Structure and merging of solar magnetic fluxtubes

Details Structure and merging of solar magnetic fluxtubes Structure and merging of solar magnetic fluxtubes

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...154..231p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 154, no. 1-2, Jan. 1986, p. 231-242.

Astronomy and Astrophysics

Astrophysics

45

Magnetic Field Configurations, Magnetohydrodynamics, Solar Magnetic Field, Faculae, Gas Pressure, Height, Radial Distribution, Twisting

Scientific paper

In the present, expansion technique-based model of the solar atmosphere's magnetic flux tubes, account is taken of the effects of field line curvature, internal structural variations, and the merging of the tube with its contiguous neighbors as it expands (through the use of a small 'seed' magnetic field between the tubes that has no influence on the solution in the limit of vanishing strength). For the solutions obtained, the internal magnetic structure of the tube evolves in height in a nonself-similar manner, although the gas pressure can vary self-similarly for the special case in which internal temperature is both uniform and equal to the external temperature. In the vicinity of the merging height, the field approaches uniformity consistent with a vertical tube with constant cross section.

Affiliated with

Also associated with

No associations

Rating

Structure and merging of solar magnetic fluxtubes 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 Structure and merging of solar magnetic fluxtubes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure and merging of solar magnetic fluxtubes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1843713