Solar active regions: SOHO/CDS and TRACE observations of quiescent coronal loops

By G. D. Zanna, Helen E. Mason. 2003

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In Astronomy and Astrophysics

Citations in the corpus

The multi-thermal emission in solar active regions (2013, methodology): “EUV spectroscopy with SOHO CDS also confirmed this (Del Zanna & Mason 2003).”
Elementary Loop Structures in the Solar Corona Analyzed from TRACE Triple-Filter Images (2005, methodology): “REFERENCES Arnaud, M., & Raymond, J. 1992, ApJ, 398, 394 Aschwanden, M. J. 2004, Physics of the Solar Corona—an Introduction (New York: Springer) Aschwanden, M. J., Alexander, D., Hurlburt, N., Newmark, J. S., Neupert, W. M., Klimchuk, J. A., & Gary, G. A. 2000a, ApJ, 531, 1129 Aschwanden, M. J., Ne”
Impulsive Phase Flare Energy Transport by Large-Scale Alfvén Waves and the Electron Acceleration Problem (2007, background): “Normal active-region loop densities are on the order of (1 3) ; 1015 cm 3 (Del Zanna & Mason 2003), and even postflare arcade loop measurements (Varady et al. 2000; Landi et al. 2003) are a few ; 1015 m 3, which might reasonably be taken as an upper limit for the preflare density in the flare…”
SDO/AIA response to coronal hole, quiet Sun, active region, and flare plasma (2010, background): “Analysis of this kind has been performed previously for the Transition Region and Coronal Explorer (TRACE; Handy et al. 1999) 173 Å and 195 Å passbands and the Extreme-ultraviolet Imaging Telescope (EIT; Delaboudinière et al. 1995) 171 Å, 195 Å and 284 Å passbands (cf., Del Zanna & Mason 2003; Del ”
An Ab Initio Approach to the Solar Coronal Heating Problem (2004, methodology): “For individual loops chosen from the simulated TRACE 171 image, that is too high by almost a factor of 10 for the 171 filter and a factor of 3 for the 195 filter, compared to the values given by Del Zanna & Mason (2003).”
High-precision density measurements in the solar corona I. Analysis methods and results for Fe XII and Fe XIII (2008, background): “The wavelength was revised to 195.179 Å by Del Zanna & Mason (2005) based on unpublished work by Fawcett (Del Zanna, private communication 2008).”
A rigidly rotating magnetosphere model for circumstellar emission from magnetic OB stars (2004, background): “High resolution images of the solar corona provide vivid evidence of how the complex solar magnetic field can structure and confine coronal plasma (e.g., Del Zanna & Mason 2003).”