Evidence for a latitudinal gradient of the cosmic ray intensity associated with a change in the tilt of the heliospheric current sheet
- 1 August 1986
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 13 (8) , 777-780
- https://doi.org/10.1029/gl013i008p00777
Abstract
No abstract availableThis publication has 13 references indexed in Scilit:
- Variations of galactic cosmic rays with heliolatitude in the outer heliosphereGeophysical Research Letters, 1986
- Differential measurement and model calculations of cosmic ray latitudinal gradient with respect to the heliospheric current sheetJournal of Geophysical Research, 1986
- Cosmic ray modulation and turbulent interaction regions near 11 AUJournal of Geophysical Research, 1985
- Deformation of the heliospheric current sheetJournal of Geophysical Research, 1985
- Variation of cosmic rays and solar wind properties with respect to the heliospheric current sheet: 1, Five‐GeV protons and solar wind speedJournal of Geophysical Research, 1985
- Latitude variation of recurrent Mev‐energy proton flux enhancements in the heliocentric radial range 11 to 20 AU and possible correlation with solar coronal hole dynamicsGeophysical Research Letters, 1985
- Estimate of cosmic-ray latitudinal gradient in 1981-1982The Astrophysical Journal, 1984
- The structure of the heliospheric current sheet: 1978–1982Journal of Geophysical Research, 1983
- Latitudinal and field‐aligned cosmic ray gradients 2 to 5 AU Voyagers 1 and 2 and IMP 8Journal of Geophysical Research, 1983
- Structure of the heliospheric current sheet in the early portion of Sunspot Cycle 21Journal of Geophysical Research, 1982