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HORIZON 202, PHITIA-NRF 101007599, Plasmasphere Ionosphere Thermosphere Integrated Research Environment and Access services: a Network of Research Facilities, 2021-2024, investigator (IAP): Obrazová (Burešová) Dalia |
ESA AO/1-9544/20/I/NS, Lidar measurements to Identify Streamers and analyse Atmospheric waves, 2021-2022, investigator (IAP): Kozubek Michal |
HORIZON 2020, EUROPLANET 2024, projekt EPN2024-RI, ID 871149, EUROPLANET 2024, 2020-2024, investigator (IAP): Souček Jan description Investing in space infrastructures such as in the Copernicus and Galileo programmes, Europe has historically been at the forefront of space exploration. The Commission has made ambitious proposals for the period 2021–2027. These include a dedicated Space programme for a total of EUR 16 billion. It is within this context the EU-funded EPN-2024-RI will provide infrastructure necessary to address the major scientific and technological challenges facing modern planetary science. Its aim is to ensure Europe’s position is at the forefront of space exploration. To do this, the project will provide Transnational Access (TA) to an enhanced set of world-leading field and laboratory facilities, Virtual Access (VA) to state-of-the-art data services and tools linked to the European Open Science Cloud (EOSC), and Networking Activities (NA) to widen the user base and draw in new partners from around the world.close |
COST CA19139, Process-based models for climate impact attribution across sectors (PROCLIAS), 2020-2024, investigator (IAP): Urban Aleš description Many complex process-based models are available in Europe to project future climate impacts. Yet, the current climate impact research community is fragmented, modeling mostly individual systems. The integration of climate impacts across different natural and societal sectors is only slowly emerging. Likewise, attribution of impacts to climate and other factors is still a strongly under-researched field given that climate change is already strongly manifesting itself, an increasing number of court cases dealing with climate impacts is being negotiated and policy debates on loss and damage are intensifying. This lack of coordination amongst impact modelers and insufficient awareness about impact attribution methods hampers important scientific and political progress and more coordination and networking is urgently needed. Therefore, PROCLIAS aims to develop common protocols, harmonized datasets and a joint understanding of how to conduct cross-sectoral, multi-model climate impact studies at regional and global scales allowing for attribution of impacts of recent climatic changes and robust projections of future climate impacts. The Action will do so by focusing on key interactions of climate impacts across sectors, their accumulated effect, especially of extreme events, the attribution of impacts to climate change and the quantification of uncertainties. PROCLIAS will make use of all COST networking tools to train young researchers to conduct and analyse multi-model simulations in a cross-sectoral way, to support a common platform for collecting impact model simulations and methods for analyzing them and to disseminate the data, code and results to scientists as well as, in a more synthesized form, to stakeholders. close |
HORIZON 2020 ID 870437, SafeSpace - Radiation Belt Environmental Indicators for the Safety of Space Assets, 2020-2022, investigator (IAP): Santolík Ondřej description Monitoring space weather events is crucial. The EU-funded SafeSpace project aims to advance space weather nowcasting and forecasting capabilities, contributing significantly to the safety of space assets through the transition of powerful tools from research to operations. This will be achieved through the synergy of five well-established space weather models. SafeSpace hopes to improve radiation belt, culminating in a prototype early warning system for detrimental space weather events, integrating information all the way from the Sun to the inner magnetosphere. Working, also, with a major European space company, SafeSpace, hopes to define indicators of particle radiation of use to space industry and spacecraft operators. close |
HORIZON 2020, ID 870452, PAGER - Prediction of Adverse effects of Geomagnetic Storms and Energetic Radiation, 2020-2022, investigator (IAP): Souček Jan description A geomagnetic storm is a major disturbance of Earth\'s magnetosphere. It occurs when there is a very efficient exchange of energy from the solar wind into the space environment surrounding Earth. Predicting these storms is vital. This is the objective of the EU-funded PAGER project, which has assembled a team of leading academic and industry experts in space weather research, space physics, empirical data modelling and space environment effects on spacecraft from Europe and the United States. The project will provide a 1-2 day probabilistic forecast of ring current and radiation belt environments. This will allow satellite operators to respond to predictions that present a threat. The most advanced codes will be used, adapted to perform ensemble simulations and uncertainty quantifications.
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ESA 4000129250/19/NL/AS, Q/V Band Large Scale Spatio-Temporal Channel Models for Satcom Design and Operations, 2020-2021, investigator (IAP): Fišer Ondřej, team: Pitaš, K.; |
ESA ESA 4000126709/18/NL/IA, VERA: VERtical coupling in Earth´s atmosphere at mid and high latitudes, 2019-2020, investigator (IAP): Laštovička Jan description
The Earth\'s atmosphere consists of several layers that differ in physical properties. The goal of the vertical coupling in Earth’s atmosphere at mid and high latitudes (VERA) project is to understand the coupling mechanisms by which the upper atmosphere (ca. 85-600 km) is influenced by the processes in the regions below. Our focus is on sudden stratospheric warming (SSW) events, during which the middle atmosphere (10-85 km) is highly disturbed. The ionosphere response to SSWs has previously been studied for low latitude regions, where forcing from the magnetosphere is indirect and relatively modest. VERA will assess the importance of vertical atmospheric coupling at mid- and high- latitudes, using observations from low Earth orbit (LEO) satellites and ground-based radars, as well as state-of-the-art numerical models. The conclusions derived from the analyses of these data can lead to a significant breakthrough on driving forces of the ionospheric weather.
ESA\'s satellite constellation mission, Swarm, will play a key role in the VERA project. Swarm\'s high precision magnetometers and its dedicated constellation for geospace research enable monitoring of the mid- and low-latitude inter-hemispheric field-aligned currents, which will be fully explored in VERA. In addition to the Swarm data, 10 years of CHAMP magnetometer data will be used to allow the opportunity to investigate more SSW events. These satellite observations will be enhanced by the analysis of ground-based ionospheric observations. Moreover, observational results will be supported by a recently-developed empirical model of the high-latitude ionosphere, E-CHAIM, and a physics-based model, TIEGCM.
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ESA 4000126708/19/NL/IA, ILGEW - Investigating Lightning Generated ELF Whistlers to Improve Ionospheric Models, 2019-2020, investigator (IAP): Truhlík Vladimír, team: Obrazová, D.; Chum, J. |
HORIZON 2020 ID 776011, TechTIDE - Warning and Mitigation Technologies for Travelling Ionospheric Disturbances Effects, 2017-2020, investigator (IAP): Obrazová (Burešová) Dalia description Travelling Ionospheric Disturbances (TIDs) constitute a threat for operational systems for which the ionosphere is an essential part (i.e., radio systems) or for which the ionosphere is fundamentally a nuisance (i.e. GNSS based systems and applications). The overarching objective of TechTIDE is to design and test new viable TID impact mitigation strategies for the technologies affected by the TIDs and in close collaboration with operators of these technologies, to demonstrate the added value of the proposed mitigation techniques which are based on TechTIDE products. To achieve this main goal, it is necessary to address the following specific objectives:
i. Improve understanding regarding the physical processes resulting in the formation of TIDs, and consequently to identify the drivers in the interplanetary medium, the magnetosphere and the atmosphere;
ii. Define the impact of the TIDs on the space based navigation systems (mainly EGNOS services and N-RTK) and on ground-based HF communication and geolocation systems;
iii. Develop improved methodologies, based on consortium partners’ algorithms, suitable to support for the first time the direct,real-time identification and tracking of TIDs over wide world regions;
iv. Establish an operational system to issue warnings of the occurrence of TIDs over the region extending from Europe to South Africa, to estimate the parameters that specify the TID characteristics and the inferred perturbation, and provide all additional geophysical information to the users to help them assess the risks and to develop mitigation techniques, tailored to their applications;
v. Work systematically with potential users to assess the functionality, reliability and efficiency of the TechTIDE services paving the way to its systematic exploitation from users and to its sustainable operation. close |
NATO SPS ID SfP 984894, Testing for the first time a novel experimental technique for the identification and tracking TIDs over Europe, 2016-2018, investigator (IAP): Obrazová (Burešová) Dalia |
HORIZON 2020, projekt EPN2020-RI ID 654208, EUROPLANET 2020 Research Infrastructure: “Europlanet 2020 RI has received funding from the European Union, 2015-2019, investigator (IAP): Santolík Ondřej description The Europlanet 2020 Research Infrastructure (EPN2020-RI) will address key scientific and technological challenges facing modern planetary science by providing open access to state-of-the-art research data, models and facilities across the European Research Area. Its Transnational Access activities will provide access to world-leading laboratory facilities that simulate conditions found on planetary bodies as well as specific analogue field sites for Mars, Europa and Titan. Its Virtual Access activities will make available the diverse datasets and visualisation tools needed for comparing and understanding planetary environments in the Solar System and beyond. By providing the underpinning facilities that European planetary scientists need to conduct their research, EPN2020-RI will create cooperation and effective synergies between its different components: space exploration, ground-based observations, laboratory and field experiments, numerical modelling, and technology.
EPN2020-RI builds on the foundations of successful FP6 and FP7 Europlanet programmes that established the ‘Europlanet brand’ and built structures that will be used in the Networking Activities of EPN2020-RI to coordinate the European planetary science community’s research. It will disseminate its results to a wide range of stakeholders including industry, policy makers and, crucially, both the wider public and the next generation of researchers and opinion formers, now in education. As an Advanced Infrastructure we place particular emphasis on widening the participation of previously under-represented research communities and stakeholders. We will include new countries and Inclusiveness Member States, via workshops, team meetings, and personnel exchanges, to broaden/widen/expand and improve the scientific and innovation impact of the infrastructure. EPN2020-RI will therefore build a truly pan-European community that shares common goals, facilities, personnel, data and IP across national boundaries close |
HORIZON 2020, projekt ARISE2, ID 653980, ARISE2 - Atmospheric dynamics Research InfraStructure in Europe 2, 2015-2018, investigator (IAP): Laštovička Jan, team: Šindelářová T. - member of Management Committee, Chum J., Baše J., Fišer J., Hruška F., Obrazová (Burešová) D. description It has been robustly demonstrated that variations in the circulation of the middle atmosphere influence weather and climate throughout the troposphere all the way to the Earth’s surface. A key part of the coupling between the troposphere and stratosphere occurs through the propagation and breaking of planetary-scale Rossby waves and gravity waves. Limited observation of the middle atmosphere and these waves in particular limits the ability to faithfully reproduce the dynamics of the middle atmosphere in numerical weather prediction and climate models.
ARISE2 capitalizes upon the work of the EU-funded first ARISE project combining for the first time international networks with complementary technologies such as infrasound, lidar and
airglow. This joint network provided advanced data products that started to be used as benchmarks for weather forecast models. The ARISE network also allows enhanced and detailed monitoring of other extreme events in the Earth system such as erupting volcanoes, magnetic storms, tornadoes and tropical thunderstorms. In order to improve the ability of the network to monitor atmospheric dynamics, ARISE2 proposes to extend i) the existing network coverage in Africa and the high latitudes, ii) the altitude range in the stratosphere and mesosphere, iii) the observation duration using routine observation modes, and to use complementary existing infrastructures and innovative instrumentations. Data will be collected over the long term to improve weather forecasting to monthly or seasonal timescales, to monitor atmospheric extreme events and climate change. Compared to the first ARISE project, ARISE2 focuses on the link between models and observations for future assimilation of data by operational weather forecasting models. Among the applications, ARISE2 proposes infrasound remote volcano monitoring to provide notifications to civil aviation. The data portal will provide high-quality data and advanced data products to a wide scientific community. close |
EU, 7th FP , , 2012-2014, investigator (IAP): Laštovička Jan, team: Laštovička, J. |
NATO RTO. SCI-229-RTG , , 2011-2014, investigator (IAP): Obrazová (Burešová) Dalia |