X-ray sources and magnetic reconnection in the X3.9 flare of 2003 November 3

By Astrid Veronig, M. Karlický, B. Vršnak, M. Temmer, Jasmina Magdalenic, Brian R. Dennis, W. Otruba, W. Pötzi. 2006

136 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/e1bf38e0c1a8a810dd5943d0eae947ecc594dc1b

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

In Molecular Biology

1. Wei Liu
2. V. Petrosian
3. M. Temmer
4. Qingrong Chen
5. L. Sui
6. N. Vilmer
7. Heng Ji
8. H. Hudson

Citations in the corpus

• Sixty-five years of solar radioastronomy: flares, coronal mass ejections and Sun–Earth connection (2008, background): “While the coronal source (interpreted as the upper anchor of the current sheet) initially remains stationary, the loop-top source initially moves downward (see another example in Veronig et al. 2006).”
• Hard X-ray emission from the solar corona (2008, background): “The prototype of this class is the event of 23 July 2002 (Lin et al 2003; Asai et al 2006), and the events of 3 November 2003 10 UTC (Veronig et al 2006) and 24 August 2002 may also belong to this category.”
• 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 energy dispersion is consistent with previous observations (e.g., Veronig et al. 2006) and in line with the expected picture that higher loops are newly energized and thus are hotter and/or host nonthermal electrons of harder spectra, while lower loops are previously energized and have…”
• An Observational Overview of Solar Flares (2011, background): “Several further reported events confirm this pattern (e.g.,Liu et al. 2004; Sui et al. 2004; Veronig et al. 2006; Joshi et al. 2007).”
• Solar Flares: Magnetohydrodynamic Processes (2011, background): “…now recognized as the common properties of LDE flares: The temperature distribution is somewhat chaotic in the early phase when the flare started, while in the late phase the temperature is systematically higher near the edge of the cusp-shaped loop (Veronig et al., 2006, and references therein).”
• Double Coronal Hard and Soft X-Ray Source Observed by RHESSI: Evidence for Magnetic Reconnection and Particle Acceleration in Solar Flares (2007, background): “Due to its low brightness and/or technical difficulties, X-ray imaging spectroscopy of the weaker coronal source was not available or has not been studied for the above RHESSI events (Sui & Holman 2003; Sui et al. 2004; Veronig et al. 2006; Li & Gan 2007).”