Solar wind from high-latitude coronal holes at solar maximum

Geophysical Research Letters

Volumn 29, Issue 9, 2002, Pages 28-1-28-4

  McComas, D J ^a   Elliott, H A ^a   Von Steiger, R ^b  

^a SOUTHWEST RESEARCH INSTITUTE   (United States)

^b INTERNATIONAL SPACE SCIENCE INSTITUTE   (Switzerland)

Author keywords

[No Author keywords available]

Indexed keywords

FREEZING; WIND EFFECTS;

TRANSITION LAYERS;

GEOPHYSICS;

CORONA; SOLAR WIND;

EID: 0036558509     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001gl013940     Document Type: Article

References (17)

1. The Ulysses solar wind plasma experiment
2. The southern high-speed stream: Results from the SWICS instrument on Ulysses
3. Origin of the solar wind from composition data
4. The solar wind ion composition spectrometer
5. Bidirectional solar wind electron heat flux events
6. Latitude variation of solar wind corotating stream interaction regions: Ulysses
7. Ulysses' return to the slow solar wind
8. Solar wind observations over Ulysses' first full polar orbit
9. Ulysses observations of the irregularly structured mid-latitude solar wind during the approach to solar maximum
10. Coronal holes as a source of solar wind
11. Nature of the boundary between open and closed magnetic field regions at the Sun revealed by composition data and numerical models
12. Composition aspects of the upper solar atmosphere
13. Composition of quasi-stationary solar wind flows from SWICS/Ulysses
14. Evolution of coronal stream structure during the rising phase of solar cycle 23
15. Solar wind stream interfaces in corotating interaction regions: SWICS/Ulysses results
16. The transition between fast and slow solar wind from composition data
17. Heliospheric magnetic field configuration and its coronal sources