Hard X-ray emission from the solar corona

By S. Krucker, M. Battaglia, P. Cargill, L. Fletcher, H. Hudson, A. MacKinnon, S. Masuda, L. Sui, M. Tomczak, A. Veronig and 2 more. 2008

242 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/6aa09c1aa42bafac4a5d1d3b782d0d120e995496

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. H. Hudson
3. V. Petrosian
4. Wei Liu
5. Astrid Veronig
6. L. Fletcher
7. S. Krucker
8. Brian R. Dennis

In Molecular Biology

1. M. Temmer
2. Wei Liu
3. V. Petrosian
4. Gordon D. Holman
5. N. Vilmer
6. Heng Ji
7. H. Hudson
8. L. Fletcher

Citations in the corpus

• Global Properties of Solar Flares (2011, background): “The implied spatial scales of this trapping may be large (e.g., Krucker et al. 2008), and have long durations (e.g., Figure 3).”
• An Observational Overview of Solar Flares (2011, background): “The following recent reviews of observations of flare and related phenomena, including theory, are also recommended for further reading: Priest & Forbes (2002); Aschwanden (2002); Benz (2008); Krucker et al. (2008a); Vršnak & Cliver (2008); Schrijver (2009).”
• 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).”
• Recent Advances in Understanding Particle Acceleration Processes in Solar Flares (2011, background): “Both types of emission indicate the presence of electron acceleration in the pre-flare phase, which is often accompanied by X-ray emission from a thermal source in the corona (Krucker et al. 2008a; Fletcher et al. 2011).”
• ELECTRON ACCELERATION BY MULTI-ISLAND COALESCENCE (2010, background): “Because magnetic reconnection is a possible mechanism of the energy release process, particle acceleration may also occur through magnetic reconnection, although difficulties remain when trying to interpret observations (Miller et al. 1997; Krucker et al. 2008; Benz 2008, and references therein).”
• COMBINED STEREO/RHESSI STUDY OF CORONAL MASS EJECTION ACCELERATION AND PARTICLE ACCELERATION IN SOLAR FLARES (2010, background): “This means that the HXR flux entirely originates from the coronal source (e.g. Krucker et al. 2008).”
• Deducing Electron Properties from Hard X-ray Observations (2011, background): “Treating these observations as evidence for a hot coronal region (Krucker et al. 2008; Tomczak 2009) produced by the primary energy release process, and electron precipitation from this primary acceleration region into the dense chromosphere, Machado et al. (1982) studied the energetics of…”
• Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares (2011, background): “In fact, these coronal hard X-ray sources can extend to high energies (up to ∼800 keV, Krucker et al. 2008b) and seem to be non-thermal in origin, thus making them of great interest in locating and understanding the particle acceleration process.”
• The Relationship Between Solar Radio and Hard X-ray Emission (2011, background): “Coronal HXR emission is almost certainly present in most flares but difficult to observe, and a recent comprehensive review is devoted to this subject (see Krucker et al. 2008a).”