CPW-TEC:
Climatology of planetary waves seen in ionospheric F-region perturbations using TEC of GPS

(DFG JA 836/19-1, 2005-2007, JA 836/24-1, 2008-2009)

zur Startseite des LIM
Staff: P. Hoffmann                          PI: Prof. Christoph Jacobi


Long-period planetary waves (PW) cannot propagate directly into the upper thermo­sphere. Nevertheless, they already have been identified there from ionosonde measure­ments and partly they can directly be correlated to neutral atmosphere PW.

Ionosondes, as most ground-based system, however, cannot provide a full global picture of PW due to the limited regional coverage following from their geographical distribu­tion. One possible mean to overcome this disadvantage is using ionospheric information from ground-based GPS receivers, available on a routine basis through the International GPS Service. How­ever, from ground-based GPS measurements only the vertically integrated electron den­sity (TEC) can be derived. Therefore, the interpretation of waves seen in TEC requires a particular careful analysis of the observations. Additional measurements allowing the estimation of the profile shape including the height of the electron density maximum shall be used to evaluate or to complete the TEC findings.

The propagation of PW into the thermosphere is analyed using the circulation model COMMA and correlation of ionospheric waves with neutral atmospheric PW mainly anaylsed using ground-based radars such as the Collm SKiYMET meteor radar

Publications related to the project

An overview over the project (poster at EGU 2008 General Assembly)

Planetary wave
spectra

Upper panel: Differential TEC (black) and TID proxy modulation at PW time scales. Lower panel: Seasonal cycle of GW (potential energy from SABER temperature profiles) modulation at PW time scales.

The project is part of the DFG priority program "CAWSES". The project bases on a collaboration with

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Last modification 7.6.2010