Evidence for Nonuniform Heating of Coronal Loops Inferred from Multithread Modeling ofTRACEData
- 1 October 2000
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 541 (2) , 1059-1077
Abstract
No abstract availableKeywords
This publication has 38 references indexed in Scilit:
- Time Variability of the “Quiet” Sun Observed withTRACE. II. Physical Parameters, Temperature Evolution, and Energetics of Extreme‐Ultraviolet NanoflaresThe Astrophysical Journal, 2000
- The Effect of Hydrostatic Weighting on the Vertical Temperature Structure of the Solar CoronaThe Astrophysical Journal, 2000
- Three‐dimensional Stereoscopic Analysis of Solar Active Region Loops. II.SOHO/EIT Observations at Temperatures of 1.5–2.5 MKThe Astrophysical Journal, 2000
- Three‐dimensional Stereoscopic Analysis of Solar Active Region Loops. I.SOHO/EIT Observations at Temperatures of (1.0–1.5) x 106KThe Astrophysical Journal, 1999
- A Nanoflare Explanation for the Heating of Coronal Loops Observed byYohkohThe Astrophysical Journal, 1997
- Cooling of solar flares plasmas. 1: Theoretical considerationsThe Astrophysical Journal, 1995
- Elemental abundances in the upper solar atmospherePhysica Scripta, 1992
- Plasma Loops in the Solar Corona1991
- The XUV structure of solar active regionsSolar Physics, 1982
- Spatial distribution of XUV emission and density in a loop prominenceSolar Physics, 1980