IMAGE/RPI Model

This model was developed based on data from the Radio Plasma Imager (RPI) on the IMAGE spacecraft. Since the launch of IMAGE in March 2000, RPI has continuously recorded plasmasphere soundings. The electron density profile inverted from a single such plasmagram gives the density distribution along a considerable portion of the magnetic field line. Based on many of such field-line profiles Huang et al. (2004) have constructed a model that varies with L-value and latitude.

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Contributor(s)

Initial contribute: 2019-07-02

Authorship

:  
Center for Atmospheric Research, University of Massachusetts Lowell
:  
bodo_reinisch@uml.edu
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Classification(s)

Application-focused categoriesNatural-perspectiveSpace-earth regions

Detailed Description

English {{currentDetailLanguage}} English

Quoted from: https://ccmc.gsfc.nasa.gov/modelweb/plasmas/image.html

Parameter: Electron density in the plasmasphere

Brief Description:
This model was developed based on data from the Radio Plasma Imager (RPI) on the IMAGE spacecraft. Since the launch of IMAGE in March 2000, RPI has continuously recorded plasmasphere soundings. The electron density profile inverted from a single such plasmagram gives the density distribution along a considerable portion of the magnetic field line. Based on many of such field-line profiles Huang et al. (2004) have constructed a model that varies with L-value and latitude.

Availability: Please contact model authors.

References:
Xueqin Huang, Bodo W. Reinisch, Paul Song, James L. Green, Dennis L. Gallagher, Developing an empirical density model of the plasmasphere using IMAGE/RPI observations, Advances in Space Research 33, 829 - 832, 2004

模型元数据

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X. Huang, B. Reinisch (2019). IMAGE/RPI Model, Model Item, OpenGMS, https://geomodeling.njnu.edu.cn/modelItem/a8661fbd-d085-4d08-8a36-4b8a37179afe
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Contributor(s)

Initial contribute : 2019-07-02

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Authorship

:  
Center for Atmospheric Research, University of Massachusetts Lowell
:  
bodo_reinisch@uml.edu
Is authorship not correct? Feed back

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