Planetary Science Virtual Observatory: VESPA/Europlanet outcome and prospects

2020 ◽  
Author(s):  
Stéphane Erard ◽  
Baptiste Cecconi ◽  
Pierre Le Sidaner ◽  
Angelo Pio Rossi ◽  
Hanna Rothkaehl ◽  
...  
Keyword(s):  
Open Science ◽  
Planetary Science ◽  
Geological Mapping ◽  
Virtual Observatory ◽  
Science Data ◽  
Small Bodies ◽  
Horizon 2020 ◽  
Data Services ◽  
Research And Innovation ◽  
Data Stewardship

<p>The Europlanet-2020 programme, which ended Aug 2019, included an activity called VESPA (Virtual European Solar and Planetary Access) which focused on adapting Virtual Observatory (VO) techniques to handle Planetary Science data. We will present some aspects of VESPA at the end of this 4-years development phase and at the onset of the newly selected Europlanet-2024 programme in Feb 2020. VESPA currently distributes 54 data services which are searchable according to observing conditions and encompass a wide scope including surfaces, atmospheres, magnetospheres and planetary plasmas, small bodies, heliophysics, exoplanets, and lab spectroscopy. Versatile online visualization tools have been adapted for Planetary Science, and efforts were made to connect the Astronomy VO with related environments, e.g., GIS for planetary surfaces. The new programme will broaden and secure the former “data stewardship” concept, providing a handy solution to Open Science challenges in our community. It will also move towards a new concept of “enabling data analysis”: a run-on-demand platform will be adapted from another H2020 programme in Astronomy (ESCAPE); VESPA services will be made ready to use for Machine Learning and geological mapping activities, and will also host selected results from such analyses. More tutorials and practical use cases will be made available to facilitate access to the VESPA infrastructure.</p><p>VESPA portal: http://vespa.obspm.fr</p><p>The Europlanet 2020/2024 Research Infrastructure projects have received funding from the European Union's Horizon 2020 research and innovation programme under grant agreements No 654208 and No 871149</p>

scholarly journals Virtual European Solar & Planetary Access (VESPA): Progress and prospects

2020 ◽  
Author(s):  
Stéphane Erard ◽  
Baptiste Cecconi ◽  
Pierre Le Sidaner ◽  
Angelo Pio Rossi ◽  
Carlos Brandt ◽  
...  
Keyword(s):  
Distribution System ◽  
Data Science ◽  
Large Data ◽  
Open Science ◽  
Planetary Science ◽  
Science Data ◽  
Horizon 2020 ◽  
Data Services ◽  
Related Data ◽  
Research And Innovation

<p>The H2020 Europlanet-2020 programme, which ended on Aug 31<sup>st</sup>, 2019, included an activity called VESPA (Virtual European Solar and Planetary Access), which focused on adapting Virtual Observatory (VO) techniques to handle Planetary Science data [1] [2]. The outcome of this activity is a contributive data distribution system where data services are located and maintained in research institutes, declared in a registry, and accessed by several clients based on a specific access protocol. During Europlanet-2020, 52 data services were installed, including the complete ESA Planetary Science Archive, and the outcome of several EU funded projects. Data are described using the EPN-TAP protocol, which parameters describe acquisition and observing conditions as well as data characteristics (physical quantity, data type, etc). A main search portal has been developed to optimize the user experience, which queries all services together. Compliance with VO standards ensures that existing tools can be used as well, either to access or visualize the data. In addition, a bridge linking the VO and Geographic Information Systems (GIS) has been installed to address formats and tools used to study planetary surfaces; several large data infrastructures were also installed or upgraded (SSHADE for lab spectroscopy, PVOL for amateurs images, AMDA for plasma-related data).</p><p>In the framework of the starting Europlanet-2024 programme, the VESPA activity will complete this system even further: 30-50 new data services will be installed, focusing on derived data, and experimental data produced in other Work Packages of Europlanet-2024; connections between PDS4 and EPN-TAP dictionaries will make PDS metadata searchable from the VESPA portal and vice versa; Solar System data present in astronomical VO catalogues will be made accessible, e.g. from the VizieR database. The search system will be connected with more powerful display and analysing tools: a run-on-demand platform will be installed, as well as Machine Learning capacities to process the available content. Finally, long-term sustainability will be improved by setting VESPA hubs to assist data providers in maintaining their services, and by using the new EU-funded European Open Science Cloud (EOSC). In addition to favoring data exploitation, VESPA will provide a handy and economical solution to Open Science challenges in the field.</p><p>The Europlanet 2020 & 2024 Research Infrastructure project have received funding from the European Union's Horizon 2020 research and innovation programme under grant agreements No 654208 & 871149.</p><p>[1] Erard et al 2018, Planet. Space Sci. <strong>150</strong>, 65-85. 10.1016/j.pss.2017.05.013. ArXiv 1705.09727  </p><p>[2] Erard et al. 2020, Data Science Journal <strong>19</strong>, 22. doi: 10.5334/dsj-2020-022.</p>

The PVOL database in Europlanet 2024 RI

2020 ◽  
Author(s):  
Ricardo Hueso ◽  
Agustin Sánchez-Lavega ◽  
Jon Legarreta ◽  
Iñaki Ordonez-Etxeberria ◽  
Jose Félix Rojas ◽  
...  
Keyword(s):  
Data Access ◽  
Planetary Science ◽  
Space Science ◽  
Virtual Observatory ◽  
The European Union ◽  
Scientific Publications ◽  
Horizon 2020 ◽  
Data Services ◽  
The Impact ◽  
Future Plans

<p>PVOL is an online database of amateur observations of solar system planets hosted by the University of the Basque Country at http://pvol2.ehu.es/ [1]. PVOL stands for Planetary Virtual Observatory and Laboratory and is one of the data services integrated in VESPA: a large collection of data services integrated in the Virtual European Solar and Planetary Access services using the same data access protocol (EPN-TAP) [2]. VESPA is an integral part of the Europlanet 2020 and 2024 Research Infrastructures and PVOL is one of its most used services. PVOL accumulates images provided by more than 300 amateur observers distributed through the globe and currently contains more than 47,000 image files. Most of the data correspond to image observations of Jupiter (67%) and Saturn (22%), but PVOL contains also useful data from Venus, Mars, Uranus and Neptune and some smaller collections of objects with no atmosphere (the Moon and Galilean satellites). In this contribution we document future plans for the service which will be carried out through 2021-2023 and we show the scientific potential of the data available in PVOL.</p> <p>Future plans for PVOL include frequent observation alerts, integration in the database of navigation files of the images from the popular WinJupos software (ims files), addition of amateur spectra of the giant planets, and a search engine and new data service of Jupiter maps obtained from the JunoCam instrument on the Juno mission that will also be integrated in PVOL/VESPA. This will allow to perform combined searches of data obtained close in time from amateurs (PVOL), HST (queries of HST images are also integrated in VESPA) and JunoCam (new service).</p> <p>The science potential of amateur data comes from the availability of long-term data (PVOL contains Jupiter data since 2000 and Mars and Venus data since 2016), frequent observations (several daily observations of each planet close to their oppositions capable to cover complete longitudes of each planet) and high-resolution images provided by key contributors, with some of them capable to resolve highly-contrasted features of 0.05-0.10 arcsec. We review recent trends in analysis of this data from an analysis of scientific publications partially or highly based on data obtained from PVOL. We show that amateur observations remain as a valuable resource for high-impact science on modern research on different planets (3-5).</p> <p><strong>Acknowledgements</strong></p> <p>Europlanet 2024 RI has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149. We are very grateful to the ensemble of amateur astronomers sending their data to PVOL. We are in debt by the quality of many of these observations and the regular observations provided by many of them requiring long sleepless nights and even longer days of detailed image processing.</p> <p><strong>References</strong></p> <p>(1) Hueso et al., The Planetary Virtual Observatory and Laboratory (PVOL) and its integration into the Virtual European Solar and Planetary Access (VESPA). Planet. Space Science, 150, 22-35 (2018).</p> <p>(2) Erard et al., VESPA: A community-driven Virtual Observatory in Planetary Science. Planet. Space Science, 150, 65-85 (2018).</p> <p>(3) Sánchez-Lavega et al., The impact of a large object on Jupiter in 2009 July, Astrophysical Journal Letters, 715, L155 (2010).</p> <p>(4) Sánchez-Lavega et al., An extremely high altitude plume seen at Mars morning terminator. Nature, 518, 525-528 (2015).</p> <p>(5) Sánchez-Lavega et al., A complex storm system in Saturn’s north polar atmosphere in 2018, Nature Astronomy, 4, 180-187 (2020).</p>

Planets in a Room: an educational tool for Europlanet

2020 ◽  
Author(s):  
Livia Giacomini ◽  
Francesco Aloisi ◽  
Ilaria De Angelis ◽  
Stefano Capretti
Keyword(s):  
Online Community ◽  
Low Cost ◽  
Planetary Science ◽  
Science Museum ◽  
Educational Systems ◽  
The European Union ◽  
Non Profit ◽  
Horizon 2020 ◽  
Research And Innovation ◽  
3D Printed

<p>Planets in a room (PIAR) is a DIY kit to build a small, lowcost spherical planet simulator and planetarium projector. Teachers, science communicators that run a small museum or planetarium, planetary scientists, amateur astronomers and other individuals can easily build it and use it on their own, to show and teach the Earth and other planets and to develop and share material with a growing online community. Having started in 2017 with a first version made using 3d-printed technology, PIAR has lately gone green, with a new wooden, plastic-free version of the kit. (http://www.planetsinaroom.net/)</p> <p>The project has been developed by the italian non-profit association Speak Science, with the collaboration of the Italian National Institute for Astrophysics (INAF) and the Roma Tre University, Dipartimento di Matematica e Fisica.</p> <p>It was funded by the Europlanet Outreach Funding Scheme in 2017 and was presented to the scientific community at EPSC and other scientific Congresses in the following years. Today, it is being distributed to an increasing number of schools, science museum and research institutions. PIAR is also one of the projects selected by the Europlanet Society for education and public outreach of planetary science: in 2020, it is being distributed to the 12 Europlanet Regional Hubs all around Europe, to be used in a number of educational projects.</p> <p>In this talk we will review the state of the art of the project presenting a selection of educational material and projects that have been developed for PIAR by scientists, teachers and communicators and that are focused on planetary science and on planetary habitability.</p> <p> </p> <p>Acknowledgements</p> <p>We acknowledge for this project the vast community of amateur and professionals that is actively working on innovative educational systems for astronomy such as planetarium and virtual reality projects (both hardware and software). Planets in a room is based on the work of this vast community of people and their experiences and results. We also acknowledge Europlanet for funding this work: the project Europlanet 2024 RI has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149.”</p> <p> </p> <p>References</p> <p>Giacomini L., Aloisi F., De Angelis I., “Planets in a room”, EPSC Abstracts Vol. 11, EPSC2017-280, 2017</p> <p>Giacomini L., Aloisi F., De Angelis I., Capretti S., “Planets in a Room: a DIY, low-cost educational kit”, EPSC Abstracts Vol. 12, EPSC2018-254, 2018</p> <p>Giacomini L., Aloisi F., De Angelis I., Capretti S., “Planets on (low-cost) balloons”, EPSC AbstractsVol. 13, EPSC-DPS2019-1243-1, 2019</p> <p>Giacomini L., Aloisi F., De Angelis I., Capretti S, “(Green) Planets in a Room”, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-22153, https://doi.org/10.5194/egusphere-egu2020-22153, 2020</p>

The Europlanet Evaluation Toolkit

2021 ◽  
Author(s):  
Anita Heward ◽  
Jen DeWitt
Keyword(s):  
Worked Examples ◽  
Planetary Science ◽  
Hard Copy ◽  
The European Union ◽  
Horizon 2020 ◽  
Evaluation Approach ◽  
Research And Innovation ◽  
Word Clouds ◽  
Interactive Workshop ◽  
The Impact

<div> <p>In this presentation, we will give an overview of the Europlanet Evaluation Toolkit, a resource that aims to empower outreach providers and educators in measuring and appraising the impact of their activities. The toolkit is intended to provide advice and resources that can be simply and easily integrated into normal outreach and education activities. It is available as an interactive online resource (http://www.europlanet-eu.org/europlanet-evaluation-toolkit/), as a downloadable PDF and as a hard copy (including a book and set of activity cards).</p> </div><div> <p>The toolkit has been developed over a number of years with content provided by professional outreach evaluators Karen Bultitude and Jennifer DeWitt (UCL, UK). Initially, a series of focus groups and scoping discussions were held with active outreach providers from the planetary science community in order to determine what they wanted from such a toolkit, and what sort of tools would be of most interest. A shortlist of tools was developed based on these discussions, with volunteers testing out the tool instructions once they were drafted.</p> </div><div> <p>The toolkit begins with a brief introduction to evaluation and steps to choosing the right tools. This advice takes the form of a series of questions to help design an evaluation approach and make the most efficient and effective use possible of limited time and resources.</p> </div><div> <p>The toolkit offers a choice of 14 data collection tools that can be selected according to the audience (e.g. primary, secondary, interested adult, general public), the type of environment and activity (e.g. drop-in, interactive workshop, ongoing series, lecture/presentation or online) or according to when they might best be used (during, beginning/end, or after an event). The online version of the toolkit includes a set of interactive tables to help with the selection of which tool is most appropriate for any given situation.</p> </div><div> <p>The toolkit includes descriptions and worked examples of how to use two techniques (word-clouds and thematic coding) to analyse the data, as well as some top tips for evaluation and recommended resources.</p> </div><div> <p>For some of the tools, case study examples include information about how the tools have been used in the context of an event, how data was actually collected and analysed and what conclusions were reached, based on the data gathered.</p> </div><div> <p>The Europlanet Evaluation Toolkit has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 871149 (Europlanet 2024 RI) and 654208 (Europlanet 2020 RI).</p> </div>

A European Fault Database as a stepping stone towards improved subsurface evaluation of hazards and resources

2021 ◽  
Author(s):  
Serge Van Gessel ◽  
Rob van Ede ◽  
Hans Doornenbal ◽  
Johan ten Veen ◽  
Esther Hintersberger ◽  
...  
Keyword(s):  
The Netherlands ◽  
Pannonian Basin ◽  
Water Injection ◽  
Active Faults ◽  
Geological Mapping ◽  
The European Union ◽  
Stepping Stone ◽  
Horizon 2020 ◽  
Research And Innovation ◽  
Seismogenic Faults

<p>Faults are prominent features in the subsurface that define the geological development and distribution of geological formations and resources therein. Faults can define resources themselves (e.g. minerals, thermal conduits), but more often they can pose a hazard to subsurface drilling, injection and extraction activities . Well-known examples are Basel – Switzerland (geothermal stimulation), Oklahoma – US (waste water injection) and Groningen – The Netherlands (conventional hydrocarbon extraction).</p><p>Despite that faults are a typical product of geological mapping, there was, until now, no consistent insight in these structures in a pan-European context. There are some examples focusing on the publication of seismogenic faults (e.g. GEM Global Active Faults Database, SHARE  European Database of Seismogenic Faults, USGS Quaternary faults database), yet deeply buried faults are under-represented here. With the European fault database, the GeoERA-HIKE project addresses the following objectives: i) develop a consistent and uniform repository for fault data and characteristics across Europe, ii) Implement an associated tectonic vocabulary which provides a framework for future interpretation, modelling and application of fault data, and iii) assess the applicability of fault data in case studies.</p><p>The current fault database is envisioned to be a major stepping stone for a sustained and uniform development and dissemination of tectonic data and knowledge which will be applicable to a broad spectrum of subsurface research challenges. The database contains data from Geological Survey Organizations and partners in the Netherlands, Germany, Austria, Belgium, Iceland, Denmark, Poland, Lithuania, Italy, France, Ukraine, Portugal, Slovenia, Albania and various countries in the Pannonian Basin Area.</p><p>The GeoERA-HIKE project has received funding from the European Union’s Horizon 2020 research and innovation programme under agreement No. 731166</p>

A Standards-based Data Catalogue integrating scientific, community-based and citizen science data across the Arctic

2021 ◽  
Author(s):  
Torill Hamre ◽  
Finn Danielsen ◽  
Michael Køie Poulsen ◽  
Frode Monsen
Keyword(s):  
Citizen Science ◽  
Scientific Community ◽  
The Arctic ◽  
Observation System ◽  
Data Systems ◽  
Science Data ◽  
Community Based ◽  
Horizon 2020 ◽  
Research And Innovation ◽  
Data Collections

<p>INTAROS is a Horizon 2020 research and innovation project developing an integrated Arctic Observation System by extending, improving, and unifying existing systems in the different regions of the Arctic. INTAROS integrates distributed repositories hosting data from ocean, atmosphere, cryosphere and land, including scientific, community-based monitoring (CBM) and citizen science (CS) data. Throughout the project, INTAROS has been working closely with several local communities and citizen science programs across the Arctic, to develop strategies and methods for ingestion of data into repositories enabling the communities to maintain and share data. A number of these CBM and CS data collections have been registered in the INTAROS Data Catalogue. Some of these collections are hosted and sustained by large international programs such as PISUNA, eBird, Secchi Disk Study and GLOBE Observer. Registration in the INTAROS Data Catalogue contributes to making these important data collections better known in a wider community of users with a vested interest in the Arctic. It also enables sharing of metadata through open standards for inclusion in other Arctic data systems. This catalogue is a key component in INTAROS, enabling users to search for data across the targeted spheres to assess their usefulness in applications and geographic areas. The catalogue is based on a world-leading system for data management, the Comprehensive Knowledge Archive Network (CKAN). With rich functionality offered out of the box combined with a flexible extension mechanism, CKAN allows for quickly setting up a fully functional data catalogue. The CKAN open-source community offers numerous extensions that can be used as-is or adapted to implement customised functionality for specific user communities. To hold additional metadata elements requested by the partners we modified the standard database schema of CKAN. The presentation will focus on the current capabilities and plans for sustaining and enhancing the INTAROS Data Catalogue.</p>

scholarly journals FAIR Science for Social Machines: Let's Share Metadata Knowlets in the Internet of FAIR Data and Services

2019 ◽  
Vol 1 (1) ◽  
pp. 22-42 ◽  
Author(s):  
Barend Mons
Keyword(s):  
Scientific Practice ◽  
Critical Role ◽  
Public Funding ◽  
Open Science ◽  
Central Feature ◽  
Relative Role ◽  
Patient Privacy ◽  
Science Data ◽  
Social Machines ◽  
Data Stewardship

In a world awash with fragmented data and tools, the notion of Open Science has been gaining a lot of momentum, but simultaneously, it caused a great deal of anxiety. Some of the anxiety may be related to crumbling kingdoms, but there are also very legitimate concerns, especially about the relative role of machines and algorithms as compared to humans and the combination of both (i.e., social machines). There are also grave concerns about the connotations of the term “open”, but also regarding the unwanted side effects as well as the scalability of the approaches advocated by early adopters of new methodological developments. Many of these concerns are associated with mind-machine interaction and the critical role that computers are now playing in our day to day scientific practice. Here we address a number of these concerns and provide some possible solutions. FAIR (machine-actionable) data and services are obviously at the core of Open Science (or rather FAIR science). The scalable and transparent routing of data, tools and compute (to run the tools on) is a key central feature of the envisioned Internet of FAIR Data and Services (IFDS). Both the European Commission in its Declaration on the European Open Science Cloud, the G7, and the USA data commons have identified the need to ensure a solid and sustainable infrastructure for Open Science. Here we first define the term FAIR science as opposed to Open Science. In FAIR science, data and the associated tools are all Findable, Accessible under well defined conditions, Interoperable and Reusable, but not necessarily “open”; without restrictions and certainly not always “gratis”. The ambiguous term “open” has already caused considerable confusion and also opt-out reactions from researchers and other data-intensive professionals who cannot make their data open for very good reasons, such as patient privacy or national security. Although Open Science is a definition for a way of working rather than explicitly requesting for all data to be available in full Open Access, the connotation of openness of the data involved in Open Science is very strong. In FAIR science, data and the associated services to run all processes in the data stewardship cycle from design of experiment to capture to curation, processing, linking and analytics all have minimally FAIR metadata, which specify the conditions under which the actual underlying research objects are reusable, first for machines and then also for humans. This effectively means that—properly conducted—Open Science is part of FAIR science. However, FAIR science can also be done with partly closed, sensitive and proprietary data. As has been emphasized before, FAIR is not identical to “open”. In FAIR/Open Science, data should be as open as possible and as closed as necessary. Where data are generated using public funding, the default will usually be that for the FAIR data resulting from the study the accessibility will be as high as possible, and that more restrictive access and licensing policies on these data will have to be explicitly justified and described. In all cases, however, even if the reuse is restricted, data and related services should be findable for their major uses, machines, which will make them also much better findable for human users. With a tendency to make good data stewardship the norm, a very significant new market for distributed data analytics and learning is opening and a plethora of tools and reusable data objects are being developed and released. These all need FAIR metadata to be routed to each other and to be effective.

scholarly journals DRIvE Project Unlocks Demand Response Potential with Digital Twins

Proceedings ◽  
2020 ◽  
Vol 65 (1) ◽  
pp. 14
Author(s):  
Laura Pérez ◽  
Juan Espeche ◽  
Tatiana Loureiro ◽  
Aleksandar Kavgić
Keyword(s):  
Knowledge Transfer ◽  
Demand Response ◽  
Low Carbon ◽  
Distribution Grid ◽  
Horizon 2020 ◽  
Research And Innovation ◽  
Digital Twins ◽  
Future Workshop ◽  
Innovative Solutions ◽  
Innovation Project

DRIvE (Demand Response Integration Technologies) is a research and innovation project funded under the European Union’s Horizon 2020 Framework Program, whose main objective is unlocking the demand response potential in the distribution grid. DRIvE presented how the use of digital twins de-risks the implementation of demand response applications at the “Flexibility 2.0: Demand response and self-consumption based on the prosumer of Europe’s low carbon future” workshop within the conference “Sustainable Places 2020”. This workshop was organized to cluster and foster knowledge transfer between several EU projects, each developing innovative solutions within the field of demand response, energy flexibility, and optimized synergies between actors of the built environment and the power grid.

Radial diffusion coefficients database in the frame of SafeSpace project

2021 ◽  
Author(s):  
Christos Katsavrias ◽  
Ioannis A. Daglis ◽  
Afroditi Nasi ◽  
Constantinos Papadimitriou ◽  
Marina Georgiou
Keyword(s):  
Diffusion Coefficients ◽  
Radiation Belt ◽  
Field Measurements ◽  
Radial Diffusion ◽  
Relativistic Electrons ◽  
Outer Radiation Belt ◽  
Horizon 2020 ◽  
Research And Innovation ◽  
The Difference ◽  
Cycle 24

<p>Radial diffusion has been established as one of the most important mechanisms contributing the acceleration and loss of relativistic electrons in the outer radiation belt. Over the past few years efforts have been devoted to provide empirical relationships of radial diffusion coefficients (D<sub>LL</sub>) for radiation belt simulations yet several studies have suggested that the difference between the various models can be orders of magnitude different at high levels of geomagnetic activity as the observed D<sub>LL</sub> have been shown to be highly event-specific. In the frame of SafeSpace project we have used 12 years (2009 – 2020) of multi-point magnetic and electric field measurements from THEMIS A, D and E satellites to create a database of calculated D<sub>LL</sub>. In this work we present the first statistics on the evolution of D<sub>LL </sub>during the various phases of Solar cycle 24 with respect to the various solar wind parameters and geomagnetic indices.</p><p>This work has received funding from the European Union's Horizon 2020 research and innovation programme “SafeSpace” under grant agreement No 870437.</p>

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