On the Aerodynamic Drag Force Acting on Interplanetary Coronal Mass Ejections

By P. Cargill. 2004

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In Astronomy and Astrophysics

Citations in the corpus

Space weather: the solar perspective (2021, background): “This has consequences on the CME transit time and impact speed at planetary atmospheres (drag force; see Gopalswamy et al. 2000; Vršnak 2001; Cargill 2004; Vršnak 2006).”
The Interaction of Successive Coronal Mass Ejections: A Review (2016, methodology): “The potential full coalesence of two ejecta into one was discussed in a few studies (Odstrcil et al., 2003; Schmidt and Cargill, 2004; Chatterjee and Fan, 2013) but has not been investigated in details with realistic reconnection rates.”
The Physical Processes of CME/ICME Evolution (2017, methodology): “…(1) cd does not vary with distance (e.g., Cargill 2004), (2) ICME virtual-mass effect is not included (e.g., Bein et al. 2013; Feng et al. 2015; Cargill 2004; Tappin 2006), (3) solar wind properties are taken to be constant in time (e.g., Temmer et al. 2011), (4) and (5) the geometry of the…”
Deriving the radial distances of wide coronal mass ejections from elongation measurements in the heliosphere - application to CME-CME interaction (2009, background): “It is expected that fast shock waves can propagate inside preceding ejections (Schmidt and Cargill, 2004; Lugaz et al., 2005) and merge with the preceding shock waves.”
ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, background): “…by a viscous drag force (as solar gravity can be neglected), which is proportional to a drag coefficient, the CME cross section, the ambient solar wind density, and the square of the velocity difference between the CME and the solar wind (e.g., Cargill 2004; Vršnak et al. 2013; Žic et al. 2015).”
COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “After the magnetic driving force of the eruption ceases, the CME is slowed down by the drag force until its velocity adjusts to the speed of the solar wind (e.g. Cargill 2004; Manoharan 2006; Vršnak et al. 2008, and references therein).”
The association of coronal mass ejections with their effects near the Earth (2005, methodology): “This ongoing discussion has led Cargill (2004) to investigate the aerodynamic force acting on ICMEs by applying appropriate MHD simulations. He “assumes a drag force proportional to the square of the relative velocity, as has been used in hydrodynamic”. In that he differs from Vřsnak, 2001a who assu”
The Heliospheric Magnetic Field (2013, methodology): “…electrons released by the Jovian magnetosphere (Teegarden et al., 1974; Chenette et al., 1974) provide a point source in the heliosphere which can be used to infer magnetic connectivity to Jupiter and, hence, the large-scale structure of the HMF (Chenette, 1980; Moses, 1987; Owens et al., 2010).”
Propagation of Interplanetary Coronal Mass Ejections: The Drag-Based Model (2013, background): “where cd is the dimensionless drag coefficient (Cargill, 2004), A is the ICME cross-sectional area, ρw is the ambient solar-wind density, and M is the ICME mass.”