Data assimilation retrieval of electron density profiles from radio occultation measurements
In this paper, the Kalman filter is used to retrieve the electron density profile along the tangent points by assimilating the slant total electron content data observed during a radio occultation (RO) event into an empirical background model. The RO data observed by COSMIC satellites on day of year...
Saved in:
Published in: | Journal of Geophysical Research: Space Physics Vol. 116; no. A3 |
---|---|
Main Authors: | , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
Washington
Blackwell Publishing Ltd
01-03-2011
|
Subjects: | |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | In this paper, the Kalman filter is used to retrieve the electron density profile along the tangent points by assimilating the slant total electron content data observed during a radio occultation (RO) event into an empirical background model. The RO data observed by COSMIC satellites on day of year 266 in 2009 are selected to do both the simulation work and the real data retrieval test. The results show that the data assimilation technique can improve the electron density retrieval in comparison with the Abel inversion. It is less influenced by the ionospheric inhomogeneity than the Abel method. Some pseudo‐large‐scale features made by the Abel retrieval, such as the plasma cave underneath the equatorial ionization anomaly region and the three peaks along the latitude direction in the E layer, disappear in the data assimilation retrieval results. Independent validation by ground‐based ionosonde observations confirms the improvement of data assimilation retrieval below the F2 peak. In addition, some potential research on RO data assimilation is also discussed.
Key Points
Kalman filter assimilation is used to retrieve the EDP from RO observations
The COSMIC observations are selected to do both simulations and real data tests
Evaluations show that data assimilation has a better performance than Abel |
---|---|
Bibliography: | istex:D7CE5E6404E40E3EEA027FAEDCEA064746C4CC00 ArticleID:2010JA015980 Tab-delimited Table 1. ark:/67375/WNG-LPJKV30N-X |
ISSN: | 0148-0227 2169-9380 2156-2202 2169-9402 |
DOI: | 10.1029/2010JA015980 |