1 The Square Kilometre Array Exploring the Universe with the world s largest radio telescope
2 THE SQUARE KILOMETRE ARRAY 01 In the 20th century, we discovered our place in the Universe. Our telescopes have revealed an expanding Universe with billions of galaxies, each filled with stars of all sizes and temperatures, along with black holes, neutron stars, planets and gas clouds. The Square Kilometre Array The largest and most sensitive radio telescope in the world In the 20th century, we discovered our place in the Universe. Our telescopes have revealed an expanding Universe with billions of galaxies, each filled with stars of all sizes and temperatures, along with black holes, neutron stars, planets and gas clouds. In the 21st century, we now seek to understand the complete evolution of our Universe and its constituents. To address these fundamental questions, a new generation of astronomical facilities is needed with a revolutionary new radio telescope, the Square Kilometre Array (SKA), playing a crucial role. The SKA will be built in Australia and Southern Africa and will comprise thousands of linked radio wave receptors. Recent innovative technological developments in both computing and radio frequency devices have made it possible and affordable for the SKA to be built by With an unprecedented large radio wave collecting area, the SKA will be 50 times more sensitive, and be able to survey the sky times faster, than any imaging radio telescope array previously built. By observing a large volume of the Universe, over much of cosmic time, the SKA will answer many of the fundamental questions we are asking now, and many more that we do not yet know to ask.
3 THE SQUARE KILOMETRE ARRAY 03 THE SQUARE KILOMETRE ARRAY Introduction Radio sky Radio astronomy produced some of the greatest discoveries of the 20th century, including the cosmic microwave background, pulsars and gravitational lenses to name just a few. Central to these discoveries have been innovations in technology pushing the observational frontiers of sensitivity as well as spatial, temporal and spectral resolution. One such innovation in technology - radio interferometry - was awarded a Nobel Prize for Physics. The SKA will carry on this tradition of innovation by combining fundamental developments in radio frequency technology, data transport and high-performance computing. The SKA - A revolution in astronomy The Square Kilometre Array will provide about a million square metres of collecting area. This huge increase in scale compared to existing telescopes demands a revolutionary break from traditional radio telescope design. Three antenna types: dishes, mid frequency aperture arrays and low frequency aperture arrays, will be used to provide continuous frequency coverage from 70 MHz to 10 GHz. To achieve both high sensitivity and high resolution images of the sky the antennas will be densely distributed in the central regions and then positioned in clusters along spiral arms becoming more widely spaced further away from the centre. Combining the signals from the antennas will create a telescope with a collecting area equivalent to a dish with an area of about one square kilometre. The SKA will use three antenna types: dishes, mid frequency aperture arrays and low frequency aperture arrays. Artist s impressions of the concept designs: SKA dish (above); mid frequency aperture array tiles (above right); low frequency aperture array dipoles (below right). The SKA will be the world s premier imaging and surveying telescope with a combination of unprecedented versatility, sensitivity and resolution that will open up new windows of discovery. The galaxies M81 and M82 seen in visible light (above top) and radio frequency (above). Only the radio observations reveal the interaction between the two galaxies in the form of a gigantic stream of gas. (Credit: KNPO, NRAO) The multiple fields-of-view provided by aperture array technology will enable many astronomers to use the SKA telescope and view different areas of the sky at the same time. (Credit: M. Kramer) The sky seen at optical wavelengths (far left), at a radio frequency of 408 MHz (middle) and at the frequency of emission of neutral hydrogen, MHz (right). (Credit: Axel Mellinger/NASA SkyView, G. Haslam/MPIfR, J. Dickey/NASA SkyView) 03
4 THE SQUARE KILOMETRE ARRAY 05 The SKA project The project is led by the SKA Organisation. Based near Manchester, UK, the SKA Organisation is co-ordinating the activities of the international partners. TIMELINE 2024 FULL OPERATION PHASE TWO CONSTRUCTION 2020 The SKA Organisation is co-ordinating the global science and engineering activities for the world s largest radio telescope. FULL SCIENCE OPERATIONS WITH PHASE ONE PHASE ONE CONSTRUCTION DETAILED DESIGN AND PRECONSTRUCTION PHASE 2012 SITE SELECTION TELESCOPE CONCEPTUAL DESIGN 1991 SKA CONCEPT The SKA will: Be the largest radio telescope in the world. Revolutionise our understanding of the Universe and the laws of fundamental physics. Be built in radio-quiet locations in Australia and Southern Africa. Have 50 times the sensitivity and times the survey speed of current imaging instruments. Extend to at least km from one of the central core regions. Have a life span of at least 50 years. Be continuously upgradable as computing power increases. Use new antenna technology, signal transport, signal processing and computing. As the SKA will be an aperture synthesis instrument, comprising many independent receiving elements, exciting science will be achievable before the full array is complete. Initial science results are expected in 2020.
5 THE SQUARE KILOMETRE ARRAY Transformational science The SKA will be a highly flexible instrument designed to address a wide range of fundamental questions in astrophysics, cosmology, particle astrophysics and astrobiology. The exceptional sensitivity and resolution will enable the SKA to probe previously unexplored parts of the distant Universe. A number of key science projects have been selected: (Credit: T.A. Oosterloo/ASTRON) Probing the Dark Ages - the first black holes and stars. Galaxy evolution, cosmology and dark energy. The origin and evolution of cosmic magnetism. The cradle of life - searching for life and planets. Extreme tests of general relativity with pulsars and black holes. (Credit: M. Bietenholz/York/NRAO) The SKA will observe the very first black holes, stars and galaxies that shaped the development of the Universe. While these projects address important scientific questions of our time, we cannot foresee the unexpected discoveries that the SKA will make. What is clear is that our understanding of the Universe and its fundamental physics will be transformed by the SKA. One of the design goals is therefore to maximise the SKA s ability to explore the unknown. Comparison of current radio observations (far left) and a simulation of SKA observations (left) showing the greatly increased number of faint galaxies expected in observations of the continuum radio sky. (Credit: C. Jackson/ CSIRO) (Credit: MERLIN) (Credit: W. Reich/MPIfR) (Credit: Kassim/NRL/NRAO) 07
6 THE SQUARE KILOMETRE ARRAY What happened just after the Big Bang? Which came first - stars or galaxies? KEY SCIENCE PROJECT: xhi=0.79 xhi=0.61 xhi=0.42 xhi=0.20 Probing the Dark Ages the first black holes and stars After the Big Bang the Universe expanded and cooled, turning the hot primordial soup of particles into a sea of neutral gas. The process started the period in the evolution of the Universe referred to as the Dark Ages. As the name suggests, there was no light in the Universe during the Dark Ages except for the faint glow remaining from the Big Bang. The small density inhomogeneities left over from the period of fast initial expansion gradually grew under the force of gravity, and eventually formed the first stars and galaxies. The light from these first objects slowly reionised the whole intergalactic medium and ended the Dark Ages. option to look at the first few hundred million years of the evolution of the Universe and the first stars. Moreover, HI 21 cm studies of the neutral intergalactic medium may be the most important window on cosmology since the discovery of the cosmic microwave background. Radio emission in the 21 cm line of neutral hydrogen (HI), as well as molecular lines like those from carbon monoxide (CO) provide the best observational windows through which to detect directly the era when gas in galaxies was first turned into stars. The SKA will be the only telescope able to directly detect this distant epoch, thus providing our best The SKA will observe the very first black holes, stars and galaxies that shaped the nascent Universe during this time. The SKA will even be able to detect black holes accreting during the Dark Ages. The SKA will provide detailed pictures and full 3D maps of the early cosmic web of neutral gas, the key to understanding the Universe that we live in today. Simulation snapshot of the complex geometry of reionisation. The galaxies are shown as dark dots, the ionised gas surrounding them is light orange and the neutral gas which the SKA will see is dark green. (Credit: I. Iliev, G. Mellema) Accreting black holes, such as those forming just after the Dark Ages, may very well be radio signposts of the first structures forming. Not only are these first supermassive black holes important in understanding how galaxies formed, they may also influence their environment. The cosmic web of early structures. Simulated image showing the neutral hydrogen sky in the early Universe as seen by the SKA. Galaxies (bright points) form along filaments and sheets in a honey-comb fashion surrounding vast low-density voids (dark regions). (Credit: I. Iliev, G. Mellema and collaborators/u. Toronto) 0 (ARCMIN) Pockets of neutral gas (black) becoming more ionised (white) with increasing age of the Universe. The cube is 100 Mpc on a side. (Credit: S. Furlanetto) V (MHz) 160 Simulated evolution of the 21 cm emission of neutral hydrogen from the Dark Ages through the epoch of reionisation. Light shows the neutral areas, dark the ionised ones. Horizontally going to the left we look back in time (lower frequency), while the vertical scale shows angle on the sky. The SKA should be able to see this evolution in detail. (Credit: I. Iliev, G. Mellema) The giant elliptical galaxy, NGC1316 or Fornax A, shown in the radio (orange) superimposed on an optical image. The radio emission consists of two large radio lobes, each about light years across. The giant elliptical galaxy at the centre is cannibalising a smaller galaxy, stripping away material from it that spirals toward a super-massive black hole at the centre of its larger neighbour. (Credit: NRAO, STSci/POSS-II) 09
7 THE SQUARE KILOMETRE ARRAY What is mysterious dark energy? How are galaxies born and how do they evolve? KEY SCIENCE PROJECT: A simulated SKA observing cone depicting the complex filamentary structure of HI on cosmic scales, which encodes the mysterious physics of the dark Universe. Each coloured pixel in the cone represents a galaxy emitting neutral hydrogen (HI, rest-frame 21 cm) radiation. (Credit: Danail Obreschkow (Oxford) and the SKADS Sky Simulation team) The evolution of the Universe and the formation of large scale structure appear to be governed by the strange action of a dark energy. Apart from the observed fact that dark energy has caused a recent acceleration in the expansion of the Universe, its properties are virtually unknown. DARK ENERGY 73% COLD DARK MATTER 23% NORMAL MATTER 4% Illustration of the recent finding that the vast majority of the Universe is filled with some unknown dark energy and the yet to be identified cold dark matter. There may also be a significant fraction of hot dark matter. Only a small fraction of the Universe is made up of the normal matter that consists of atoms. The structure of the Universe can be determined by observing the cosmic distribution of nature s most fundamental element - hydrogen. Hydrogen is the most abundant element in the Universe and the raw material from which stars form. It is now well established that the rate of star formation in galaxies has evolved dramatically over the last half of the Universe s lifetime. Yet over the same interval, the amount of neutral hydrogen gas appears to have barely changed. Gaining a thorough understanding of galaxy assembly, growth, and evolution remains one of the key challenges for astrophysics. By investigating how galaxies turn gas into stars, the SKA will allow us to understand galaxy formation and evolution. The SKA will track how neutral hydrogen flows into and out of galaxies and will also be able to monitor how gas is exchanged or lost as clusters of galaxies interact with each other. With these data the SKA will measure the geometry of the Universe, and test whether dark energy is a vacuum energy or something more exotic, perhaps providing evidence of genuinely new physics or extra dimensions. Revealing the large-scale structure of the Universe with the SKA will also allow the determination of both the neutrino mass scale and the number of massive neutrinos, connecting astrophysics with particle physics. The SKA and its wide field of view will allow the accurate determination of the rate of evolution in the equation of state of dark energy with cosmic time Wm Wm-2 Simulation of the filamentary structure of the dark matter today. (Credit: Millennium Gas simulation by F. Pearce/Virgo Consortium) 85MPC = 1 Galaxy evolution, cosmology and dark energy SKA MPC Z A SIMULATED SKA OBSERVING CONE Combined optical (colours) and radio (contours) image showing the gravitational lens system B where dark matter associated with two galaxies produces multiple images of a background source. (Credit: HST/STScI, MERLIN) 11
8 Where do we find cosmic magnets and what do they look like? How does magnetism affect star and galaxy formation? What generates these giant magnetic fields in space? THE SQUARE KILOMETRE ARRAY 13 KEY SCIENCE PROJECT: The origin and evolution of cosmic magnetism Magnetic fields play important roles in the Universe. This shows magnetic field loops in the Sun s corona in X-ray light. (Credit: TRACE mission/nasa) One of the many remarkable discoveries made by 20th century astronomers was that stars, planets, galaxies, and even diffuse interstellar gas, are all magnetic. Surprisingly, our Universe seems to be free of magnetic charges (monopoles) which would quickly destroy any magnetic field, ensuring that magnetism is long lived. These cosmic magnetic fields play a vital role in controlling how stars and galaxies form, age and evolve. In addition, this naturally occurring magnetism regulates solar activity and space weather, protects the Earth from harmful particles, and is vital for the navigation of birds and other species. However, in spite of the importance and ubiquity of astrophysical magnets, we do not understand what creates them, or how they maintain their strength over billions of years of cosmic time. With the SKA, we can finally open the window to this magnetic Universe. Magnetic fields are illuminated by electrons spiralling around the field lines which emit radio waves, called synchrotron emission. Astronomers will also use the SKA to exploit an effect called Faraday rotation, in which polarised radio light from a background object is subtly changed when it passes through a cloud of gas in which significant magnetism is present. By measuring Faraday rotation in the radio emission from tens of millions of faint, distant, galaxies, the SKA will be able to detect magnetic fields throughout the Universe. The resulting three-dimensional maps of magnetism in the Milky Way, in nearby galaxies and in intergalactic space will reveal what cosmic magnets look like, where they have came from, and what role they have played in the evolving Universe. The SKA will investigate cosmic magnetism by observing Faraday rotation of polarised radio waves. Two possible sources for the intergalactic magnetic field are the jets in Active Galactic Nuclei (AGNs) and Pulsar Nebulae. These images show well studied examples of the AGN and surrounding radio galaxy 3C353 (top) and the Crab supernova remnant (below) which harbours a radio pulsar. (Credit: NRAO) Optical image of the spiral galaxy M51 with the magnetic field determined from radio observations superimposed. (Credit: Hubble Heritage/NASA/ STSci, R. BECK/MPIfR)
9 Are we alone in the Universe? Could the complex molecules in star forming regions be the starting point for life? Do Earth-like planets orbit other stars? KEY SCIENCE PROJECT: The cradle of life - searching for life and planets The first of these questions is one of the most fundamental problems that has been contemplated by humanity across the ages. The 21st century may see this question answered definitively, with the SKA playing a key role. Concept of an extrasolar planet. (Credit: NASA) The first decade of the 21st century has seen an explosion in the number of planets identified outside the solar system. None of these are known to harbour life. Yet, the possibility of finding life-supporting planets has moved from mere speculation to being a goal of astronomers. Observations with the SKA will contribute to a wide range of astrobiological goals, from understanding how planets form, to searching for exoplanets. The gas from which stars form is known to contain surprisingly complex organic molecules. Today, molecules containing as many as 13 atoms are known. Do even more complex molecules exist? Might some of these complex molecules include the building blocks of life? With its exquisite sensitivity, the SKA will be able to probe for more rare and exotic species of molecules. Most of the planets in the Milky Way galaxy may orbit stars that are small and cool, known as M dwarves. The SKA s superb angular resolution will also enable it to monitor the motions of these stars, looking for any tell-tale wobbles caused by orbiting planets. The Earth s radio wave radiation is generated by humans, by our TV transmitters, radars, and other transmissions. Detection of artificial transmissions from a planet around another star would be the most compelling evidence for life elsewhere and a profound moment for all of humanity. While searches for extraterrestrial transmission have been conducted before, the SKA sensitivity will allow, for the first time, signals to be detected from nearby stars that are no stronger than those generated by our own 21st century TVs and radars. THE SQUARE KILOMETRE ARRAY The cycle of life. Interstellar gas and molecules form stars, planetary disks and finally planets, before a dying star redistributes the ingredients back into space. During this cycle complex organic molecules are formed. (Credit: B. Saxton/NRAO) 15
10 Was Einstein right or will general relativity eventually fail? Are there still ripples in space-time from the early Universe? What are the properties of black holes? THE SQUARE KILOMETRE ARRAY The best test so far of Einstein s theory in strong gravitational fields is provided by the only known double pulsar system, where two pulsars orbit each other in 145 min. (Credit: M. Kramer) KEY SCIENCE PROJECT: Extreme tests of general relativity with pulsars and black holes Pulsar orbiting a black hole. Einstein s theory of general relativity has passed all tests with flying colours, so far. But, it may still not be the last word in our understanding of nature s most fundamental force - gravity. Scientists around the world are struggling to find a theory of quantum gravity which would combine gravitation with the bizarre world of quantum physics. Most theories of gravity also predict ripples in We can confront Einstein s predictions and those of other theories of gravity experimentally by exploiting the Universe s best clocks - pulsars. The SKA will discover tens of thousands of them, some of which will orbit stellar-sized and supermassive black holes. These systems can be used to put Einstein s theories to the most extreme test ever, in particular general relativity s description of black holes. pulsars, the SKA will act as a huge gravitational space-time which propagate through the Universe as gravitational waves. While pulsars provide the only evidence for the existence of gravitational waves so far, they do not only produce them but observations of pulsars can also lead to the detection of gravitational waves. Using Pulsars discovered and monitored with the SKA will act like a cosmic gravitational wave detector, allowing the study of ripples in the fabric of spacetime that propagate at ultra-low frequencies. (Credit: D. Champion, M. Kramer) wave detector, discovering and studying spacetime ripples left over from the early Universe from exotic phenomena like cosmic strings or merging super-massive black holes. The SKA will be sensitive to nano-hz frequencies which are much lower than those probed by ground-based detectors such as the Laser Interferometer Gravitational-wave Observatory (LIGO) or planned space-based detectors like the Laser Interferometer Space Antenna (LISA). Pulsars orbiting black holes will test Einstein s description of these enigmatic objects to the extreme. (Credit: M. Kramer) 17
11 THE SQUARE KILOMETRE ARRAY 19 Exploration of the unknown Putting technology to the test Can we predict everything in the Universe on the basis of what we know now? What else will we discover when exploring the cosmic frontier? The SKA is a tool for as-yet-unborn users and must therefore be a versatile, multi purpose instrument with flexibility that allows us to expect the unexpected. Radio astronomy was responsible for many of the fundamental discoveries in physics and astrophysics in the last century. The list is long and includes: The cosmic microwave background Quasars Pulsars Gravitational lenses Masers Interstellar molecules The first extrasolar planets Galactic magnetic fields Many of the discoveries happened unexpectedly, so we should be prepared for the possibility. However, the scientific challenges outlined in previous pages are today s most exciting problems - will they still be the outstanding problems that will confront astronomers and humankind in the period 2020 to 2050 and beyond, when the SKA will be in its most productive years? If history is any example, the excitement of the SKA may not arise out of current questions, but from new questions that will be raised by the new types of observations that the SKA will permit. The unique sensitivity, multiple independent views of the sky, and the extremely large field-of-view make the SKA a discovery machine. We cannot predict what we will find, but we know it will surprise us. Cosmic explosions of unknown type may be detectable as radio signals with the SKA. (Credit: NASA) Optical fibres will be essential to transport the huge amount of data to the central SKA processor node. (Credit: Wikimedia Commons) The SKA - a technological and engineering challenge The SKA demands new approaches to radio telescope design. The path to the SKA involves mass producing low cost antennas and using programmable signal processing engines as well as addressing the challenge of transporting high data rates across large distances. After undergoing fast, high resolution sampling up to 160 Gbit/sec of data will be transmitted from each dish to a central processor. Data transport from the dishes alone will produce ten times the current global internet traffic. The use of wide field of view expansion technologies could increase total data rates for the SKA to many petabits (10 15 ) per second of data, which represents over 100 times the internet traffic data rates today. Processing and post-processing will require exascale central computing engines (10 18 operations per second). The SKA will also stretch algorithm development in two vital areas. Faster and better ways will be needed to make the high dynamic range (106:1) images central to SKA science drivers New technology and progress in fundamental engineering science are both required. Areas of particular relevance include: Low cost collecting area Low noise, highly integrated, receivers Phased array antenna technology Wideband optical fibre signal transport systems Fast, high resolution, analogue-to-digital converters High performance computing engines Data storage and innovative retrieval technologies and effective radio interference (RFI) mitigation algorithms will also be required. Pushing the instrument in the direction of a software telescope allows designers to take advantage of Moore s law for digital hardware - processing power doubles every 18 months. Image of the cosmic microwave background radiation (CMB) anisotropy. (Credit: WMAP/NASA)) Data transport from the dishes will produce ten times the current global internet traffic.
12 Pivotal SKA technology is being demonstrated with a suite of precursor and pathfinder telescopes and design studies by SKA groups around the world. Pivotal SKA technology is being demonstrated by SKA groups around the world with a suite of precursor and pathfinder telescopes, and design studies. The SKA project is building on THE SQUARE KILOMETRE ARRAY 21 Precursors, pathfinders and design studies the experience gained to develop innovative technologies, models and operational strategies suitable for the SKA telescope. The Australian SKA precursor ASKAP. (Credit: Rob Millenaar) The South African SKA precursor demonstrator KAT-7. (Credit: Dr Nadeem Oozeer) Examples of SKA precursor and pathfinder instruments. Above: Arecibo (Credit: NAIC Arecibo Observatory a facility of the NSF); top right: The Murchison Widefield Array (MWA) (Credit: Dr Natasha Hurley- Walker, ICRAR); middle right: The international LOFAR (low frequency array) telescope (Credit: Top-Foto Assen); right: The Very Large Array (VLA). The Expanded Very Large Array (EVLA) project is an SKA pathfinder project (Credit: NRAO AUI, Bob Tetro); far right: The Electronic Multi Beam Radio Astronomy Concept (EMBRACE) (Credit: ASTRON).
13 THE SQUARE KILOMETRE ARRAY SKA location The sites On 25th May 2012 the members of the SKA Organisation agreed on a dual site implementation for the Square Kilometre Array telescope. The ASKAP and MeerKAT precursor telescopes in Australia and South Africa will be integrated into phase one of the SKA, building on their unique science capabilities. The SKA will be constructed in two phases: Phase one 190 SKA dishes and 64 MeerKAT dishes equipped with single pixel feeds will be located in South Africa (SKA1 dish mid). 60 SKA dishes and 36 ASKAP dishes equipped with phased array feeds will be located in Australia (SKA1 dish survey). 50 stations of low frequency aperture array antennas, with about antennas per station, will be located in Australia (SKA1 AA low). Phase two The dish array will be extended to about dishes with a maximum separation of km across Southern Africa (SKA2 dish mid). South Africa Australia The low frequency aperture arrays will be extended to 250 stations in Australia (SKA2 AA low). A new component comprising 250 mid frequency aperture array stations will be located in South Africa (SKA2 AA mid). 23
14 Much of the SKA design challenge lies in transporting high data rates across large distances. SKA and industry The SKA: a science and engineering partnership THE SQUARE KILOMETRE ARRAY 25 Radio astronomy provides a demanding yet open, development and test environment for state-of-the-art devices, information and communication technology, high performance computing and software. Construction of the SKA over a seven year period is equivalent to building and commissioning a 100 m radio telescope every 20 days a task beyond the experience of the astronomy community. Large scale industry involvement will therefore be necessary. Even before the construction phase, many of the R&D programs needed for SKA demonstrators require industry experience, especially in crucial areas such as economic mass production, system engineering and mega-scale project management. The international SKA project, and its associated national programs, welcome interest from potential industry collaborators. Joint research and development is viewed as a shared-risk endeavour with the potential for exploitation of intellectual property. Advantages of industry collaboration beyond commercial contracts: Potential for early involvement in a project spanning a range of engineering and computing disciplines. The ability to perfect leading edge technologies and products in association with the users of a technologically demanding application. Increased visibility of being associated with an innovative international mega-science project. The ability to generate and share information with R&D partners in an open environment. The opportunity to interact with creative professionals in a highly imaginative project. Artist s impression of the SKA layout on the ground in the central core regions. (Credit: SKA Community, C. Walsh)
15 THE SQUARE KILOMETRE ARRAY 27 The design, construction and operation of the SKA will impact skills development in science, engineering and in associated industries, not only in the host countries but in all countries involved. Beyond astronomy The SKA will deliver benefits beyond astronomy The SKA is driving technology development in antennas, data transport, software and computing, and power. Spin off innovations in this area will benefit other systems that process large volumes of data from geographically dispersed sources. Systems that carry out high speed detection and analysis could also benefit intelligent surveillance for the recognition of faces in a crowd, weather and traffic monitoring and monitoring of financial and retail markets. The energy requirements of the SKA present an opportunity to accelerate technology development in scalable renewable energy generation, distribution, storage and demand reduction. The SKA project offers an environment in which governments, industry and research organisations can work together in a global partnership with a mutually beneficial common goal. The SKA offers an environment in which governments, industry and research groups can work together in a global partnership with a mutually beneficial common goal. The influence of the SKA extends beyond radio astronomy. The project has the potential to provide longstanding human capital development and employment benefits. The design, construction and operation of the SKA will impact skills development, employment and economic growth in science, engineering and associated industries, not only in the host countries but in all partner countries.