Modeling 3-D solar wind structure

By D. Odstrcil. 2003

374 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/9097a4b23d314bd236c19d18c6c6525689fc2acc

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Citations in the corpus

The Open Flux Problem (2017, methodology): “The models were the empirical Wang–Sheeley–Arge (WSA) model (Arge et al. 2003) coupled with the Enlil Heliospheric MHD model (Odstrcil 2003) and the Magnetohydrodynamic Algorithm outside a Sphere (MAS) MHD model, also coupled with Enlil.”
The Physical Processes of CME/ICME Evolution (2017, methodology): “Falkenberg et al. (2010) and Vršnak et al. (2010, 2014) compared the DBM and ENLIL ICME arrival-time predictions, and found that results of the two models to be similar accurate.”
Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model (2015, methodology): “…of CMEs (see (Zhao and Dryer, 2014) and references therein), only the Wang-Sheeley-Arge (WSA) coronal model (Arge and Pizzo, 2000; Arge et al., 2004) coupled with the global heliospheric ENLIL solar wind model (Odstrčil, 2003) has been used extensively in space weather operations world-wide.”
Three-dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations (2008, methodology): “Images of numerical CME models have been made in this fashion before (Wu et al. 1999; Odstrcil 2003; Manchester et al. 2004a; Lugaz et al. 2005, e.g.).”
The Origin, Early Evolution and Predictability of Solar Eruptions (2018, methodology): “For example, ENLIL simulates the solar wind plasma and magnetic field only beyond 30R , i.e., the corona is ne- glected.”
MESSENGER Observations of Mercury's Magnetic Field Structure (2012, methodology): “An aberration angle was calculated for each MESSENGER orbit using Mercury’s instantaneous orbital speed and a mean solar wind speed of 405 km/s from the ENLIL model for the period 24 March to 12 December 2011 [Odstrcil, 2003].”
Mercury's magnetopause and bow shock from MESSENGER Magnetometer observations (2013, methodology): “Figure 8 shows the solar wind statistics at Mercury at the time of the bow shock crossings, obtained from averages of MESSENGER MAG observations of the IMF and from ENLIL model predictions of the solar wind density, speed, ram pressure, and Alfvén Mach number [Odstrcil, 2003; Baker et al., 2013].”