Temperatures of Extreme-Ultraviolet-emitting Plasma Structures Observed by the Transition Region and Coronal Explorer
- 18 February 2002
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 567 (2) , L159-L163
- https://doi.org/10.1086/340003
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Evidence for Nonuniform Heating of Coronal Loops Inferred from Multithread Modeling ofTRACEDataThe Astrophysical Journal, 2000
- The Magnetic Helicity Sign of Filament ChiralityThe Astrophysical Journal, 2000
- Time Variability of the “Quiet” Sun Observed withTRACE. II. Physical Parameters, Temperature Evolution, and Energetics of Extreme‐Ultraviolet NanoflaresThe Astrophysical Journal, 2000
- Active Region Loops Observed with SUMER on Board theSOHOThe Astrophysical Journal, 2000
- High-resolution Imaging of the Solar Chromosphere/Corona Transition RegionThe Astrophysical Journal, 1999
- Extreme-Ultraviolet Jets and Hα Surges in Solar MicroflaresThe Astrophysical Journal, 1999
- High-resolution Observations of Plasma Jets in the Solar CoronaSolar Physics, 1999
- Observations of Transition Region PlasmaSolar Physics, 1999
- What is Moss?Solar Physics, 1999
- Elemental abundances in the upper solar atmospherePhysica Scripta, 1992