The JB2006 empirical thermospheric density model

被引:100
作者
Bowman, Bruce R. [1 ]
Tobiska, W. Kent [2 ]
Marcos, Frank A. [3 ]
Valladares, Cesar [4 ]
机构
[1] USAF, Space Command, Space Anal A9AC, Peterson AFB, CO 80914 USA
[2] Space Environm Technol, Pacific Palisades, CA 90272 USA
[3] USAF, Res Lab, Space Vehicles Directorate, VSBXT, Bedford, MA 01731 USA
[4] Boston Coll, Space Res Inst, Chestnut Hill, MA 02467 USA
关键词
thermosphere; thermosphere models; solar EUV; neutral density; semiannual variation;
D O I
10.1016/j.jastp.2007.10.002
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
A new empirical atmospheric density model is developed using the CIRA72 (Jacchia 71) model as the basis for the diffusion equations. New solar indices based on orbit-based sensor data are used for the solar irradiances in the extreme and far ultraviolet wavelengths. New exospheric temperature and semiannual density equations are employed to represent the major thermospheric density variations. Temperature correction equations are also developed for diurnal and latitudinal effects, and finally density correction factors are used for model corrections required at high altitude (1500-4000 km). The new model, Jacchia-Bowman 2006, is validated through comparisons of accurate daily density drag data previously computed for numerous satellites. For 400 km altitude the standard deviation of 16% for the standard Jacchia model is reduced to 10% for the new JB2006 model for periods of low geomagnetic storm activity. (C) 2007 Elsevier Ltd. All rights reserved.
引用
收藏
页码:774 / 793
页数:20
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