Published March 1990
| Version v1
Journal article
On the numerical calculation of the solar rotational splitting coefficients
Description
An alternative method for numerically calculating the solar rotational splitting coefficient is developed. The efficacy of the method is illustrated using South Pole data. The robustness of a(2i+1) is shown to be excellent for i = 0 and to decrease with increasing i, whereas the values of b(2i+1) appear to be sensitive to the method of calculation. 11 refs
Additional details
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 351
- Series
- Astrophys. J.
- Journal Page Range
- 682-686
- ISSN
- 0004-637X
- CODEN
- ASJOA
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 21055478
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ALGORITHMS; ANGULAR VELOCITY; ASTROPHYSICS; CONVECTION; LEAST SQUARE FIT; LEGENDRE POLYNOMIALS; MAGNETIC FIELDS; OSCILLATIONS; P WAVES; ROTATION; SUN
- Descriptors DEC
- ENERGY TRANSFER; FUNCTIONS; HEAT TRANSFER; MAIN SEQUENCE STARS; MAXIMUM-LIKELIHOOD FIT; NUMERICAL SOLUTION; PARTIAL WAVES; POLYNOMIALS; STARS; VELOCITY