Physics of the Neupert Effect: Estimates of the Effects of Source Energy, Mass Transport, and Geometry Using RHESSI and GOES Data
By A. Veronig, John C. Brown, B. R. Dennis, R. Schwartz, L. Sui, A. Tolbert. 2005
156 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/77ebbd0235839b78746f6c09878df5dabf16981e
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Citations in the corpus
- An Observational Overview of Solar Flares (2011, background): “These data includea circularly polarized component (Veronig et al. 2005; Bone et al. 2007), establishing t e presence of non-thermal electrons, visible in the whole loop through unpolarized thermal emission and consistent with the high density needed for the coronal thick target (Bone et al. 2007).”
- Implications of X-ray Observations for Electron Acceleration and Propagation in Solar Flares (2011, background): “…of the “theoretical Neupert effect,” i.e., comparisons of the beam power supply of hard X-ray-emitting electrons and the thermal energy of evaporated plasma observed in soft X-rays, found it to strongly depend on the lowenergy cutoff to the non-thermal electron distribution (Veronig et al. 2005).”
- Double Coronal Hard and Soft X-Ray Source Observed by RHESSI: Evidence for Magnetic Reconnection and Particle Acceleration in Solar Flares (2007, background): “This type of correlation is known as the Neupert effect (Neupert 1968) and has been observed in many (but not all) flares (Dennis & Zarro 1993; Veronig et al. 2005; Liu et al. 2006b).”
- Hard X-ray emission from the solar corona (2008, background): “…the standard impulsive-phase pattern characterized by bright hard X-ray footpoints (Hoyng et al 1981; Hudson and Ryan 1995), the Neupert effect (Neupert 1968; Dennis and Zarro 1993; Veronig et al 2005b), and the soft-hard-soft spectral pattern2 (Parks and Winckler 1969; Hudson and Fárńık 2002).”
- Updated Expressions for Determining Temperatures and Emission Measures from Goes Soft X-Ray Measurements (2005, background): “…of the plasma that produces the soft X–rays, and these physical quantities are of great importance: from them, the energetics of solar flares and other energy releases can be deduced, and their time variations can be interpreted directly in terms of physical models (e.g., Veronig et al., 2005).”