Acceleration in Fast Halo CMEs and Synchronized Flare HXR Bursts

By M. Temmer, Astrid Veronig, B. Vršnak, J. Rybák, P. Gömöry, S. Stoiser, D. Maričić. 2008

194 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/4ed38b511e0a015fd6cdaf942e9e87301e2fae88

How researchers see this paper

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In Astronomy and Astrophysics

1. M. Temmer
2. G. Aulanier
3. B. Vršnak
4. Wei Liu
5. P. Démoulin
6. V. Petrosian
7. H. Hudson
8. Qingrong Chen

In Molecular Biology

1. M. Temmer
2. Wei Liu
3. V. Petrosian
4. Qingrong Chen
5. P. Démoulin
6. Heng Ji
7. H. Hudson
8. L. Fletcher

Citations in the corpus

• PLASMOID EJECTIONS AND LOOP CONTRACTIONS IN AN ERUPTIVE M7.7 SOLAR FLARE: EVIDENCE OF PARTICLE ACCELERATION AND HEATING IN MAGNETIC RECONNECTION OUTFLOWS (2013, result): “This is in line with observed synchronous eruption accelerations and flare onsets (Zhang et al. 2001, 2002; Temmer et al. 2008; Liu et al. 2011a).”
• COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “…relationship between the large-scale CME acceleration and the energy release process in the associated flare (e.g. Lin 2004; Maričić et al. 2007; Temmer et al. 2008; Vršnak & Cliver 2008): After the magnetic structure looses equilibrium and starts rising, a current sheet is formed below…”
• OBSERVING FLUX ROPE FORMATION DURING THE IMPULSIVE PHASE OF A SOLAR ERUPTION (2011, background): “The impulsive acceleration phase of the CME coincides in time very well with the rise phase of the flare (also see, Burkepile et al. 2004; Temmer et al. 2008; Cheng et al. 2010a).”
• An Observational Overview of Solar Flares (2011, methodology): “But the extremely good correspondence in time between HXR bursts and both filament lift-off (Maričić et al. 2007;Temmer et al. 2008) and coronal “supra-arcade downflows” (Asai et al. 2004b) (interpreted as retracting flux tubes formed in reconnection behind a CME) does not really permit us to say…”
• CRITERIA FOR FLUX ROPE ERUPTION: NON-EQUILIBRIUM VERSUS TORUS INSTABILITY (2010, background): “…on, magnetic reconnection plays a key role in the eruption as the peak of the upward acceleration is typically found correlated with the peak of the hard X-rays and of the time derivative of soft X-rays flux (e.g. Neupert et al. 2001; Zhang et al. 2001; 2 Vršnak et al. 2004; Temmer et al. 2008).”