Abstract
This work is a continuation of paper [1], in which we discussed some incorrect approaches to the identification of large-scale types of solar wind and associated incorrect conclusions in the analysis of solar–terrestrial physics data. In this paper, we analyze the lists of 28 events of coronal mass ejection (CME) and 31 events of corotating interaction region (CIR) in 2013–2016 used by Shen et al. [2] to compare the responses of the Earth’s radiation belts to various interplanetary drivers. The interpretation of solar wind types in these lists differs both from our catalog [3] for Sheath, ICME, and CIR and from the catalog by Richardson and Cane [4] for CME. In addition, the authors of paper [2] do not distinguish the Sheath- and ICME-induced magnetic storms and include them in the general type of CME-induced storms. Our analysis has shown that, among the 28 events of CME-induced storms mentioned, 16 events belong to Sheath, 2 events to MC, 4 events to Ejecta, 2 events to CIR, and 4 events to undisturbed solar wind with shocks. The catalog [4], which also does not distinguish the Sheath and ICME, contains 18 of the 28 events presented in paper [2]. Among 31 CIR events presented by the authors of paper [2], according to our analysis, 25 events belong to CIR, 2 events to Sheath, and 4 events to undisturbed solar wind. In catalog [4], one of the 31 CIR events from paper [2] is presented as CME. Since the properties of CIR and Sheath compression regions are close, the conclusions of the authors of paper [2] on the properties of CIR-induced storms are only slightly distorted by the incorrect identification of stream types, whereas the conclusions concerning the CME-induced storms, which more than by a half represent the Sheath-induced storms, seem incorrect to us.
Similar content being viewed by others
REFERENCES
Yermolaev, Yu.I., Lodkina, I.G., Nikolaeva, N.S., et al., Some problems of identifying types of large-scale solar wind and their role in the physics of the magnetosphere, Cosmic Res., 2017, vol. 55, no. 3, pp. 178–189.
Shen, X.-C., Hudson, M.K., Jaynes, A., et al., Statistical study of the storm time radiation belt evolution during Van Allen Probes era: CME- versus CIR-driven storms, J. Geophys. Res.: Space Phys., 2017, vol. 122, pp. 8327–8339. doi 10.1002/2017JA024100
Yermolaev, Yu.I., Nikolaeva, N.S., Lodkina, I.G., and Yermolaev, M.Yu., Catalog of large-scale solar wind phenomena during 1976–2000, Cosmic Res., 2009, vol. 47, no. 2, pp. 81–94.
Richardson, I.G. and Cane, H.V., Near-Earth interplanetary coronal mass ejections during solar cycle 23 (1996–2009): Catalog and summary of properties, Sol. Phys., 2010, vol. 264, no. 1, pp. 189–237. https:// doi.org/10.1007/s11207-010-9568-6.
King, J.H. and Papitashvili, N.E., Solar wind spatial scales in and comparisons of hourly wind and ACE plasma and magnetic field data, J. Geophys. Res., 2004, vol. 110, no. A2, A02209. doi 10.1029/2004JA010804
Yermolaev, Y.I., Lodkina, I.G., Nikolaeva, N.S., and Yermolaev, M.Y., Dynamics of large-scale solar wind streams obtained by the double superposed epoch analysis, J. Geophys. Res.: Space Phys., 2015, vol. 120, no. 9, pp. 7094–7106.
Yermolaev, Y.I., Lodkina, I.G., Nikolaeva, N.S., and Yermolaev, M.Y., Dynamics of large-scale solar-wind streams obtained by the double superposed epoch analysis. 2. Comparisons of CIRs vs. Sheaths and MCs vs. Ejecta, Sol. Phys., 2017, vol. 292, no. 12, id 193. doi 10.1007/s11207-017-1205-1
Nikolaeva, N.S., Yermolaev, Yu.I., and Lodkina, I.G., Modeling the time behavior of the Dst index during the main phase of magnetic storms generated by various types of solar wind, Cosmic Res., 2013, vol. 51, no. 6, pp. 401–412.
Nikolaeva, N.S., Yermolaev, Yu.I., and Lodkina, I.G., Modeling of the corrected Dst*index temporal profile on the main phase of the magnetic storms generated by different types of solar wind, Cosmic Res., 2015, vol. 53, no. 2, pp. 119–127.
Nikolaeva, N.S., Yermolaev, Yu.I., Lodkina, I.G., and Yermolaev, M.Yu., Does magnetic storm generation depend on the solar wind type?, Geomagn. Aeron. (Engl. Transl.), 2017, vol. 57, no. 5, pp. 512–518.
ACKNOWLEDGMENTS
We are grateful to the developers of the OMNI database and ICME catalog [4] for giving us an opportunity to use the data. The OMNI data were obtained from the GSFC/SPDF OMNIWeb interface on the website http://omniweb.gsfc.nasa.gov and the ICME catalog data on the website http://www.srl.caltech. edu/ACE/ASC/DATA/level3/icmetable2.htm/. This work was supported by the Russian Science Foundation, project no. 16-12-10062.
Author information
Authors and Affiliations
Corresponding author
Additional information
Translated by Yu. Preobrazhensky
Rights and permissions
About this article
Cite this article
Lodkina, I.G., Yermolaev, Y.I., Yermolaev, M.Y. et al. Some Problems of Identifying Types of Large-Scale Solar Wind and Their Role in the Physics of the Magnetosphere: 2. Cosmic Res 56, 331–342 (2018). https://doi.org/10.1134/S0010952518050052
Received:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S0010952518050052