Heliopause imaging in EUV: Oxygen O+ ion 83.4‐nm resonance line emission
- 1 March 2000
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 105 (A3) , 5189-5200
- https://doi.org/10.1029/1999ja000345
Abstract
No abstract availableKeywords
This publication has 54 references indexed in Scilit:
- A new reference spectrum for the EUV irradiance of the quiet Sun: 1. Emission measure formulationJournal of Geophysical Research, 1998
- Ulysses' return to the slow solar windGeophysical Research Letters, 1998
- Effect of local interstellar medium hydrogen fractional ionization on the distant solar wind and interface regionJournal of Geophysical Research, 1995
- Detection of Interstellar Pick-Up Hydrogen in the Solar SystemScience, 1993
- Physical reasons and consequences of a three-dimensionally structured heliosphereSpace Science Reviews, 1991
- Ultraviolet spectroscopy and remote sensing of the upper atmosphereSpace Science Reviews, 1991
- The scattering rate of solar 834 Å radiation by magnetospheric O+ and O++Geophysical Research Letters, 1990
- The heliopauseReviews of Geophysics, 1990
- Plasmaspheric helium ion distribution from satellite observations of He II 304‐ÅGeophysical Research Letters, 1982
- Observational, reference and model data on solar EUV, from measurements on AE‐EGeophysical Research Letters, 1981