A Semiempirical Magnetohydrodynamical Model of the Solar Wind

By O. Cohen, Igor M. Sokolov, Ilia I. Roussev, Charles N. Arge, W. Manchester IV, Tamas I. Gombosi, R. Frazin, H. Park, M. Butala, F. Kamalabadi and 1 more. 2007

170 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/8a2954dfc58954cb8e99b519355bc408fee0fc4d

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

In Molecular Biology

Citations in the corpus

MULTISPECTRAL EMISSION OF THE SUN DURING THE FIRST WHOLE SUN MONTH: MAGNETOHYDRODYNAMIC SIMULATIONS (2008, background): “MHD models that include the photospheric magnetic field as a boundary condition have existed for more than a decade (Usmanov 1993, 1996; Mikić & Linker 1996; Linker et al. 1999; Mikić et al. 1999; Roussev et al. 2003; Riley et al. 2006; Cohen et al. 2007).”
ALFVÉN WAVE SOLAR MODEL (AWSoM): CORONAL HEATING (2013, methodology): “…heliosphere MHD model prescribed by the empirical Wang–Sheeley–Arge (WSA) model (Arge & Pizzo 2000) was able to capture the 1 AU observations, while Cohen et al. (2007); Feng et al. (2010); van der Holst et al. (2010) used the WSA to prescribe the coupled corona and inner inner heliosphere…”
NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, methodology): “In order to simulate the CME event, we use the Solar Corona (SC) model developed at the University of Michigan (Roussev et al. 2003b; Cohen et al. 2007, 2008b).”
The Open Flux Problem (2017, methodology): “Simulations of the corona and solar wind with the Space Weather Modeling Framework (Tóth et al. 2005) have scaled input maps by factors of 2–4 to improve model-observational comparisons (Cohen et al. 2007; Jin et al. 2012; Oran et al. 2015).”
Slow Solar Wind: Observations and Modeling (2016, unknown): “Alternatively, a semi-empirical, variable polytropic index is used with somewhat better results (e.g., Cohen et al. 2007).”
Three-dimensional MHD Simulation of the 2003 October 28 Coronal Mass Ejection: Comparison with LASCO Coronagraph Observations (2008, methodology): “First, like those by Lugaz et al. (2007); Cohen et al. (2007), it is the first 3D numerical full MHD simulation to reproduce observed CMEs as they are magnetically driven from active regions in the low corona.”
THREE-DIMENSIONAL SOLAR WIND MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID (2010, methodology): “Using this method, Cohen et al. (2007, 2008) are able to reproduce well the fast and slow plasma streams of the solar wind.”