Modeling of Flux Rope Coronal Mass Ejections

By A. Thernisien, R. Howard, A. Vourlidas. 2006

470 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/4785e944a6272d3ba592b9cf1fb8c7af84fcfa1a

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In Astronomy and Astrophysics

1. M. Temmer
2. N. Lugaz
3. A. Vourlidas
4. A. Thernisien
5. J. Davies
6. W. Manchester IV
7. R. Howard
8. D. Webb

In Molecular Biology

1. A. Thernisien
2. M. Temmer
3. N. Lugaz
4. A. Vourlidas
5. J. Davies
6. C. Farrugia
7. D. Webb
8. T. Howard

Citations in the corpus

• Topological Evolution of a Fast Magnetic Breakout CME in Three Dimensions (2008, background): “Recent forward modeling of CME density structures to produce synthetic line-of-sight coronagraph emission show density enhancements of, on average, 7 times background streamer densities are required to fit the bright edges of a number of CME events (Thernisien et al. 2006).”
• RECONSTRUCTING CORONAL MASS EJECTIONS WITH COORDINATED IMAGING AND IN SITU OBSERVATIONS: GLOBAL STRUCTURE, KINEMATICS, AND IMPLICATIONS FOR SPACE WEATHER FORECASTING (2010, methodology): “CME coronagraph images can be well reproduced by a forward modeling technique with a geometric model (Thernisien et al. 2006, 2009).”
• QUANTITATIVE MEASUREMENTS OF CORONAL MASS EJECTION-DRIVEN SHOCKS FROM LASCO OBSERVATIONS (2008, methodology): “…the shock strength, as presented in § 3, and the analysis of the 3D morphology and orientation of the white light shock using the Solar Corona Raytrace (SCR), a software package that simulates the appearance of various 3D geometries in white light coronagraph images (Thernisien et al. 2006).”
• IMPLEMENTATION OF THE GRADUATED CYLINDRICAL SHELL MODEL FOR THE THREE-DIMENSIONAL RECONSTRUCTION OF CORONAL MASS EJECTIONS (2011, methodology): “Thernisien et al. (2006) used it to fit a sample of 34 CMEs observed with LASCO and 26 CMEs observed with STEREO–SECCHI (Thernisien et al. 2009).”
• Coronal Mass Ejections: Observations (2012, methodology): “D information on CMEs, including forward modeling (e.g., Thernisien et al., 2006; Wood et al., 2009), tie-pointing (e.g., Mierla et al., 2009), and inverse reconstruction (Antunes et al., 2009).”
• CONNECTING SPEEDS, DIRECTIONS AND ARRIVAL TIMES OF 22 CORONAL MASS EJECTIONS FROM THE SUN TO 1 AU (2014, methodology): “…model, also known as “Graduated Cylindrical Shell” (GCS) model, is a very well tested tool, available in the IDL SolarSoft package, for deriving the initial directions and speeds of CMEs in the fields of view of the STEREO/COR2 coronagraph, covering 2.5–15.6 R⊙ (Thernisien et al. 2006, 2009).”
• THE LONGITUDINAL PROPERTIES OF A SOLAR ENERGETIC PARTICLE EVENT INVESTIGATED USING MODERN SOLAR IMAGING (2011, unknown): “Part of this pileup results from the white-light integration of plasma located on the curved surface of erupting transients (Chen et al. 1997; Thernisien et al. 2006).”
• Ensemble Modeling of CMEs Using the WSA–ENLIL+Cone Model (2015, methodology): “Other stereoscopic methods for determining the kinematic properties of CMEs include those by Thernisien, Howard, and Vourlidas (2006), Lugaz et al. (2010), and Davies et al. (2013).”
• NUMERICAL SIMULATION OF AN EUV CORONAL WAVE BASED ON THE 2009 FEBRUARY 13 CME EVENT OBSERVED BY STEREO (2009, background): “Patsourakos & Vourlidas (2009) show a fit of the 3D CME model of Thernisien et al. (2006, 2009) to the COR1-A data for this event at 06:05 UT.”
• How Many CMEs Have Flux Ropes? Deciphering the Signatures of Shocks, Flux Ropes, and Prominences in Coronagraph Observations of CMEs (2012, methodology): “s snapshot image. The full movie is available online. methods which demonstrated that a 3D geometric representation of a FR-like shape could account for the observed CME density envelopes and shapes (Thernisien, Howard, and Vourlidas, 2006). This issue has now been consolidated with the successful a”