Community-wide validation of geospace model ground magnetic field perturbation predictions to support model transition to operations

被引:127
|
作者
Pulkkinen, A. [1 ,2 ]
Rastaetter, L. [2 ]
Kuznetsova, M. [2 ]
Singer, H. [3 ]
Balch, C. [3 ]
Weimer, D. [4 ]
Toth, G. [5 ]
Ridley, A. [5 ]
Gombosi, T. [5 ]
Wiltberger, M. [6 ]
Raeder, J. [7 ,8 ]
Weigel, R. [9 ]
机构
[1] Catholic Univ Amer, Dept Phys, Washington, DC 20064 USA
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] NOAA, Space Weather Predict Ctr, Boulder, CO USA
[4] Virginia Polytech Inst & State Univ, Ctr Space Sci & Engn Res, Blacksburg, VA 24061 USA
[5] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA
[6] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[7] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
[8] Univ New Hampshire, Dept Phys, Durham, NH 03824 USA
[9] George Mason Univ, Dept Computat & Data Sci, Fairfax, VA 22030 USA
基金
美国国家科学基金会;
关键词
model transition; geomagnetically induced currents; model validation; IONOSPHERE-THERMOSPHERE MODEL; SOLAR-WIND; SPACE WEATHER; MAGNETOSPHERIC MODEL; GLOBAL SIMULATION; CHALLENGE; SUBSTORM; MAGNETOHYDRODYNAMICS; FRAMEWORK; CURRENTS;
D O I
10.1002/swe.20056
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we continue the community-wide rigorous modern space weather model validation efforts carried out within GEM, CEDAR and SHINE programs. In this particular effort, in coordination among the Community Coordinated Modeling Center (CCMC), NOAA Space Weather Prediction Center (SWPC), modelers, and science community, we focus on studying the models' capability to reproduce observed ground magnetic field fluctuations, which are closely related to geomagnetically induced current phenomenon. One of the primary motivations of the work is to support NOAA SWPC in their selection of the next numerical model that will be transitioned into operations. Six geomagnetic events and 12 geomagnetic observatories were selected for validation. While modeled and observed magnetic field time series are available for all 12 stations, the primary metrics analysis is based on six stations that were selected to represent the high-latitude and mid-latitude locations. Events-based analysis and the corresponding contingency tables were built for each event and each station. The elements in the contingency table were then used to calculate Probability of Detection (POD), Probability of False Detection (POFD) and Heidke Skill Score (HSS) for rigorous quantification of the models' performance. In this paper the summary results of the metrics analyses are reported in terms of POD, POFD and HSS. More detailed analyses can be carried out using the event by event contingency tables provided as an online appendix. An online interface built at CCMC and described in the supporting information is also available for more detailed time series analyses.
引用
收藏
页码:369 / 385
页数:17
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