Exospheric Hydrogen Model

A Monte Carlo simulation of the terrestrial hydrogen exosphere is used to derive a global model of the exospheric hydrogen density. A third-order spherical harmonic expansion in longitude and colatitude is used to represent H at a particular radius. The h_exos.dat file provides the harmonic expansion coefficients for 40 radii (between 6640 km and 62126 km) for solstice and equinox conditions, and for four levels of solar activity (F10.7 = 80, 130, 180, 230). Details of the Monte Carlo simulation are explained in Hodges (1994). The simulation results show significant differences with previous exosphere models, as well as with the H distributions of the MSIS-86 thermosphere model.

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Initial contribute: 2019-07-02

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Center for Space Sciences University of Texas at Dallas
:  
hodges@utdallas.edu
:  
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Application-focused categoriesNatural-perspectiveSpace-earth regions

Detailed Description

English {{currentDetailLanguage}} English
 
Parameter: Exospheric hydrogen density
Availability: Related software can be retrieved directly from CCMC's anonymous FTP site.
 
Brief Description:

A Monte Carlo simulation of the terrestrial hydrogen exosphere is used to derive a global model of the exospheric hydrogen density. A third-order spherical harmonic expansion in longitude and colatitude is used to represent H at a particular radius. The h_exos.dat file provides the harmonic expansion coefficients for 40 radii (between 6640 km and 62126 km) for solstice and equinox conditions, and for four levels of solar activity (F10.7 = 80, 130, 180, 230). Details of the Monte Carlo simulation are explained in Hodges (1994). The simulation results show significant differences with previous exosphere models, as well as with the H distributions of the MSIS-86 thermosphere model.

References:
Hodges, R.R., Monte Carlo simulation of the terrestrial hydrogen exosphere, J. Geophys. Res., 99, 23229-23247, 1994.

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R. Richard Hodges Jr. (2019). Exospheric Hydrogen Model , Model Item, OpenGMS, https://geomodeling.njnu.edu.cn/modelItem/0fc52edb-6b83-4e3f-8d60-58650a781034
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Contributor(s)

Initial contribute : 2019-07-02

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Authorship

:  
Center for Space Sciences University of Texas at Dallas
:  
hodges@utdallas.edu
:  
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Is authorship not correct? Feed back

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