Ulysses in the south polar cap at solar maximum: Heliospheric magnetic field

Geophysical Research Letters

Volumn 28, Issue 22, 2001, Pages 4159-4162

  Smith, E J ^a   Balogh, A ^b   Forsyth, R J ^b   McComas, D J ^c  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

^c SOUTHWEST RESEARCH INSTITUTE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EXTRAPOLATION; MAGNETIC FIELDS; MAGNETIC FLUX; WIND; MAGNETISM; SOLAR WIND;

SOLAR WIND;

GEOPHYSICS; MAGNETIC POLARITY;

MAGNETOSPHERE; SOLAR WIND;

CURRENT SHEETS; FIELD COMPONENTS; HELIOSPHERIC MAGNETIC FIELDS; MAGNETIC SECTORS; RADIAL DISTANCE; RADIAL EXPANSIONS; SOLAR WIND INTERACTIONS; SOUTH POLAR REGION;

EID: 0035891815     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001GL013471     Document Type: Article

References (14)

1. Origin of the solar wind: Theory
2. The behavior of the open magnetic flux of the sun
3. Latitudinal variation of the underlying heliospheric magnetic field: Comparison of Ulysses first and second orbits
4. Large-scale structure of the heliospheric magnetic field: 1976-1991
5. Ulysses observations of the irregularly structured mid-latitude solar wind during the approach to solar maximum
6. Ulysses' second orbit: Remarkably different solar wind
7. Simultaneous observations of solar energetic particle events by IMP-8 and the Ulysses COSPIN high energy telescope at high solar latitudes
8. Sources of the solar wind at solar activity maximum
9. Energetic particle characteristics in the high latitude heliosphere near solar maximum
10. Ulysses observations of the radial magnetic field component: Absence of a latitude gradient
11. Radial and azimuthal components of the heliospheric magnetic field: Ulysses observations
12. Latitudinal dependence of the radial IMF component-Coronal imprint
13. Radial evolution of density structure in the solar corona