Geoefficiency and energy partitioning in CIR-driven and CME-driven storms
By N. Turner, W. Cramer, S. Earles, B. Emery. 2009
159 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/8d1acfbfd284f0bdad1e67e981d4f2987c0bfe16
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In Astronomy and Astrophysics
Citations in the corpus
- Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963-2011) (2012, background): “…valuable for studies of the magnetospheric and ionospheric response to different types of solar wind structures (e.g., Emery et al. 2009, 2011; Turner et al. 2009) and is available at the CEDAR workshop web site (http://cedarweb.hao. ucar.edu/wiki/index.php/Tools_and_Models:Solar_Wind_…”
- Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “The studies comparing coupling efficiency for different storm drivers (e.g., Turner et al. 2009; Yermolaev et al. 2010; Myllys et al. 2016) show that ICMEs, despite being the key drivers of intense geomagnetic storms, have on average the weakest coupling efficiency.”