Athletes who are cheered on during sporting activities are likely to perform better than athletes who don’t. The HeartLink project is investigating how to remotely cheer athletes while they are participating in sporting events. Dr Franco Curmi writes about his work for the HeartLink project.
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A historical discovery does not always equal the unearthing of new documents or artefacts. Sometimes it’s about re-evaluating what we already know. Prof. Victor Mallia-Milanes tells Tuovi Mäkipere more.
How do you test the sensors in smartphones, smartwatches, and up-and-coming medical devices? With a Femtotools FT-RS1002 Microrobotic System of course! In 2016 the Department of Microelectronics and Nanoelectronics (Faculty of ICT, UoM) set up a slew of devices to be able to to probe, prod and poke devices up to a resolution of 1 nm (thinner than the diameter of a human hair).
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Number of axes: 3 Maximum velocity: 5 mm/s Minimum motion increment: 1 nm Actuation principle: Piezoelectric scanning/stepping Sensor probe tip area: 50 µm x 50 µm FT-S100000 sensor force range: ±100000 µN FT-S100000 sensor resolution at 10Hz: ±5 µN Operating temperature: 5°C to 100°C |
The team of computer scientists collaborated with global semiconductor chip maker ST Microelectronics to p roduce MEMS (Micro-Electro-Mechanical Systems). MEMS are the tiny sensors or devices often found in smartphones that allow them to act like a compass, know how fast a person is going, or detect sound. In Malta, the new equipment is being used to measure mechanical properties (for example shear testing and flexure testing) of tiny mirrors that can be used to turn phones into high-quality projectors (part of the Lab4MEMS2 project part-funded by the EU). This toolkit is incredibly versatile, forming part of a station that can have additional add-ons to widen its applications. Now the team wants to buy more sensitive microforce probes and microgrippers that will allo w the manipulation and assembly of microsystems. This toolkit’s micromechanical testing can be used in many research and industrial applications. This way, the horizon is open for studies into semiconductor technology, microsystem development, materials science, micromedicine, or biotechnology—placing Malta on the semiconductor map.
A magnificent feat of engineering, the LHC goes where no other machine has gone before.
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The Department of Physics, Faculty of Science and the Institute of Space Sciences & Astronomy (ISSA; both at the University of Malta) have just acquired a 5.3m dual-reflector parabolic dish, as part of a European Regional Development Fund (ERDF) project to extend postgraduate research lab facilities. The radio telescope will now allow students and researchers to study celestial objects such as the sun or the centre of the galaxy through the radio waves they emit.
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| Dish diameter: 5.3m
Feed horns: L-Band and K-band Gain: 44 dBi @ 4GHz Observing modes: Continuum and line observation Total weight (including pedestal): 1900 kg Surface accuracy: 0.5mm PC-based automated control unit |
When pointed to a radio-loud celestial object (an object which emits large amounts of radio waves, such as the sun), the telescope will receive radio waves from these sources and convert them to voltage readings in the feed. The converted signal is then transmitted to a digitiser that converts these signals into bits and bytes.
The digitised signals are then processed and broken down into the different frequency counterparts (similar to what a car radio does with the radio waves it receives from its antenna), which allows for continuum observation of the skies above. The telescope provides a test-bed for several research initiatives being undertaken at ISSA.
Some of its specialisations include improving the hardware and software processing back-ends for radio telescopes. The on-site telescope can speed up this sort of research immensely. ISSA is part of the largest radio telescope project in the world: the SKA (Square Kilometre Array).