Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998

By O. S. Cyr, R. Howard, N. Sheeley, S. Plunkett, D. Michels, S. Paswaters, M. Koomen, G. Simnett, Barbara J. Thompson, J. Gurman and 4 more. 2000

498 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/37865acee1a42f83a52ef2644894c5d293af6364

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In Astronomy and Astrophysics

1. Nat Gopalswamy
2. M. Temmer
3. B. Vršnak
4. D. Webb
5. T. Howard
6. S. Yashiro
7. R. Howard
8. A. Vourlidas

Citations in the corpus

• Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption (2004, methodology): “Firstly, it is an extension of previous statistical analyses of kinematics of large samples of CMEs (e.g. Hundhausen 1993; Hundhausen et al. 1994; Harrison 1995; St. Cyr et al. 1999, 2000; Moon et al. 2002; Gopalswamy et al. 2003, and references therein).”
• Visibility of coronal mass ejections as a function of flare location and intensity (2005, result): “Under the assumption of all metric type II bursts having associated CMEs, St. Cyr et al. [2000] carried out a preliminary analysis of the visibility function of LASCO CMEs.”
• Processes that Promote and Deplete the Exosphere of Mercury (2007, methodology): “The data from Skylab, SMM, Helios, Solwind, and SoHO indicate a correlation between sunspot numbers (SSN) and the CME occurrence rate (Hildner et al. 1976; Howard et al. 1986; Webb and Howard 1994; Cliver et al. 1994; Cyr et al. 2000; Gopalswamy et al. 2003).”
• A Statistical Study of Main and Residual Accelerations of Coronal Mass Ejections (2006, background): “The earlier study on CME acceleration by St. Cyr et al. (1999) did not show this either.”
• A Statistical Study of Two Classes of Coronal Mass Ejections (2002, background): “Res., 104, 24739 St. Cyr, O. C., Burkepile, J. T., Hundhausen, & Lecinski, A. R. 1999, J. Geophys.”
• AUTOMATED LASCO CME CATALOG FOR SOLAR CYCLE 23: ARE CMEs SCALE INVARIANT? (2008, background): “CME angular span, speeds, latitudes and masses have been measured and statistically analyzed (e.g. Yashiro et al. 2004; Cremades & St. Cyr 2007, and references therein).”
• COMPREHENSIVE ANALYSIS OF CORONAL MASS EJECTION MASS AND ENERGY PROPERTIES OVER A FULL SOLAR CYCLE (2010, methodology): “This resource has been used extensively to study various CME properties (St. Cyr et al. 2000; Yashiro et al. 2004; Gopalswamy et al. 2009).”
• Deflection of coronal mass ejection in the interplanetary medium (2004, background): “A solar coronal mass ejection (CME) is a large-scale eruption of the plasma and magnetic fields from the Sun (e.g., Howard et al., 1982, 1985; Hundhausen, 1988, 1993; Gosling, 1990, 1996; Webb et al., 2000; St. Cyr et al., 2000; Gopalswamy et al., 2000).”
• Coronal Mass Ejections: Observations (2012, methodology): “It has detected CMEs at a rate slightly higher than earlier observations, varying from around one per day around solar minimum to nearly five per day at solar maximum (St Cyr et al., 2000; Gopalswamy et al., 2005, 2006b).”
• Coronal Mass Ejections Associated with Impulsive Solar Energetic Particle Events (2001, background): “In the LASCO CME list compiled by St. Cyr and Plunkett,2 we identiÐed 12 candidate associations, including the 2000 May 1 event, based on a requirement for the Ðrst CME observation to be hr[2 before the electron injection time.”