The JB2006 empirical thermospheric density model

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 se...

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Veröffentlicht in:Journal of atmospheric and solar-terrestrial physics 2008-03, Vol.70 (5), p.774-793
Hauptverfasser: Bowman, Bruce R., Kent Tobiska, W., Marcos, Frank A., Valladares, Cesar
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container_issue 5
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container_title Journal of atmospheric and solar-terrestrial physics
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creator Bowman, Bruce R.
Kent Tobiska, W.
Marcos, Frank A.
Valladares, Cesar
description 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.
doi_str_mv 10.1016/j.jastp.2007.10.002
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subjects Earth, ocean, space
Exact sciences and technology
External geophysics
Neutral density
Physics of the ionosphere
Physics of the magnetosphere
Semiannual variation
Solar EUV
Thermosphere
Thermosphere models
title The JB2006 empirical thermospheric density model
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