The influence of the Sun's magnetic field on energetic particles at high heliospheric latitudes

Geophysical Research Letters

Volumn 28, Issue 24, 2001, Pages 4525-4528

  Sanderson, T R ^a   Marsden, R G ^a   Tranquille, C ^a   Balogh, A ^b   Forsyth, R J ^b   Goldstein, B E ^c   Gosling, J T ^d   Harvey, K L ^e  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b IMPERIAL COLLEGE LONDON   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d LOS ALAMOS NATIONAL LABORATORY   (United States)

^e Also Solar Physics Research Corporation   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; SUN; WIND; ORBITS; SOLAR ENERGY;

LATITUDES;

GEOPHYSICS; MAGNETISM;

MAGNETIC FIELD; SOLAR CYCLE;

CORONAL HOLE; ENERGETIC PARTICLES; FIRST-PASSAGE; HELIOSPHERES; HIGH LATITUDES; NEUTRAL LINE; ORDERS OF MAGNITUDE; ULYSSES SPACECRAFT;

EID: 0035894846     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2001GL013146     Document Type: Article

References (12)

1. The evolution of the interplanetary sector structure in 1992
2. CME-driven solar wind disturbances at high heliographic latitudes
3. Latitudinal variations of solar wind corotating stream interaction regions: Ulysses
4. Stream interaction regions at high heliographic latitudes during Ulysses' second polar orbit
5. Structure of the heliospheric current sheet in the early portion of sunspot cycle 21
6. The NASA/NSO spectromagnetograph
7. Cosmic ray transport in a heliospheric magnetic field with non-polar coronal holes
8. Recurrent depressions of galactic cosmic rays in CIRs: 22-year cycle
9. Ulysses' second orbit: Remarkably different solar wind
10. Ulysses observations of the irregularly structured mid-latitude solar wind during the approach to solar maximim
11. Ulysses high-latitude observations of ions accelerated by co-rotating interaction regions
12. Disappearance of the heliospheric sector structure at Ulysses