An estimate of drift effects in various models of the heliospheric magnetic field

Space Science Reviews

Volumn 97, Issue 1-4, 2001, Pages 331-335

  Burger, R A ^a,b   Van Niekerk, Y ^b   Potgieter, M S ^b  

^a UNIVERSITY OF DELAWARE   (United States)

^b NORTH WEST UNIVERSITY   (South Africa)

Author keywords

[No Author keywords available]

Indexed keywords

CALCULATION; CONFERENCE PAPER; COSMIC RADIATION; FREQUENCY MODULATION; MAGNETIC FIELD; MODEL; POLARIZATION; SOLAR ENERGY;

EID: 0034816555     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/A:1011845504912     Document Type: Conference Paper

References (9)

1. Antiprotons at solar maximum
2. Steady-state drift-dominated modulation models for galactic cosmic rays
3. Motion of the footpoints of heliospheric magnetic field lines at the Sun: Implications for recurrent energetic particle events at high heliographic latitudes
4. The modulation of cosmic rays in the high latitude heliosphere: A computer simulation
5. The polar heliospheric magnetic field
6. The passage of energetic charged particles through interplanetary space
7. Solar cycle variation of the interplanetary magnetic field spiral
8. The effect of the heliospheric current sheet on cosmic ray intensities at solar maximum: Two alternative hypotheses