Latitudinal variation of the underlying heliospheric magnetic field direction: Comparison of the Ulysses first and second orbits

Space Science Reviews

Volumn 97, Issue 1-4, 2001, Pages 161-164

  Forsyth, R J ^a   Balogh, A ^a   Smith, E J ^b  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

CONFERENCE PAPER; MAGNETIC FIELD; MATHEMATICAL MODEL; SPACE; SPACE FLIGHT; SUN; VELOCITY; WIND;

EID: 0034804980     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1011859119507     Document Type: Conference Paper

References (6)

1. Motion of the footpoints of heliospheric magnetic field lines at the sun: Implications for recurrent energetic particle events at high heliographic latitudes
2. The underlying magnetic field direction in Ulysses observations of the southern polar heliosphere
3. The underlying parker spiral structure in the Ulysses magnetic field observations, 1990-1994
4. Ulysses observations of the irregularly structured mid-latitude solar wind during the approach to solar maximum
5. The role of coronal mass ejections and interplanetary shocks in interplanetary magnetic field statistics and solar magnetic flux ejection
6. Recent observations of the heliospheric magnetic field at Ulysses: Return to low latitude