科技报告详细信息
| The Role of Scale and Model Bias in ADAPT's Photospheric Eatimation | |
| Godinez Vazquez, Humberto C.1  Hickmann, Kyle Scott1  Arge, Charles Nicholas1  Henney, Carl1  | |
| [1] Los Alamos National Lab. (LANL), Los Alamos, NM (United States) | |
| 关键词: Heliospheric and Magnetospheric Physics; Mathematics; Solar Photosphere; Data Assimilation; | |
| DOI : 10.2172/1182619 RP-ID : LA-UR--15-23781 PID : OSTI ID: 1182619 |
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| 美国|英语 | |
| 来源: SciTech Connect | |
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【 摘 要 】
The Air Force Assimilative Photospheric flux Transport model (ADAPT), is a magnetic flux propagation based on Worden-Harvey (WH) model. ADAPT would be used to provide a global photospheric map of the Earth. A data assimilation method based on the Ensemble Kalman Filter (EnKF), a method of Monte Carlo approximation tied with Kalman filtering, is used in calculating the ADAPT models.
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