Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption

By B. Vršnak, D. Ruždjak, D. Sudar, Nat Gopalswamy. 2004

133 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/af341a6096691cbd0a16645b70ceb66eaee76de7

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. M. Temmer
2. Nat Gopalswamy
3. B. Vršnak
4. S. Yashiro
5. N. Lugaz
6. R. Howard
7. A. Vourlidas
8. W. Manchester IV

In Oceanography

1. B. Vršnak
2. Nat Gopalswamy
3. W. Manchester IV
4. Tibor Török
5. D. Ruždjak
6. D. Sudar
7. Astrid Veronig
8. E. Kilpua

Citations in the corpus

• The CME-flare relationship: Are there really two types of CMEs? (2005, methodology): “…the case studies showing that the CME acceleration is closely related to the energy release in the associated flares (e.g., Kahler et al. 1988; Zhang et al. 2001; Gallagheret al. 2003; Neupert et al. 2001; Shanmugaraju et al. 2003; Subramanian et al. 2003; Zhang et al. 2004; Vršnak et al. 2004a).”
• The SOHO/LASCO CME Catalog (2009, background): “CMEs are subject to propelling and retarding forces in the corona and interplanetary medium (see e.g., Vršnak et al. 2004).”
• Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts (2008, background): “On the one hand, magnetic reconnection adds poloidal flux to the CME sustaining the Lorentz force which drives the CME acceleration (Chen 1996; Chen & Krall 2003; Vršnak et al. 2004).”
• The Origin, Early Evolution and Predictability of Solar Eruptions (2018, background): “Indeed, observations indicate that the driving force decreases approximately as r−α, where the exponent ranges between α ≈ 1 and 2 (Vršnak, 2001; Vršnak et al, 2004c; Vršnak, 2006).”
• The Physical Processes of CME/ICME Evolution (2017, background): “Second, that the Lorentz force driving the CME can sometimes significantly contribute to the CME dynamics up to large distances from the Sun (e.g., Vršnak et al. 2004; Temmer et al. 2011).”
• COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “Several authors found a correlation between the CME acceleration and the flare soft X-ray emission (Zhang et al. 2001, 2004; Zhang & Dere 2006; Vršnak et al. 2004; Maričić et al. 2007; Vršnak et al. 2007).”
• Solar flares, coronal mass ejections and solar energetic particle event characteristics (2016, background): “5 h) are most likely not associated with the given CME (Dougherty et al. 2002; Vršnak et al. 2004).”