Reconstruction of magnetic clouds in the solar wind: Orientations and configurations
By Qiang Hu, B. Sonnerup. 2002
282 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/6af30a3bbcc56bd45ddac771e53db54d48da1161
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Citations in the corpus
- The Plasma and Suprathermal Ion Composition (PLASTIC) Investigation on the STEREO Observatories (2008, methodology): “More recent approaches include reconstruction of the magnetic field, flux tube orientation, etc., based on the GradShafranov equation (Hu and Sonnerup 2002), and using kinematic expansions of the clouds (Riley and Crooker 2004).”
- Constraints on the global structure of magnetic clouds: Transverse size and curvature (2006, methodology): “Initially designed for the study of the terrestrial magnetopause [e.g., Hau and Sonnerup], the GS technique can be applied to flux-rope reconstruction [e.g., Hu and Sonnerup, 2002].”
- Fitting Flux Ropes to a Global MHD Solution: A Comparison of Techniques. Appendix 1 (2004, methodology): “…of the magnetopause (Sonnerup and Guo, 1996; Hau and Sonnerup, 1999; Hu and Sonnerup, 2000), and subsequently applied to flux rope observations (Hu and Sonnerup, 2001, 2002; Hu et al., 2003), the Grad–Shafranov reconstruction (GSR) technique makes two basic assumptions: (1) that the structure…”
- ON SUN-TO-EARTH PROPAGATION OF CORONAL MASS EJECTIONS (2013, methodology): “We reconstruct the in situ ICME structure using a Grad–Shafranov (GS) technique (Hau & Sonnerup 1999; Hu & Sonnerup 2002), which has been validated by well (but not too much) separated multi-spacecraft measurements (Liu et al. 2008a; Möstl et al. 2009).”
- RECONSTRUCTING CORONAL MASS EJECTIONS WITH COORDINATED IMAGING AND IN SITU OBSERVATIONS: GLOBAL STRUCTURE, KINEMATICS, AND IMPLICATIONS FOR SPACE WEATHER FORECASTING (2010, methodology): “Initially designed for the study of the terrestrial magnetopause (e.g., Hau & Sonnerup 1999), the Grad-Shafranov (GS) technique can be applied to flux-rope reconstruction (e.g., Hu & Sonnerup 2002).”
- Kinematic Treatment of Coronal Mass Ejection Evolution in the Solar Wind (2004, background): “So far, only three events have been analyzed, including a double flux rope (Hu & Sonnerup 2002; Hu et al. 2003).”
- The Physical Processes of CME/ICME Evolution (2017, background): “The rotation of the field is suggestive of a flux rope geometry (e.g., Lepping et al. 1990; Hu and Sonnerup 2002; Liu et al. 2008a), while the occasional presence of counter-streaming electrons suggest the magnetic field remains attached to the Sun at both ends (e.g., Gosling et al. 2001).”