Ulysses' second fast-latitude scan: Complexity near solar maximum and the reformation of polar coronal holes

Geophysical Research Letters

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

  McComas, D J ^a   Elliott, H A ^a   Gosling, J T ^a   Reisenfeld, D B ^a   Skoug, R M ^a   Goldstein, B E ^a   Neugebauer, M ^a   Balogh, A ^a  

^a SOUTHWEST RESEARCH INSTITUTE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ORBITS; SUN; WIND;

MAGNETIC POLARITY;

GEOPHYSICS;

ASTROPHYSICS; SOLAR WIND;

EID: 0036558588     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001gl014164     Document Type: Article

References (19)

1. The magnetic field investigation on the Ulysses mission: Instrumentation and preliminary scientific results
2. The Ulysses solar wind plasma experiment
3. Ulysses observations of a recurrent high speed solar wind stream and the heliomagnetic streamer belt
4. The southern high-speed stream: Results from the SWICS instrument on Ulysses
5. Bidirectional solar wind electron heat flux events
6. Latitude variation of solar wind corotating stream interaction regions: Ulysses
7. Coronal mass ejections at high heliographic latitudes: Ulysses
8. The northern edge of the band of solar wind variability: Ulysses at ∼4.5 AU
9. Ulysses' return to the slow solar wind
10. Ulysses' rapid crossing of the polar coronal hole boundary
11. Solar wind observations over Ulysses' first full polar orbit
12. Ulysses observations of the irregularly structured mid-latitude solar wind during the approach to solar maximum
13. Ulysses' second orbit: Remarkably different solar wind
14. Solar wind from high latitude coronal holes at solar maximum
15. UVCS observations of a high-latitude coronal hole with high oxygen temperatures and the next solar cycle polarity
16. Ulysses' solar wind plasma observations from peak southerly latitude through perihelion and beyond
17. Ulysses observations of Alfven waves in the southern and northern solar hemispheres
18. Composition of quasi-stationary solar wind flows from SWICS/Ulysses
19. The solar cycle variation of coronal mass ejections and the solar wind mass flux