Sources of geomagnetic activity during nearly three solar cycles

By Ian G. Richardson, H. V. Cane, E. Cliver. 2002

207 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/0eb8501458eb731c47a6523a020c5637e7a12bd2

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In Astronomy and Astrophysics

Citations in the corpus

The Heliospheric Magnetic Field (2013, background): “Firstly, they drive the largest geomagnetic disturbances (Gosling, 1993; Richardson et al., 2002).”
Differences between CME‐driven storms and CIR‐driven storms (2006, background): “[8] It is well known that CIR-driven storms generally occur in the late declining phase of the solar cycle and that CME-driven storms tend to occur at solar maximum [Gonzalez et al., 1999; Yermolaev and Yermolaev, 2002; Richardson et al., 2001, 2002].”
A survey of interplanetary coronal mass ejections in the near-Earth solar wind during 1996-2002 (2003, background): “Another of our interests is the contribution of ICMEs to geomagnetic activity, both storms and long-term averages [e.g., Cane et al., 2000; Richardson et al., 2001a, 2002].”
Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963-2011) (2012, methodology): “In past studies (Richardson et al. 2000, 2001, 2002; Richardson 2006), we divided the near-Earth solar wind since 1972 into three basic flow types in order to assess, for example, the contribution of each type of solar wind flow to long-term (> ~solar rotation) averages of geomagnetic indices and…”
Solar and interplanetary sources of major geomagnetic storms during 1996–2002 (2004, background): “, to the geomagnetic activity has also been studied in details for three solar cycles (1972–2000) by Richardson et al. [2002]. [20] In the following section we discuss the characteristics of the interplanetary sources of major storms that occurred during 1996–2002.”