The Relationship of the Chromosphere to the Lower Solar Transition Region
- 10 July 2004
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 609 (2), 1153-1163
- https://doi.org/10.1086/421235
Abstract
No abstract availableThis publication has 34 references indexed in Scilit:
- Properties of the Lower Transition Region: The Widths of Optically Allowed and Intersystem Spectral LinesThe Astrophysical Journal, 2004
- The O+ and O++ emission lines near 834 Å in the quiet sun solar spectrumGeophysical Research Letters, 2002
- CHIANTI—An Atomic Database for Emission Lines. IV. Extension to X‐Ray WavelengthsThe Astrophysical Journal Supplement Series, 2001
- Evidence for Nonuniform Heating of Coronal Loops Inferred from Multithread Modeling ofTRACEDataThe Astrophysical Journal, 2000
- A Comparison of Measurements of Solar Extreme‐Ultraviolet Spectral Line Intensities Emitted by C, N, O, and S Ions with Theoretical CalculationsThe Astrophysical Journal, 1999
- The Electron Pressure in the Solar Lower Transition Region Determined from Ovand SiiiiDensity‐sensitive Line RatiosThe Astrophysical Journal, 1998
- CHIANTI - an atomic database for emission linesAstronomy and Astrophysics Supplement Series, 1997
- Nonthermal velocities in the solar transition zone observed with the high-resolution telescope and spectrographSolar Physics, 1993
- The structure of the static corona and transition regionThe Astrophysical Journal, 1986
- A newly observed solar feature - Macrospicules in He II 304 AThe Astrophysical Journal, 1975