Erratum: Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone

Details Erratum: Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone Erratum: Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...536.1005b&link_type=abstract

The Astrophysical Journal, Volume 536, Issue 2, pp. 1005-1005.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

In the paper ``Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone'' by A. S. Brun, S. Turck-Chièze, and J. P. Zahn (525, 1032 [1999]), several corrections are required: 1. The words ``greater than'' just after equation (11) for the definition of rbcz should be removed. 2. The beginning of first sentence of the next paragraph should read: ``With the latitudinal dependence of the angular velocity at the base of the convection zone borrowed from Thompson et al. (1996), Ωbcz/2π=456-72x2-42x4 nHz,'' instead of ``Ωbcz>/2π=456-72x2- 42x4.'' 3. In the footnote to Table 1, ``Rbzc'' should be ``Rbcz,'' as it is appears for ``Tbcz'' in the same footnote. 4. In Table 2, in the ``Parameters'' column, ``i0'' should be ``Z0,'' as in Table 1. 5. In Table 3, ``Observaton'' should be ``Observation.'' The Press sincerely regrets these errors.

Affiliated with

Also associated with

No associations

Rating

Erratum: Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the 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 Erratum: Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Erratum: Standard Solar Models in the Light of New Helioseismic Constraints. II. Mixing below the Convective Zone will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1391712