Major geomagnetic storms (Dst<=-100~nT) generated by corotating interaction regions in 1996--2004

By I. Richardson, D. Webb, Jie Zhang, D. Berdichevsky, D. Biesecker, Justin C. Kasper, R. Kataoka, J. Steinberg, Barbara J. Thompson, C. Wu and 1 more. 2006

136 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/dae7e8da6010fbf7606b2391457ea88f456603f1

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In Astronomy and Astrophysics

1. Nat Gopalswamy
2. S. Yashiro
3. H. Cane
4. I. G. Richardson
5. S. Akiyama
6. M. Temmer
7. R. Schwenn
8. R. Howard

In Molecular Biology

1. Nat Gopalswamy
2. I. G. Richardson
3. H. Cane
4. S. Akiyama
5. S. Yashiro
6. T. Howard
7. D. Webb

Citations in the corpus

• Solar wind drivers of geomagnetic storms during more than four solar cycles (2012, background): “Geomagnetic activity associated with individual streams in 2003 has also been discussed by Richardson et al. (2006) and Tsurutani et al. (2011a).”
• Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963-2011) (2012, background): “…et al. 2001; Zhang et al. 2007; Echer et al. 2008; Richardson & Cane 2010, 2011a, and references therein), and also during the passage of high-speed streams past the Earth (e.g., Sheeley et al. 1976, 1977; Richardson 2006; Richardson et al. 2006; Tsurutani et al. 2006, and references therein).”
• Geoeffectiveness of halo coronal mass ejections (2007, background): “About 10% of strong storms are caused by CIRs, but the Dst values are generally not too far below 100 nT [see, e.g., Sheeley et al., 1976; Miyoshi and Kataoka, 2005; Richardson et al., 2006].”