Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 – 2009): Catalog and Summary of Properties

By I. G. Richardson, H. Cane. 2010

885 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/c7b78b3e58d62edc77ed7bd73c0915f67c755930

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. M. Temmer
2. N. Lugaz
3. I. G. Richardson
4. H. Cane
5. Jan Luhmann
6. J. Davies
7. Yuming Wang
8. C. Farrugia

In Molecular Biology

1. M. Temmer
2. I. G. Richardson
3. H. Cane
4. N. Lugaz
5. J. Davies
6. C. Farrugia
7. Jan Luhmann
8. M. L. Mays

Citations in the corpus

• The Interaction of Successive Coronal Mass Ejections: A Review (2016, background): “…was learnt from numerical simulations; however, there have been many reported detections of shocks propagating inside a magnetic cloud or magnetic ejecta at 1 AU (Wang et al., 2003a; Collier, Lepping, and Berdichevsky, 2007; Richardson and Cane, 2010a; Lugaz et al., 2015b; Lugaz et al., 2016).”
• > 25 MeV Proton Events Observed by the High Energy Telescopes on the STEREO A and B Spacecraft and/or at Earth During the First ∼ Seven Years of the STEREO Mission (2014, background): “It was also suggested by Wibberenz and Cane (2006) to be occurring during impulsive electron events.”
• CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU (2014, background): “…region in front of a magnetic driver, which is either an irregular structure or a large-scale magnetic flux rope (e.g. Burlaga et al. 1981; Bothmer & Schwenn 1998; Lynch et al. 2003; Leitner et al. 2007; Möstl et al. 2009a; Richardson & Cane 2010; Isavnin et al. 2013; Al-Haddad et al. 2013).”
• Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model (2015, methodology): “These included the Richardson and Cane (2010) ICME catalog5, and the Wind ICME catalog6 with circular flux rope model fitting (based on Hidalgo et al. (2000)).”
• Solar Orbiter (2012, background): “Observations at 1 AU, however, find that less than half of all ICMEs, even those associated with strong flares, have a flux rope structure (Richardson and Cane, 2004; Richardson and Cane, 2010; Kilpua et al., 2011).”
• Near-earth solar wind flows and related geomagnetic activity during more than four solar cycles (1963-2011) (2012, methodology): “The ICME identifications made in our previous studies (e.g., Richardson & Cane 1993; Richardson & Cane 1995; Richardson et al. 1997; Cane & Richardson 2003; Richardson & Cane 2010) have been incorporated into the solar wind classification.”