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Systematic Evaluation of Ionosphere/Thermosphere (IT) Models: CEDAR Electrodynamics Thermosphere Ionosphere (ETI) Challenge (2009–2010)

教师个人信息

姓名
Mark Butala 浙江大学教师主页
学院
ZJUI
研究方向
遥感,图像重建与层析成像,统计信号与图像处理理论与应用
成果类型
图书章节
Modeling the IonosphereThermosphere

出版物信息

章节名称
Systematic Evaluation of Ionosphere/Thermosphere (IT) Models: CEDAR Electrodynamics Thermosphere Ionosphere (ETI) Challenge (2009–2010)
章节作者
J. S. Shim, M. Kuznetsova, L. Rastätter, D. Bilitza, M. Butala, M. Codrescu, B. A. Emery, B. Foster, T. J. Fuller-Rowell, J. Huba, A. J. Mannucci, X. Pi, A. Ridley, L. Scherliess, R. W Schunk, J. J. Sojka, P. Stephens, D. C. Thompson, D. Weimer, L. Zhu, D. Anderson, J. L. Chau, E. Sutton
章节序号
13
章节页码
145-160
著作名称
Modeling the IonosphereThermosphere
图书作者
Joseph Huba, Robert Schunk, George Khazanov
出版社
American Geophysical Union
P-ISBN
9780875904917
E-ISBN
9781118704417
摘要

In order to model and predict the weather of the near-Earth space environment, it is necessary to understand the important coupling mechanisms from the surface of the Sun to the Earth's ionosphere, including its coupling with the atmosphere below. This chapter reports the simulations of the mid-latitude to low-latitude ionosphere. Multiday simulations during the Whole Heliosphere Interval (WHI) 2008 are performed using two versions of SAMI3 model: (1) SAMI3 with externally specified E X B drifts and (2) SAMI3 with a potential solver to self-consistently specify electric fields. The results are compared with GPS-derived global total electron content (TEC) maps. The chapter details the E X B drifts calculated by the self-consistent SAMI3 and compares these results with an empirical model. It provides initial results for a multi-year run of the descending phase of Solar Cycle 23 to illustrate the broader range of Integrated Sun-Earth System (ISES) activity underway.

DOI
10.1002/9781118704417

纸电馆藏信息

馆藏地
海宁国际分馆-特藏
索书号
P352/LM1/SC2
条码号
000000337049