Element Separation in the Chromosphere Ionization-Diffusion Models for the FIP-Effect

Details Element Separation in the Chromosphere Ionization-Diffusion Models for the FIP-Effect Element Separation in the Chromosphere Ionization-Diffusion Models for the FIP-Effect

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ssrv...85..253p&link_type=abstract

Space Science Reviews, v. 85, Issue 1/2, p. 253-260 (1998).

Computer Science

1

Sun: Abundances, Chromosphere, Solar Wind

Scientific paper

Ionization-diffusion mechanisms to understand the first ionization potential (FIP) fractionation as observed in the solar corona and the solar wind are reviewed. The enrichment of the low-FIP elements (<10 eV) compared to the high-FIP elements, seen in e.g. slow and fast wind or polar plumes, is explained. The behaviour of the heavy noble gases becomes understandable. The absolute fractionation, i.e. in relation to hydrogen, can be calculated and fits well to the measurements. The theoretical velocity-dependence of the fractionation will with used to determine the velocities of the solar wind in the chromosphere.

Affiliated with

Also associated with

No associations

Rating

Element Separation in the Chromosphere Ionization-Diffusion Models for the FIP-Effect does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Element Separation in the Chromosphere Ionization-Diffusion Models for the FIP-Effect, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Element Separation in the Chromosphere Ionization-Diffusion Models for the FIP-Effect will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1047462