热改正
- 网络bolometric correction
热改正-
由近红外观测结果估算了其在K波段的热改正BCK和视热星等m（bol）以及有效温度Te。
Prom the results of the near infrared photometry , the bolometric corrections in the K band , the apparent bolometric magnitudes and the effective temperatures can be estimated .
-
由湍流激发的湍流磁场，作为一个非理想效应对太阳热结构的改正是从MHD方程组推导出来，它的形式是ReynoldsStress张量和磁扰动张量的贡献。
The turbulent magnetic fields which is generated by the turbulence is derived from the magnetohydrodynamics equations . It 's form is the contribution of the Reynolds stress tensor and magnetic fluctuating tensor .