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The Ionosphere Prediction Service

Published online by Cambridge University Press:  24 July 2018

Carlo Albanese
Affiliation:
Telespazio, Rome, Italy
Filippo Rodriguez
Affiliation:
Telespazio, Rome, Italy
Roberto Ronchini
Affiliation:
Telespazio, Rome, Italy
Stefano Di Rollo
Affiliation:
Telespazio, Rome, Italy
Francesco Berrilli
Affiliation:
University of Rome “Tor Vergata”, Rome, Italy
Alice Cristaldi
Affiliation:
University of Rome “Tor Vergata”, Rome, Italy
Dario Del Moro
Affiliation:
University of Rome “Tor Vergata”, Rome, Italy
Roberta Forte
Affiliation:
University of Rome “Tor Vergata”, Rome, Italy
Giorgiana De Franceschi
Affiliation:
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Claudio Cesaroni
Affiliation:
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Luca Spogli
Affiliation:
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Vincenzo Romano
Affiliation:
Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
Marcio Aquino
Affiliation:
University of Nottingham, Nottingham, UK
Sreeja Vadakke Veettil
Affiliation:
University of Nottingham, Nottingham, UK
Osman Kalden
Affiliation:
Telespazio Vega DE, Darmstadt, Germany
Michael Hutchinson
Affiliation:
Nottingham Scientific Ltd, Nottingham, UK
Eric Guyader
Affiliation:
European Commission, Bruxelles, Belgium
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Abstract

The aim of the Ionosphere Prediction Service (IPS) project is to design and develop a prototype platform to translate the prediction and forecast of the ionosphere effects into a service customized for specific GNSS user communities. The project team is composed by Telespazio (coordinator), Nottingham Scientific Ltd, Telespazio Vega Deutschland, the University of Nottingham, the University of Rome “Tor Vergata” and the Italian Istituto Nazionale di Geofisica e Vulcanologia (INGV). The IPS development is conceived of two concurrent activities: prototype service design and development & research activity that will run along the whole project. Service design and development is conceived into four phases: user requirements collection, architecture specification, implementation and validation of the prototype. A sub-activity analyses also the integration feasibility in the Galileo Service center, located in Madrid. The research activity is the scientific backbone of IPS that will provide the models and algorithms for the forecasting products.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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