New advanced radio tools for monitoring and diagnostics near Earth plasma environment

To give a more detailed and complete understanding of physical plasma processes that govern the solar-terrestrial space, and to develop qualitative and quantitative models of the magnetosphere-ionosphere-thermosphere coupling, it is necessary to design and build the next generation of instruments fo...

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Published in2015 1st URSI Atlantic Radio Science Conference (URSI AT-RASC) p. 1
Main Authors Rothkaehl, Hanna, Przepiorka, Dorota, Matyjasiak, Barbara, Krankowski, Andrzej, Morawski, Marek
Format Conference Proceeding
LanguageEnglish
Published International Union of Radio Science (URSI) 01.05.2015
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Summary:To give a more detailed and complete understanding of physical plasma processes that govern the solar-terrestrial space, and to develop qualitative and quantitative models of the magnetosphere-ionosphere-thermosphere coupling, it is necessary to design and build the next generation of instruments for space diagnostics and monitoring. Novel ground based wide area sensor networks, such as the LOFAR (Low Frequency Array) radar facility, comprising wide band, and vector sensing radio receivers and multi-spacecraft plasma diagnostics should help to solve outstanding problems of Space Physics and describe long-term environmental changes. The Low Frequency Array LOFAR is a new fully digital radio telescope designed for frequencies between 30 MHz and 240 MHz located in Europe. The three new LOFAR stations will be installed until summer 2015 in Poland. The LOFAR facilities in Poland will be distributed among three sites: Lazy (East of Krakow), Borowiec near Poznan and Baldy near Olsztyn. All they will be connected via PIONIER dedicated links to Poznan. Each site will host one LOFAR station (96 high band 96 low band antennas). They will be mostly working as a part of European network, however, when less occupied, they can operate as a national network. The new digital Radio Frequency Analyzer (RFA) on board the low orbiting RELEC satellite was designed to monitor and investigate the ionospheric plasma properties. This two-point ground-based and topside ionosphere located space plasma diagnostic can be a useful new tool for monitoring and diagnosing turbulent plasma properties. The RFA on board the RELEC satellite is the first in a series of experiments which was launched in July 2014 in order to study near-Earth environment. In order to improve and validate the large and small scales ionospheric structures we will used the GPS observations collected at IGS/EPN network employed to reconstruct diurnal variations of TEC using all satellite passes over individual GPS stations and the data retrieved from FORMOSAT-3/COSMIC radio occultation measurements. The main purpose of this presentation is to describe new advanced diagnostic techniques of the near-Earth space plasma and point out the scientific challenges of the radio frequency analyzer located on-board low orbiting satellites and LOFAR facilities.
DOI:10.1109/URSI-AT-RASC.2015.7303155