Abstract
A complex catalogue of high speed streams produced by coronal holes and their effects in the terrestrial magnetosphere – the so-called geomagnetic storms – for Solar Cycle 24 (2009 to 2019) is presented here. This catalogue is structured in three parts describing the high-speed stream characteristics, the interplanetary magnetic field state, and the properties of the associated geomagnetic storms. The catalogue is available online at http://www.geodin.ro/varsiti/.
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The Catalogue of High Speed Streams Associated with Geomagnetic Storms during Solar Cycle 24 is available online at: http://www.geodin.ro/varsiti/.
References
Akasofu, S.I.: 1981, Energy coupling between the solar wind and the magnetosphere. Space Sci. Rev. 28, 121.
Cerrato, Y., Saiz, E., Cid, C.: 2012, Terrestrial Magnetosphere, 177. ADS.
Cid, C., Saiz, E., Cerrato, Y.: 2012, Geomagnetic Storms and Substorms, 207. ADS.
Domingo, V., Fleck, B., Poland, A.I.: 1995, The SOHO mission: an overview. Solar Phys. 162, 1. DOI. ADS.
Gerontidou, M., Mavromichalaki, H., Daglis, T.: 2018, High-speed solar wind streams and geomagnetic storms during Solar Cycle 24. Solar Phys. 293, 131. DOI. ADS.
Gonzalez, W.D., Joselyn, J.A., Kamide, Y., Kroehl, H.W., Rostoker, G., Tsurutani, B.T., Vasyliunas, V.M.: 1994, What is a geomagnetic storm? J. Geophys. Res. 99, 5771. DOI. ADS.
Grandin, M., Aikio, A.T., Kozlovsky, A.: 2019, Properties and geoeffectiveness of solar wind high-speed streams and stream interaction regions during Solar Cycles 23 and 24. J. Geophys. Res. 124, 3871. DOI. ADS.
Gupta, V., Badruddin: 2010, High-speed solar wind streams during 1996 – 2007: sources, statistical distribution, and plasma/field properties. Solar Phys. 264, 165. DOI. ADS.
Joselyn, J.A., Tsurutani, B.T.: 1990, Geomagnetic sudden impulses and storm sudden commencements: a note on terminology. Eos Trans. 71, 1808. DOI. ADS.
King, J.H., Papitashvili, N.E.: 2005, Solar wind spatial scales in and comparisons of hourly Wind and ACE plasma and magnetic field data. J. Geophys. Res. 110, A02104. DOI. ADS.
Kuklin, G.V.: 1976, Cyclical and secular variations of solar activity. Symp. Int. Astron. Union 71, 147. DOI.
Lindblad, A., Lundstedt, H.: 1981, A catalogue of high speed plasma streams in the solar wind. Solar Phys. 74, 197. DOI. ADS.
Lindblad, B.A., Lundstedt, H.: 1983, A catalogue of high-speed plasma streams in the solar wind 1975 – 78. Solar Phys. 88, 377. DOI. ADS.
Lindblad, B.A., Lundstedt, H., Larsson, B.: 1989, A third catalogue of high-speed plasma streams in the solar wind – data for 1978 – 1982. Solar Phys. 120, 145. DOI. ADS.
Maris, G., Maris, O.: 2010, Rapid solar wind and geomagnetic variability during the ascendant phases of the 11-yr solar cycles. In: Kosovichev, A.G., Andrei, A.H., Rozelot, J.-P. (eds.) Solar and Stellar Variability: Impact on Earth and Planets 264, 359. DOI. ADS.
Maris, G., Maris, O.: 2011, Fast solar wind and geomagnetic variability during the descendant phase of the 11-yr solar cycle. In: Zhelyazkov, I., Mishonov, T. (eds.) Amer. Inst. Physics C.S. 1356, 177. DOI. ADS.
Maris, G., Maris, O.: 2012, In: Maris, G., Demetrescu, C. (eds.) High Speed Streams in the Solar Wind During the 23rd Solar Cycle, Research Signpost Publ., Trivandrum, 97.
Maris, O., Maris, G.: 2005, Specific features of the high-speed plasma stream cycles. Adv. Space Res. 35, 2129. DOI. ADS.
Mavromichalaki, H., Vassilaki, A.: 1998, Fast plasma streams recorded near the Earth during 1985 – 1996. Solar Phys. 183, 181. DOI. ADS.
Mavromichalaki, H., Vassilaki, A., Marmatsouri, E.: 1988, A catalogue of high-speed solar-wind streams: further evidence of their relationship to \(\text{A}_{p}\)-index. Solar Phys. 115, 345. DOI. ADS.
Muntean, G.M., Besliu-Ionescu, D., Dobrica, V.: 2018, Complex catalogue of high speed streams and geomagnetic storms during Solar Cycle 24 (2009 – 2016). In: VarSITI Newsletter 17, 5.
Pesnell, W.D., Thompson, B.J., Chamberlin, P.C.: 2012, The Solar Dynamics Observatory (SDO). Solar Phys. 275, 3. DOI. ADS.
Phillips, J.L., Bame, S.J., Barnes, A., Barraclough, B.L., Feldman, W.C., Goldstein, B.E., Gosling, J.T., Hoogeveen, G.W., McComas, D.J., Neugebauer, M., Suess, S.T.: 1995, Ulysses solar wind plasma observations from pole to pole. Geophys. Res. Lett. 22, 3301. DOI. ADS.
Sykora, J.: 1992, The green corona, the solar wind and geoactivity. Solar Phys. 140, 379. DOI. ADS.
Wang, C., Han, J.P., Li, H., Peng, Z., Richardson, J.D.: 2014, Solar wind-magnetosphere energy coupling function fitting: results from a global MHD simulation. J. Geophys. Res. 119, 6199. DOI. ADS.
Wanliss, J.A., Showalter, K.M.: 2006, High-resolution global storm index: Dst versus SYM-H. J. Geophys. Res. 111, A02202. DOI. ADS.
Zhang, J., Richardson, I.G., Webb, D.F., Gopalswamy, N., Huttunen, E., Kasper, J.C., Nitta, N.V., Poomvises, W., Thompson, B.J., Wu, C.-C., Yashiro, S., Zhukov, A.N.: 2007, Solar and interplanetary sources of major geomagnetic storms (\(\text{Dst}\leq-100~\text{nT}\)) during 1996 – 2005. J. Geophys. Res. 112, A10102. DOI. ADS.
Acknowledgments
This work has been supported by a VarSITI Grant from 2017. We thank Daniela Lacatus and Alin Paraschiv for their help with programming and running issues. We also thank Ovidiu Mariş for making this software available to our team. We acknowledge the use of OMNI data that was obtained from the GSFC/SPDF OMNIWeb interface at https://omniweb.gsfc.nasa.gov. We also acknowledge the use of SYM-H data that was retrieved from http://wdc.kugi.kyoto-u.ac.jp/aeasy/index.html.
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Besliu-Ionescu, D., Maris Muntean, G. & Dobrica, V. Complex Catalogue of High Speed Streams Associated with Geomagnetic Storms During Solar Cycle 24. Sol Phys 297, 65 (2022). https://doi.org/10.1007/s11207-022-01998-3
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DOI: https://doi.org/10.1007/s11207-022-01998-3