First results from LUCID: schools start mapping cosmic rays and solar wind
LUCID tracks the direction of incoming cosmic ray and solar wind particles in three dimensions and determines the type of particle, the energy it deposits and the resulting radiation dose. Monitoring these energetic particles is important for understanding space weather and protecting astronauts from high levels of radiation. LUCID has captured half a million frames to date during its commissioning phase and a further 250,000 will be captured over the summer to build up a map of the radiation environment.
LUCID was launched on 8th July 2014 on the Innovate UK-funded TechDemoSat-1, which carries payloads from a number of UK academic and governmental institutions. The LUCID project was first conceived by students in 2008 and was constructed by Surrey Satellite Technology Ltd. It is one of a number of research projects developed at the Langton Star Centre, the research centre of the Simon Langton Grammar School in Kent.
“When orbiting the sunlit side of Earth, the signal detected by LUCID is dominated by the solar wind, allowing it to map the number and energy of protons and electrons against geographical area and time. But when LUCID is shielded from the Sun on the night-time leg of its orbit, we can identify cosmic ray events,” said Hewitt.
Hewitt, who has just finished his GCSE exams, has worked with a team of students to prepare LUCID for upcoming major runs of data. To access the computing power needed for LUCID data analysis, Hewitt has become the youngest student certified to use GridPP, the UK’s contribution to the worldwide grid of thousands of computers that process data from the world's largest particle accelerator, the Large Hadron Collider (LHC).
“LUCID has been developed from pixel detectors used at the LHC, which were originally designed for medical imaging. This type of detector has never been used before in open space. Our first data was extremely noisy but we have optimised detector settings for day and night captures. The initial processing of data has been automated and masking of pixels has been corrected to improve the quality of track imaging,” said Hewitt.
The concept of involving school students in cutting edge research through the Langton Star Centre is the brainchild of teacher Professor Becky Parker. The programme is now being rolled out nationally through the establishment of the Institute for Research in Schools.
“There are huge benefits to supporting authentic research in schools: increased student engagement, aspiration and take up of STEM subjects, a reinvigorated teaching profession, improved transition between school and university, increased enthusiasm amongst girls for physics and engineering,” said Parker. “This is certainly the case in our school and we would like to see schools across the country benefit from the same opportunities through the Institute for Research in Schools.”
Images, animation and captions
Dr Robert Massey
Royal Astronomical Society
Mob: +44 (0)794 124 8035
Ms Anita Heward
Royal Astronomical Society
Mob: +44 (0)7756 034 243
Dr Sam Lindsay
Royal Astronomical Society
Mob: +44 (0) 7957 566 861
Visiting Professor, School of Physics and Astronomy, Queen Mary, University of London
Director, Institute for Research in Schools
Director, Langton Star Centre
Mob: 07749 708583
The LUCID experiment
LUCID is able to characterise the energy, type, intensity and directionality of high energy particles thanks to its five Timepix detector chips. These have been developed by the Medipix2 Collaboration, originally for medical applications in X-ray imaging. The chips are arranged in an open-faced cube configuration and have an aluminium covering to shield the detector from low energy background particles.
The nationwide roll out of LUCID data has been made possible by a Science in Society Large Award from the Science and Technology Facilities Council (STFC). It is part of a wider programme of engagement with data from these detector chips called CERN@school, which is hosted at the Langton Star Centre. CERN@school is managed by Dr Elizabeth Cunningham of STFC. Dr Tom Whyntie, a CERN scientist, is the “Schools Research Champion” for CERN@school and is supported by a Special Award from the Royal Commission for the Exhibition of 1851 and the GridPP Collaboration.
Part-funded by the UK’s innovation agency, Innovate UK and South East England Development Agency (SEEDA), TechDemoSat-1 (http://www.sstl.co.uk/Missions/TechDemoSat-1/TechDemoSat-1) is a collaborative project to bolster the UK’s thriving space industry by providing a low-cost opportunity for innovative commercial and research payloads under development in the UK to gain flight heritage. It is planned to fly in a polar orbit, an altitude of approximately 635 km, for three years after it launches. LUCID is one of eight UK payloads onboard TechDemoSat-1.
Notes for editors
The Royal Astronomical Society National Astronomy Meeting (NAM 2015) will take place in Venue Cymru, Llandudno, Wales, from 5-9 July. NAM 2015 will be held in conjunction with the annual meetings of the UK Solar Physics (UKSP) and Magnetosphere Ionosphere Solar-Terrestrial physics (MIST) groups. The conference is principally sponsored by the Royal Astronomical Society (RAS) and the Science and Technology Facilities Council (STFC). Follow the conference on Twitter
The Royal Astronomical Society (RAS), founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organises scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 3800 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others. Follow the RAS on Twitter
The Science and Technology Facilities Council (STFC) is keeping the UK at the forefront of international science and tackling some of the most significant challenges facing society such as meeting our future energy needs, monitoring and understanding climate change, and global security. The Council has a broad science portfolio and works with the academic and industrial communities to share its expertise in materials science, space and ground-based astronomy technologies, laser science, microelectronics, wafer scale manufacturing, particle and nuclear physics, alternative energy production, radio communications and radar. It enables UK researchers to access leading international science facilities for example in the area of astronomy, the European Southern Observatory. Follow STFC on Twitter
The Langton Star Centre (http://thelangtonstarcentre.org ) gives school students opportunities to work on authentic research projects alongside scientists and engineers from academia and industry. The students experience real science and their teachers are reinvigorated by involvement in cutting-edge work in their subject. This new approach leads to an increase in the uptake of STEM subjects in schools, and has been piloted in 50 locations for physics-based research and five school/university partnerships for biosciences research. At the Simon Langton Grammar School for Boys, a state school with a mixed sixth form and the home of the Langton Star Centre, uptake into AS/A2 physics has increased to over 230 students in the sixth form. The Langton supplies almost 1% of the total entry to physics undergraduate courses, and 2% of female undergraduate physicists.
The Institute for Research in Schools is dedicated to promoting school-based student research across the UK. It provides consultancy and online resources for launching and sustaining inspirational projects.
Follow the Langton Star Centre on Twitter via @LangtonStar and Facebook via https://www.facebook.com/LangtonStarCentre