Catalogs of solar wind types and their role in solar-terrestrial physics

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The magnetosphere response to interplanetary drivers depends on their type. The reliability of their identification affects the сonclusions based on the analysis of the relationships between the solar wind and the magnetosphere. In this paper, we analyze the list of moderate and strong geomagnetic storms and their interplanetary sources for the period 2009–2019 presented by Qiu S. et al. It is shown that some of the events in this list were defined incorrectly, and their interpretation differs in ~20 % of cases from our catalog by Yermolaev et al. (http://www.iki.rssi.ru/omni/) for the solar wind types Sheath, ICME, and CIR, and in ~28 % of cases from the Richardson and Cane catalog for ICME. Using the uncorrected list of Qiu S. et al. can lead to incorrect identification of interplanetary drivers of magnetic storms and false conclusions. It is recommended to use the classification of interplanetary drivers from catalogs of events accepted by the scientific community as reference ones.

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Sobre autores

I. Lodkina

Space Research Institute, Russian Academy of Sciences

Autor responsável pela correspondência
Email: irina-priem@mail.ru
Rússia, Moscow

Yu. Yermolaev

Space Research Institute, Russian Academy of Sciences

Email: yermol@iki.rssi.ru
Rússia, Moscow

A. Khokhlachev

Space Research Institute, Russian Academy of Sciences

Email: irina-priem@mail.ru
Rússia, Moscow

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2. Fig. 1. Time course of the parameters of the interplanetary medium and magnetospheric indices from August 27 to September 3, 2017 (see description in the text). Event No. 134 from the list [32], with a minimum at 12:00 on August 31, 2017 with Dst = –50 nT, according to the catalog [31] falls within the Ejecta interval

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3. Fig. 2. The same as in Fig. 1. Event No. 66 of the list [32], with a minimum on 09.XI.2013 09:00 with Dst = –80 nT, according to the catalog [31] falls on the Sheath interval

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4. Fig. 3. The same as in Fig. 1. Event No. 58 of the list [32], with a minimum of MB at 10.VII.2013 22:00 with Dst = –56 nT, according to the catalog [31] falls on the Ejecta interval

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5. Fig. 4. The same as in Fig. 1. Event No. 39 of the list [32], with a minimum of MB on 3.IX.2012 11:00 with Dst = –69 nT, according to the catalog [31] falls on the Sheath interval

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6. Fig. 5. Same as in Fig. 1. Event No. 22 of the list [32], with a minimum of MB on 25.I.2012 11:00 with Dst = –75 nT, according to the catalog [31] falls within the CIR interval

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