Interplanetary conditions leading to superintense geomagnetic storms (Dst ≤ −250 nT) during solar cycle 23

By E. Echer, W. D. Gonzalez, B. Tsurutani. 2008

150 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/fe779e91158355b072413d4eb74dbb420da8ac50

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In Astronomy and Astrophysics

1. E. Kilpua
2. A. Balogh
3. Ying Liu
4. R. Steiger

In Molecular Biology

1. E. Kilpua
2. A. Balogh
3. Ying Liu
4. R. Steiger

Citations in the corpus

• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “The most important large-scale solar wind structures that drive magnetic storms (e.g., Gosling et al. 1991; Crooker 2000; Huttunen et al. 2002; Zhang et al. 2007; Echer et al. 2008b; Richardson and Cane 2012) are shown schematically in Fig.”