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Model Photospheres for Late-Type Stars from the Inversion of High-Resolution Spectroscopic Observations. Groombridge 1830 and Epsilon Eridani

机译：从反演中反演晚期恒星的模型光球高分辨率光谱观测。 Groombridge 1830和Epsilon 波江座

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Prieto Carlos Allende; Lopez Ramon J. Garcia; Lambert David L.; Cobo Basilio Ruiz;
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年度 1999
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正文语种 {"code":"en","name":"english","id":9}
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1. Model Photospheres for Late-Type Stars from the Inversion of High-Resolution Spectroscopic Observations: Groombridge 1830 and ? Eridani [J] . Carlos Allende Prieto1, Ramón J. García López2, David L. Lambert1, The Astrophysical journal . 2008,第2期

机译：高分辨率光谱观测反演的晚型恒星模型光球：Groombridge 1830和？江谷
2. Model Photospheres for Late-Type Stars from the Inversion of High-Resolution Spectroscopic Observations: The Sun [J] . Carlos Allende Prieto1, Basilio Ruiz Cobo1, J. García López1 The Astrophysical journal . 2009,第2期

机译：高分辨率光谱观测反演的晚型恒星模型光球：太阳
3. Model photospheres for late-type stars from the inversion of high-resolution spectroscopic observations: the SUN [J] . Carlos Allende Prieto, Basilio Ruiz Cobo, Ramon J.Garcia The Astrophysical journal . 1998,第2期

机译：高分辨率光谱观测反演的晚型恒星模型光球：太阳
4. 3D and NLTE Effects on Spectroscopic Parameters of Late-Type Stars [C] . Karin Lind, Maria Bergemann, Remo Collet, Subaru International Conference . 2012

机译：3D和NLTE对晚型星光镜参数的影响
5. Toward resolving stable high-resolution kinematic rupture models of large earthquakes by joint inversion of seismic, geodetic and tsunami observations. [D] . Yue, Han. 2014

机译：通过地震，大地测量和海啸观测的联合反演，建立稳定的高分辨率大地震运动破裂模型。
6. Monte Carlo Bayesian inference on a statistical model of sub-gridcolumn moisture variability using high-resolution cloud observations. Part 1: Method [O] . Peter M. Norris, Arlindo M. da Silva -1

机译：蒙特卡洛·贝叶斯（Monte Carlo Bayesian）使用高分辨率云观测结果推断亚网格柱水分变化的统计模型。第1部分：方法
7. Model Photospheres for Late-Type Stars from the Inversion of High-Resolution Spectroscopic Observations. The Sun [O] . Prieto, Carlos Allende, Cobo, Basilio Ruiz, Lopez, Ramon J. Garcia 1998

机译：从反演中反演晚期恒星的模型光球高分辨率光谱观测。太阳

Model Photospheres for Late-Type Stars from the Inversion of High-Resolution Spectroscopic Observations. Groombridge 1830 and Epsilon Eridani

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