The Role of Scale and Model Bias in ADAPT's Photospheric Eatimation

GSTDTAP > 地球科学

DOI	10.2172/1182619
报告编号	LA-UR--15-23781
来源ID	OSTI ID: 1182619
	The Role of Scale and Model Bias in ADAPT's Photospheric Eatimation
	Godinez Vazquez, Humberto C.; Hickmann, Kyle Scott; Arge, Charles Nicholas; Henney, Carl
	2015-05-20
出版年	2015
页数	19
语种	英语
国家	美国
领域	地球科学
英文摘要	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.
英文关键词	Heliospheric and Magnetospheric Physics Mathematics Solar Photosphere, Data Assimilation
URL	查看原文
来源平台	US Department of Energy (DOE)
引用统计
文献类型	科技报告
条目标识符	http://119.78.100.173/C666/handle/2XK7JSWQ/7067
专题	地球科学
推荐引用方式 GB/T 7714	Godinez Vazquez, Humberto C.,Hickmann, Kyle Scott,Arge, Charles Nicholas,et al. The Role of Scale and Model Bias in ADAPT's Photospheric Eatimation,2015.