Differences between CME‐driven storms and CIR‐driven storms

By J. Borovsky, M. Denton. 2006

613 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/06bc0c0978537faf14e938164da63d2c1ec36be8

How researchers see this paper

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In Astronomy and Astrophysics

1. Wen Li
2. Tuija I. Pulkkinen
3. M. Hudson
4. R. Thorne
5. Pete Riley
6. S. Gibson
7. Janet C. Green
8. M. Owens

In Molecular Biology

1. Tuija I. Pulkkinen
2. P. Démoulin
3. Jeff Forbes
4. R. S. Nerem
5. B. Lavraud
6. S. Cranmer
7. M. Owens
8. Pete Riley

Citations in the corpus

• Earth's Van Allen Radiation Belts: From Discovery to the Van Allen Probes Era (2019, background): “…which drive geomagnetic activity and variations in outer zone electron flux (e.g., Baker et al., 2019; Benacquista et al., 2018; Borovsky & Denton, 2006; Hudson et al., 2008; Kilpua et al., 2015; Reeves et al., 2003; Turner et al., 2019; Yuan & Zong, 2012), are shown in Figure 5, along…”
• Altered solar wind-magnetosphere interaction at low Mach numbers: Coronal mass ejections (2008, background): “This saturation also shows up in a number of geomagnetic indices [e.g., Weimer et al., 1990; Nagatsuma, 2004; Borovsky and Denton, 2006a]. ha l-0 03 77 24 0, v er si on 1 - 21 A pr 2 00 9 A number of physical explanations have been suggested in the literature [Shepherd, 2007].”
• Use of POES SEM-2 observations to examine radiation belt dynamics and energetic electron precipitation into the atmosphere (2010, background): “[4] Recently there has been much interest in the varying responses of the radiation belt to HSSWS and ICMEs [Borovsky and Denton, 2006].”
• Geoeffective Properties of Solar Transients and Stream Interaction Regions (2017, background): “The number of recurrent, generally small to medium CIR/HSS-driven magnetic storms peaks in the declining phase of solar activity cycle (e.g., Tsurutani et al. 1995; Gonzalez et al. 1999; Borovsky and Denton 2006; Zhang et al. 2008; Richardson and Cane 2012).”
• Space Weather: Terrestrial Perspective (2007, background): “The CIRs seldom have fast shocks or continuous, strongly southward IMF Bz, and thus drive only moderate magnetospheric activity (Alves et al., 2006; Borovsky and Denton, 2006).”
• Geomagnetic storms driven by ICME- and CIR-dominated solar wind (2006, background): “A recent report by Borovsky and Denton [2006] contains a review of the differences between CME- and CIR-dominated solar wind and examines the respective signatures of each in a number of regions, including the solar wind, the magnetosphere, and the auroral zone.”
• A statistical look at plasmaspheric drainage plumes (2008, background): “About 66% of all high-speed-streamdriven (CIR-driven) storms and about 38% of all CMEdriven storms satisfy these conditions [Borovsky and Denton, 2006a].”
• Multispacecraft observation of magnetic cloud erosion by magnetic reconnection during propagation (2012, background): “…(ICMEs), are magnetized plasma structures that play a pivotal role in solar-terrestrial interaction [Gosling, 1993; Wimmer-Schweingruber et al., 2006; Borovsky and Denton, 2006; Foullon et al., 2007; Gopalswamy et al., 2007; Lavraud and Borovsky, 2008;Möstl et al., 2010; Richardson and Cane, 2010].”
• Rotating solar coronal holes and periodic modulation of the upper atmosphere (2008, background): “They are most prevalent at low solar latitudes during the declining phase of solar maximum and in solar minimum and are stable structures that can persist for many solar rotations [e.g., Borovsky and Denton, 2006; Vršnak et al., 2007].”
• Origins of the Ambient Solar Wind: Implications for Space Weather (2017, background): “…apparently modest space-weather impacts from fast streams and CIRs (compared to CMEs) they have the potential for increased significance because they can persist over long times and are likely to repeat over multiple solar rotations (see, e.g., Sibeck and Richardson 1997; Borovsky and Denton 2006).”
• On the relationship between relativistic electron flux and solar wind velocity: Paulikas and Blake revisited (2010, background): “Recently much attention has been given to understanding how different solar wind drivers produce different types of responses in radiation belt electron fluxes [see Borovsky and Denton, 2006; Morley et al., 2010].”
• Generation of 100‐year geomagnetically induced current scenarios (2012, methodology): “Both storms were generated by major solar coronal mass ejection events, known to be the most significant 5 of 19 driver of large GIC [Borovsky and Denton, 2006; Kataoka and Pulkkinen, 2008; Huttunen et al., 2008].”