Stream structure and coronal sources of the solar wind during the May 12th, 1997 CME

By Charles N. Arge, Jan Luhmann, D. Odstrcil, C. Schrijver, Y. Li. 2003

337 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/fb039fdc4df30d4c37dc6584b375a19fc0f502f3

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In Astronomy and Astrophysics

1. W. Manchester IV
2. Tamas I. Gombosi
3. Igor M. Sokolov
4. Ilia I. Roussev
5. O. Cohen
6. D. Odstrcil
7. A. Pulkkinen
8. M. L. Mays

Citations in the corpus

• THREE-DIMENSIONAL SOLAR WIND MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID (2010, methodology): “Some empirical functions with various free parameters, similar to the above formula, have been employed to derive the solar wind speed near the Sun (Arge et al. 2004; Owens et al. 2005).”
• Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model (2015, methodology): “…the evolution 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…”
• A Semiempirical Magnetohydrodynamical Model of the Solar Wind (2007, methodology): “A particular example is the Wang-SheeleyArge (WSA) model (Arge & Pizzo 2000; Arge et al. 2003, 2004).”