A search for outflows from X-ray bright points in coronal holes

Details A search for outflows from X-ray bright points in coronal holes A search for outflows from X-ray bright points in coronal holes

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986udnw.reptr....m&link_type=abstract

Final Report Delaware Univ., Newark.

Physics

Coronal Holes, Magnetic Disturbances, Solar Flares, Solar Flux, Solar X-Rays, Doppler Effect, Solar Maximum Mission, Velocity Distribution

Scientific paper

Properties of X-ray bright points using two of the instruments on Solar
Maximum Mission were investigated. The mass outflows from magnetic
regions were modeled using a two dimensional MHD code. It was concluded
that mass can be detected from X-ray bright points provided that the
magnetic topology is favorable.

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