International Association of Geodesy

 

COMMISSION 4: Positioning & Applications

Study Group 1.1: Ionospheric Modelling and Analysis (joint with IAG Commission 1 & IGS & COSPAR)


   
 

Study Group 1.1 web site ... click here ...

Terms of Reference

As a result of many years of research the climatology of the ionosphere is today quite well known. However, variations of the solar activity and emissions of plasma from the solar corona change the conditions of the Sun-Earth environment and can dramatically disturb the ionospheric mean conditions. The development of sophisticated high technological systems for navigation, telecommunication, space missions, etc., created the need of predicting the meteorological conditions of the space around the Earth, giving rise to a branch of knowledge that today is called space weather. Disruptions of the ionosphere caused by massive solar flares can interfere with or even destroy communication systems, Earth satellites and power grids on Earth. A stringent application of ionospheric models would be to provide real-time corrections and integrity information for aircraft navigation and precision approach.

Ionospheric models are important for many space geodesy observing techniques to correct the delay caused by the ionosphere on the propagation of electromagnetic wave, typical applications being single-frequency GPS and GLONASS positioning or real time ambiguity resolution. The EarthÕs ionosphere has been studied for more than one hundred years using different observational techniques. A large contribution to the knowledge of the bottom-side ionosphere was done by a global network of 100-200 vertical incidence ionosondes, that started operation during the International Geophysical Year 1957-1958. Incoherent backscatter radars were used after 1958 to extend the exploration of the ionosphere to its topside. In 1957 the space age began enabling topside ionosondes onboard satellites, observations of Faraday rotation on transionospheric signals emitted by geostationary satellites, Doppler method with rockets and satellites and in situ techniques aboard spacecrafts.

Using large data bases of classical observations covering different geographical regions and different solar and geomagnetic conditions, several empirical ionospheric models were established. Among them, the International Reference Ionosphere (IRI) is probably the most widely used. IRI is continuously revised and updated through international cooperative effort of different type sponsored by the Working Group created by the Committee on Space Research (COSPAR) and the Union of Radio Sciences (URSI). Today ground-based and space-based GPS observations, and in a less extent observations of other space geodetic dual-frequency observing techniques, e.g., satellite altimetry, bring an unprecedented opportunity for ionospheric studies and may well revolutionize science and technology of the ionospheric meteorology. They provide high quality ionospheric information, with global coverage, simultaneity and time continuity and are easy and free available for ionospheric scientists.


Steering Committee

Michael Schmidt (Germany) - Chair
Susan Skone (University of Calgary, Canada) - Vice-Chair


Objectives

A first valuable step toward exploiting the GPS potentiality for ionospheric studies was already done by the IGS in 1998 by the creation of the Ionosphere Working Group. In the framework of this group, five centers are computing and making accessible on a regular basis several GPS-derived ionospheric products, mainly two-dimensional worldwide grids of vertical total electron content. We believe that the efforts to maintain a regular service for processing GPS data to form VTEC maps should be continued, but we are convinced that the effort should be pursued to fully exploit such amount of high quality data and to maximize the benefits for the scientific community. Therefore, we propose the creation of a study group on Ionospheric Modeling and Analyses, in co-operation with IGS and possibly with COSPAR, to support the already existing Ionospheric Working Groups.

The principal objectives of the Study Group may be summarized as follows: