MEASUREMENTS OF THE CORONAL ACCELERATION REGION OF A SOLAR FLARE

By S. Krucker, H. S. Hudson, L. Glesener, Simon D. M. White, Satoshi Masuda, J. Wuelser, R. Lin. 2010

194 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/9cab652da3fe38b3e9cf1f69462ebf9cd80bf788

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In Astronomy and Astrophysics

1. M. Temmer
2. Wei Liu
3. H. Hudson
4. V. Petrosian
5. Qingrong Chen
6. Brian R. Dennis
7. L. Fletcher
8. Petr Jelínek

Citations in the corpus

• PARTICLE ACCELERATION AND PLASMA DYNAMICS DURING MAGNETIC RECONNECTION IN THE MAGNETICALLY DOMINATED REGIME (2015, background): “…shown strong particle acceleration and energy conversion during magnetic reconnection and the particle distribution often takes power-law distributions, requiring a particle acceleration mechanism that is dominated by nonthermal acceleration (Krucker et al. 2008, 2010; Krucker & Battaglia 2014).”
• The Relationship Between Solar Radio and Hard X-ray Emission (2011, background): “The radio spectrum in this event has a spectral peak near 10 GHz, i.e., much higher than in the Krucker et al. (2010) event, suggesting that effectively none of the radio emission is obscured from us.”
• Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, background): “2015) and could be related to the above-the-loop-top hard X-ray source (Masuda et al. 1994; Krucker et al. 2010; Oka et al. 2015), although the detailed acceleration process in such low Mach number and high-β shocks should be studied in more detail (for recent studies about electron acceleration at ”
• An Observational Overview of Solar Flares (2011, background): “In one case in particular, the data suggest that essentially all coronal electrons present in the source are non-thermal (Krucker et al. 2010), with mimi al remaining thermal distribution.”
• PLASMOID EJECTIONS AND LOOP CONTRACTIONS IN AN ERUPTIVE M7.7 SOLAR FLARE: EVIDENCE OF PARTICLE ACCELERATION AND HEATING IN MAGNETIC RECONNECTION OUTFLOWS (2013, background): “This indicates that the 25–50 keV Masuda-type loop-top source shown in Figure 3 is primarily nonthermal and likely a particle acceleration region itself (e.g., Liu et al. 2008; Krucker et al. 2010).”