SOME-UFO

Solar Magnetic Eruptions: Understanding and Forecasting

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 Obiettivo del progetto (Objective)

'We propose a four-year project aiming to first, understand solar eruptions and second, help build a future capacity to predict them, thus contributing to the forecasting of the ever-changing space weather conditions. Inclement space weather has adverse consequences on exposed humans and technological assets in space and near-space environments, and sometimes even on ground-based facilities. As solar eruptive activity is predominantly magnetic in origin, the targeted research objectives will be achieved via a comprehensive, innovative analysis of solar magnetogram data combined with complementary information from other solar data sets. The proposed research topic presents a milestone for modern solar physics, thus carrying significant intellectual weight, and at the same time it may lead to meaningful practical improvements toward the safety and smooth operation of our manned and unmanned space infrastructure.

The proposal coordinator has spent the past nine years in the United States of America, most of them as a Senior Professional Staff Physicist at the Johns Hopkins University Applied Physics Laboratory (JHU/APL) in Laurel, Maryland. As of September 2009 he possesses a tenure-track Assistant Research Professor (Researcher C') position at the Academy of Athens in Athens, Greece. He is also an elected Board Member of the European Solar Physics Division (ESPD; 2008 - 2011). With virtually non-existent institutional funding for travel, publications, and student supervision/mentoring, he applies for Marie Curie IRG funding primarily for these three purposes rather than for salary support. The proposal demonstrates that a Marie Curie IRG Grant will substantially improve his employment conditions and help him solidify his career prospects in Europe at the same time keeping his strong ties with the US solar physics community and providing the European Space Agency (ESA) and the European solar physics community with needed expertise in the study of solar magnetism.'

Descrizione progetto (Article)

Space weather is the term used to describe the interaction between magnetic fields and particles ejected from the Sun and the Earth's magnetic field. This is not only amps surging through our planet's atmosphere. In the case of strong solar eruptions, the operations of satellites and human personnel in orbit may be disrupted. Disruptions may reach all the way to the ground in case of very intense solar eruptions, affecting ground-based communication infrastructures and power grids.

To minimise the impact of adverse space weather on modern technologies, a credible solar-activity forecasting infrastructure needs to be developed. But first, scientists need to understand fundamental physical processes driving space weather. The EU-funded project SOME-UFO (Solar magnetic eruptions: Understanding and forecasting) focused on the complex magnetic configurations of solar active regions, the primary hosts of solar eruptions.

Active regions appear as dark spots on the surface of the Sun. By scrutinizing data from multiple vantage points by aspects of theory, the SOME-UFO team determined changes in twisting magnetic fields in the days leading up to solar flares and how they change by these powerful blasts of energy. The scientists relied on several satellites and ground-based magnetographs to find long-sought clues toward a viable solar-eruption prediction.

One key factor that influences solar-flare triggering is the excess magnetic energy stored in twisted magnetic field lines as electric currents flowing along them. Another factor is the so-called magnetic helicity, providing a measure of the stress and distortion of the magnetic field lines. With this information and critical energy and helicity thresholds for eruptions delivered by the SOME-UFO project, reliable warnings could be possible by the next solar activity maximum.

Currently, forecasters see complex sunspot regions and issue flare alerts, but the when, where, and how strong elude them. The SOME-UFO scientists found the same pattern one active region after another: magnetic field lines twisting to the break point and then relaxing. More importantly, they established that this pattern could pave the way for a reliable tool for predicting a solar flare.

SOME-UFO project findings will be refined over the next few years within two new research initiatives. The European Space Agency (ESA)-funded project A-EFFort (Athens Effective Solar Flare Forecasting) aims to develop an entirely automated flare-forecasting service. On the other hand, the EU-funded project FLARECAST(Flare Likelihood and Eruption Region Forecasting) is devoted to the protection of space assets from wild space weather via another fully automated flare-prediction facility at a much larger scale than A-EFFort, and the first of its kind in the world.