Models of the solar convective zone

Details Models of the solar convective zone Models of the solar convective zone

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...66g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, Jan.-Feb. 1985, p. 66-74. In Russian.

Astronomy and Astrophysics

Astronomy

Convective Flow, Mixing Length Flow Theory, Solar Temperature, Stellar Models, Stellar Structure, Astronomical Catalogs, Boundary Value Problems, Depth, Flow Velocity, Two Dimensional Models, Velocity Distribution

Scientific paper

Models of the solar convective zone were obtained on the basis of mixing length theory. On the internal boundary these models agree with the Abraham-Iben (1971) model of the solar internal structure, while on the external boundary they agree with the HSRA, HOLMU, and VAL 80 semiempirical models and with Nelson's (1978) theoretical two-dimensional model. Calculated velocities of rising convective elements are compared with observed ones.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1593093