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    The role of particle drifts in solar modulation (1981)
    In:  Other Sources
    Details
    Publication Date: 2019-06-28
    Description: The work of Isenberg and Jokipii (1979) is examined and it is shown that their extension of the conventional drift-flux formula to static magnetic fields of arbitrary spatial variation is invalid for interplanetary cosmic-ray transport. A field configuration involving helical magnetic fields which suppresses curvature and gradient drift and which may occur in the solar wind is presented. It is concluded that the conventional drift-flux contribution to the solar modulation of cosmic rays may, but need not, be important.
    Keywords: SOLAR PHYSICS
    Type: Astrophysical Journal; vol. 248
    Format: text
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