Flux tube expansion factors and solar wind velocity - Results from a self-consistent MHD model

Details Flux tube expansion factors and solar wind velocity - Results from a self-consistent MHD model Flux tube expansion factors and solar wind velocity - Results from a self-consistent MHD model

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20...35b&link_type=abstract

Advances in Space Research, vol. 20, p. 35

Astronomy and Astrophysics

Astronomy

1

Solar Flux, Solar Wind Velocity, Self Consistent Fields, Astronomical Models, Coronal Holes, Solar Diameter

Scientific paper

Results from a self-consistent MHD model of the solar wind from a polar coronal hole are here used to examine the relationship between solar wind velocity and the superradial expansion factor of the wind's flux tubes in greater detail. The latitudinal as well as radial variations of the expansion factors are taken into account. Attention is given to the reasons for the dichotomy between findings of researchers who have found a direct relationship and those who have found an inverse relationship between expansion factor and wind velocity.

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