The sun at solar minimum: Nort - South asymmetry of the polar coronal holes

Geophysical Research Letters

Volumn 29, Issue 8, 2002, Pages

  Zhang, J ^a,b   Woch, J ^a   Solanki, S K ^a   Von Steiger, R ^c  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^c INTERNATIONAL SPACE SCIENCE INSTITUTE   (Switzerland)

Author keywords

[No Author keywords available]

Indexed keywords

DATA REDUCTION; MAGNETIC FLUX; SUN; WIND; SOLAR ENERGY;

SOLAR SURFACE;

GEOPHYSICS; SOLAR WIND;

SOLAR CYCLE; SOLAR WIND;

FLUX DENSITIES; ION COMPOSITION; IONIC CHARGE; KINETIC PROPERTIES; NORTH-SOUTH ASYMMETRY; SOLAR ACTIVITY CYCLES; SOLAR SURFACES; SOLAR WIND SPEED;

EID: 0037092249     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (16)

1. An analytic solar magnetic field model
2. Helium and minor ions in the corona and solar wind-dynamics and charge states
3. The symmetry of the heliospheric current sheet as observed by Ulysses during the fast latitude scan
4. The heliospheric magnetic field at solar minimum: Ulysses observations from pole to pole
5. The southern high-speed stream-Results from the SWICS Instrument on Ulysses
6. The solar wind ion composition spectrometer
7. Solar wind ionic charge states during the Ulysses pole-to-pole pass
8. A coronal hole and its identification as the source of a high velocity solar wind stream
9. Solar wind observations over Ulysses' first full polar orbit
10. Spatial structure of the solar wind and comparisons with solar data and models
11. Ulysses at 50 deg South: Constant immersion in the high-speed solar wind
12. Large-scale structure of the interplanetary medium
13. Recent observations of the heliospheric magnetic field at Ulysses: Return to low latitude
14. Evidence of a North-South asymmetry in the heliosphere associated with a southward displacement of the heliospheric current sheet
15. Composition of the solar wind
16. Composition of quasi-stationary solar wind flows from Ulysses/Solar wind ion composition spectrometer