Gas entry into non-spot magnetic tubes

Details Gas entry into non-spot magnetic tubes Gas entry into non-spot magnetic tubes

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977soph...52..315g&link_type=abstract

Solar Physics, vol. 52, May 1977, p. 315-325.

Physics

13

Gaseous Diffusion, Magnetic Field Configurations, Magnetohydrodynamics, Solar Magnetic Field, Solar Physics, Chromosphere, Gas Pressure, Magnetic Flux, Photosphere, Plasma Diffusion, Turbulence Effects

Scientific paper

Gas penetration into twisted magnetic tubes can occur by the inward diffusion of neutral atoms in the neighbourhood of the temperature minimum between the photosphere and chromosphere, where the degree of ionization is low. Again, turbulent buffeting indents tubes in the convection zone and, in particular near the photosphere, provides a larger area where the overall diffusion rate may be enhanced. These processes do not contribute rapidly to the gas content of magnetic tubes, but diffusion near the temperature minimum may well be the source of the observed downflow in magnetic points.

Affiliated with

Also associated with

No associations

Rating

Gas entry into non-spot magnetic tubes 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 Gas entry into non-spot magnetic tubes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gas entry into non-spot magnetic tubes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1883635