The density structure of a solar polar coronal hole
- 1 May 1999
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A5), 9781-9789
- https://doi.org/10.1029/1998ja900079
Abstract
No abstract availableKeywords
This publication has 34 references indexed in Scilit:
- CHIANTI - an atomic database for emission linesAstronomy and Astrophysics Supplement Series, 1997
- Electron Densities in the Solar Polar Coronal Holes from Density-Sensitive Line Ratios of [CLC]Si[/CLC] [CSC]viii[/CSC][CLC]and S [CSC]x[/CSC] [CLC][/CLC][/CLC]The Astrophysical Journal, 1997
- Effects of High Ion Temperatures on Spectral Line Diagnostics in the Source Region of the High‐Speed Solar WindThe Astrophysical Journal, 1997
- Emission Measures and Electron Densities for the Solar Transition RegionThe Astrophysical Journal, 1997
- EIT: Extreme-ultraviolet Imaging Telescope for the SOHO missionSolar Physics, 1995
- Effective collision strengths for Si IIIMonthly Notices of the Royal Astronomical Society, 1989
- Transition zone flows observed in a coronal hole on the solar diskThe Astrophysical Journal, 1989
- SI III line ratios in the sunThe Astrophysical Journal, 1983
- Theoretical atomic structure and electron scattering data for ions in the nitrogen isoelectronic sequence: MG VI, Si VIII, S x, A XII and Ca XIVMonthly Notices of the Royal Astronomical Society, 1980
- Densities in the quiet sun and polar coronal holes from EUV line ratios involving O III /1666.15 A/The Astrophysical Journal, 1978