论文标题
模型S-ATMOI的太阳背景系数的C2表示
C2 representations of the solar background coefficients for the model S-AtmoI
论文作者
论文摘要
我们构建了背景数量的C2表示，这些量从标准太阳能模型S的数据点开始，这些量及其大气的表征。考虑到等温大气，该模型进一步扩展了，我们将其称为Model Atmoi。从一个离散值集中构建参数的C2表示并不是微不足道的，尤其是在模型S和大气结束之间的过渡区域中。使用太阳振荡的方程（也称为AerooSatostics中的Galbrun方程），需要这项技术工作作为在理论和数值上研究太阳波的传播的至关重要的构件。构造的模型可在http://phaidra.univie.ac.at/o:1097638上找到。
We construct C2 representations of the background quantities that characterize the interior of the Sun and its atmosphere starting from the data-points of the standard solar model S. This model is further extended considering an isothermal atmosphere, that we refer to as model AtmoI. It is not trivial to build the C2 representations of the parameters from a discrete set of values, in particular in the transition region between the end of model S and the atmosphere. This technical work is needed as a crucial building block to study theoretically and numerically the propagation of waves in the Sun, using the equations of solar oscillations (also referred to as Galbrun's equation in aeroacoustics). The constructed models are available at http://phaidra.univie.ac.at/o:1097638.
