THREE-DIMENSIONAL SOLAR WIND MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID

By Xueshang Feng, Liping Yang, Changqing Xiang, S. Wu, Yufen Zhou, Dingkun Zhong. 2010

150 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/d267f2ede5a0c851e4cb41bb69975ac48b231763

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

1. Aaron Dotter
2. B. Paxton
3. Matteo Cantiello
4. J. Fuller
5. P. Marchant
6. R. Townsend
7. Adam S. Jermyn
8. R. Farmer

In Oceanography

1. Igor M. Sokolov
2. Tamas I. Gombosi
3. G. T'oth

Citations in the corpus

• Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation (2019, background): “For example, the Parker Solar Probe will provide new information on the flow of energy, structure, and dynamics of the closest star (Parker 1958a; Feng et al. 2010; Cranmer & Winebarger 2018; Gombosi et al. 2018) and the Daniel K. Inouye Solar Telescope will provide high temporal and spatial…”
• ALFVÉN WAVE SOLAR MODEL (AWSoM): CORONAL HEATING (2013, methodology): “…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 simulations to obtain 1 AU…”