Auroral ionospheric conductivities: a comparison between experiment and modeling, and theoretical f10.7-dependent model for EISCAT and ESR
Item
Title (Dublin Core)
Auroral ionospheric conductivities: a comparison between experiment and modeling, and theoretical f10.7-dependent model for EISCAT and ESR
Description (Dublin Core)
Several authors have published models of auroral conductances in the past. Some of them are based on theoretical approaches; others are the result of observations. The data bases for the latter models range from 8 h to 3 years of experiments. In this paper, we show the results of our own modeling, based on a coupled ki- netic/fluid approach. We compare these results to the sta- tistical model based on 3 years of experiment. We then model the auroral ionospheric conductances above EISCAT and the EISCAT-Svalbard Radar for different solar-activity indices. These modeled conductances are fitted with a simple law depending on the f<sub>10.7</sub> index and on the solar zenith angle.
Creator (Dublin Core)
Lilensten, J.
Blelly, P. L.
Kofman, W.
Alcaydé, D.
Date (Dublin Core)
2018-09-27
Type (Dublin Core)
Text
Format (Dublin Core)
application/pdf
Identifier (Dublin Core)
10.1007/s00585-996-1297-7
https://angeo.copernicus.org/articles/14/1297/1996/
Source (Dublin Core)
eISSN: 1432-0576
Language (Dublin Core)
eng
