Interpretation of observations by inversion
Interpretation of observations by inversion
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通过反演解释观测结果
DOI：
10.1002/asna.200310138
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发表时间：
2003
影响因子：
0.9
通讯作者：
J. C. D. T. Iniesta
中科院分区：
文献类型：
--
作者：
J. C. D. T. Iniesta
本文对辐射传输方程反演技术的最新进展进行了评述，并总结了其中的一些成果。目前正在使用两种值得考虑的显著不同的方法，每种方法的特征在于模型太阳大气是否通过算法迭代地改变。两者之间的比较可能有助于找到未来的反演技术，可以解决许多具有挑战性的太阳物理问题，仍然需要妥善解决。这些问题本身就表明了一些看起来比其他问题更合适的策略。
The most recent developments in inversion techniques of the radiative transfer equation are critically reviewed and some of their findings are summarized to illustrating their achievements. Two significantly different approaches are currently being used that deserve consideration, each characterized by whether or not the model solar atmospheres are changed itera- tively by the algorithm. The comparison between the two may help in finding future inversion techniques that can solve many challenging problems of solar physics that still need to be properly settled. These problems themselves suggest strategies that look more suitable than others.