Sources of geomagnetic storms for solar minimum and maximum conditions during 1972–2000

By I. G. Richardson, E. Cliver, H. Cane. 2001

235 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/29fd0d37ea0e863e1a0ba9d1f825b2930d282559

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. J. Borovsky
2. I. G. Richardson
3. H. Cane
4. R. Forsyth
5. N. Srivastava
6. P. Venkatakrishnan
7. M. Denton
8. M. Owens

In Molecular Biology

1. J. Borovsky
2. I. G. Richardson
3. H. Cane
4. M. Owens
5. N. Srivastava
6. P. Venkatakrishnan
7. R. Forsyth
8. M. Denton

Citations in the corpus

• 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].”
• Solar cycle changes in coronal holes and space weather cycles (2002, background): “the primary cause of the observed solar cycle trends in the IMF strength [e.g., Luhmann et al., 1993; Richardson et al., 2001].”
• The Heliospheric Magnetic Field (2013, background): “Magnetic fields in ICME sheaths can frequently be strong enough to trigger geomagnetic activity in their own right (Owens et al., 2005), with a quarter (Richardson et al., 2001) to a half (Tsurutani et al., 1988) of all geomagnetic storms potentially attributable to ICME sheaths.”
• Solar wind drivers of geomagnetic storms during more than four solar cycles (2012, background): “In past studies (Richardson 2006; Richardson et al. 2000, 2001, 2002), 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…”
• Differences between CME‐driven storms and CIR‐driven storms (2006, background): “[4] The occurrence rate of CMEs peaks strongly during solar maximum [Webb, 1991; Yashiro et al., 2004], so storms during solar maximum tend to be CME-driven storms [Richardson et al., 2001].”
• EUHFORIA: European heliospheric forecasting information asset (2018, background): “In particular coronal mass ejections (CMEs) large magnetized clouds of plasma that erupt frequently from the Sun constitute the main drivers of adverse conditions in the inner heliosphere (e.g., Richardson et al., 2001).”
• Solar and interplanetary sources of major geomagnetic storms during 1996–2002 (2004, background): “Several workers, for example, Gosling et al. [1991], Tsurutani and Gonzalez [1997], and Richardson et al. [2001] , have discussed this aspect in much detail over various periods of the solar activity cycle.”