Yasyukevich

Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences

Email: ratovsky@iszf.irk.ru
Ресей, Irkutsk

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Әрекет
1. JATS XML
2. Fig. 1. Seasonal distribution of the number of Dst-storms (a), ap-storms (b) and AE-storms (c)

Жүктеу (311KB)
3. Fig. 2. Daily distribution of the number of Dst-storms (a), ap-storms (b) and AE-storms (c)

Жүктеу (293KB)

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