1-D broadside-radiating leaky-wave antenna based on a numerically synthesized impedance surface

A newly-developed deterministic numerical technique for the automated design of metasurface antennas is applied here for the first time to the design of a 1-D printed Leaky-Wave Antenna (LWA) for broadside radiation. The surface impedance synthesis process does not require any a priori knowledge on the impedance pattern, and starts from a mask constraint on the desired far-field and practical bounds on the unit cell impedance values. The designed reactance surface for broadside radiation exhibits a non conventional patterning; this highlights the merit of using an automated design process for a design well known to be challenging for analytical methods. The antenna is physically implemented with an array of metal strips with varying gap widths and simulation results show very good agreement with the predicted performance

Beam scanning by liquid-crystal biasing in a modified SIW structure

A fixed-frequency beam-scanning 1D antenna based on Liquid Crystals (LCs) is designed for application in 2D scanning with lateral alignment. The 2D array environment imposes full decoupling of adjacent 1D antennas, which often conflicts with the LC requirement of DC biasing: the proposed design accommodates both. The LC medium is placed inside a Substrate Integrated Waveguide (SIW) modified to work as a Groove Gap Waveguide, with radiating slots etched on the upper broad wall, that radiates as a Leaky-Wave Antenna (LWA). This allows effective application of the DC bias voltage needed for tuning the LCs. At the same time, the RF field remains laterally confined, enabling the possibility to lay several antennas in parallel and achieve 2D beam scanning. The design is validated by simulation employing the actual properties of a commercial LC medium

Low Earth orbit microsatellite constellation utilizing satellite Hellas Sat 5 as a relay

Με δεδομένο ότι βρισκόμαστε σε μια εποχή ορόσημο για την ανάπτυξη στον διαστημικό τομέα, το σύνολο σχεδόν όλων των ανεπτυγμένων χωρών έχει συνειδητοποιήσει ότι η επένδυση στο σύνολο των διαστημικών τεχνολογιών αποτελεί μονόδρομο ανάπτυξης και ευημερίας. Τα δαπανούμενα ποσά είναι απολύτως ενδεικτικά της φρενίτιδας που επικρατεί στη λεγόμενη κούρσα του διαστήματος. Η εισαγωγή πλέον και του ιδιωτικού τομέα στη κούρσα αυτή έχει επιτρέψει την προώθηση του ανταγωνισμού κάτι το οποίο με τη σειρά του έχει ελαττώσει εντυπωσιακά το κόστος χρήσης και αξιοποίησης του διαστημικού τομέα. Αυτό το νέο διαστημικό οικοσύστημα που έχει αναπτυχθεί παγκοσμίως τις τελευταίες δεκαετίες, έχει επιτρέψει τη πρόσβαση στις διαστημικές τεχνολογίες από το σύνολο σχεδόν των χωρών του πλανήτη, τη στιγμή που κατά τις προηγούμενες δεκαετίες, οι μοναδικές χώρες που είχαν τη δυνατότητα να επενδύσουν στον τομέα ήταν οι ΗΠΑ και οι Ρωσία. Δορυφορική παρατήρηση της γης, πλοήγηση, αποτροπή φυσικών καταστροφών, εξερεύνηση του διαστήματος, επιστημονική ανάλυση της επιφάνειας του εδάφους, εκμετάλλευση φυσικών πόρων αλλά και πολιτικές και στρατιωτικές τηλεπικοινωνίες, είναι μόνο μερικές από τις νέες τεχνολογίες που έχει να προσφέρει ο διαστημικός τομέας. Κάθε ένας από αυτούς τους τομείς μπορεί δυνητικά να αποτελέσει πυλώνα ανάπτυξης αν αξιοποιηθεί σωστά και πλέον όλες οι χώρες έχουν συνειδητοποιήσει πως η επένδυση σε κάποιον ή και σε όλους αυτούς τους τομείς μπορούν να επιφέρουν πολλαπλά οφέλη. Ένα χαρακτηριστικό παράδειγμα του νέου διαστημικού οικοσυστήματος που έχει διαμορφωθεί κατά τις τελευταίες δεκαετίες και που δείχνει το πόσο πολύ επενδύουν πλέον οι χώρες στον διαστημικό τομέα, είναι ο υπερδιπλασιαμός των ενεργών δορυφορικών συστημάτων κατά τη πενταετία 2015 – 2020, ιδιαίτερα των τηλεπικοινωνιακών. Αξίζει να σημειωθεί πως τον Δεκέμβριο του 2015, σύμφωνα με τα στοιχεία της UCS, ο αριθμός των ενεργών δορυφόρων του έτους ανήλθε σε 1.381, αριθμός ο οποίος κατά τον ίδιο μήνα του έτους 2020 είχε φτάσει τους 3.372. Έχοντας πει όλα τα παραπάνω, η παρούσα διπλωματική εργασία στοχεύει στην παρουσίαση μιας ολοκληρωμένης ανάλυσης όλων των απαιτούμενων βημάτων που πρέπει να εξετάσει ένας μηχανικός / σχεδιαστής συστημάτων προκειμένου να κατασκευάσει και να αναπτύξει μια πλήρως λειτουργική και αξιόπιστη δορυφορική ζεύξη επικοινωνίας. Η μεθοδολογία περιλαμβάνει μια πλήρη περιγραφή των βασικών νόμων του διαστημικού περιβάλλοντος καθώς και μια εκτενή ανάλυση της τροχιακής μηχανικής και των παραμέτρων. Η ιδέα ήταν να παρουσιαστεί πώς η θεωρία μπορεί να εφαρμοστεί σε μια πραγματική δορυφορική προσομοίωση καθώς και πώς επηρεάζεται από αυτήν. Το τελευταίο βήμα ήταν ο σχεδιασμός και η κατασκευή ενός πραγματικού συστήματος δορυφορικής επικοινωνίας σε ένα εξειδικευμένο λογισμικό και η παρουσίαση των αποτελεσμάτων. Το κύριο συμπέρασμα της παραπάνω υλοποίησης είναι το γεγονός ότι μέσω της χρήσης ενός αστερισμού δορυφόρων χαμηλής Γήινης τροχιάς σε συνδυασμό με έναν γεωστατικό δορυφόρο που χρησιμοποιείται αναμεταδότης, είναι δυνατό να επιτευχθεί μια ανθεκτική και αξιόπιστη επικοινωνιακή ζεύξη με εξαιρετικά υψηλούς ρυθμούς μετάδοσης δεδομένων και σχεδόν παγκόσμια κάλυψη.Given that we are in a landmark era of the space sector development , most countries have realized that an investment in space technologies is the only way for development and prosperity. The invested budgets are absolutely indicative of the so-called space race. The introduction of the private sector in this race has allowed the promotion of competition, which in turn has dramatically reduced the cost of using and exploiting the space sector. This new space ecosystem that has been developed worldwide in recent decades, has allowed access to space technologies from almost all countries on the planet, while in previous decades, the only countries that had the opportunity to invest in the sector were USA and Russia. Satellite earth observation, navigation, prevention of natural disasters, space exploration, scientific analysis of the earth's surface, exploitation of natural resources, but also civil and military telecommunications, are just some of the new technologies that the space sector has to offer. Each of these sectors can potentially be a pillar of development if exploited properly and almost all of the modern countries have realized that investing in one or all of these sectors can offer multiple benefits. A typical example of the new space ecosystem that has been formed during the last decades and that shows how much money countries are now investing in the space sector, is the dramatic increase of the active satellite systems during the years 2015 – 2020, especially the telecommunication ones. It is worth mentioning that in December 2015, according to UCS data, the number of active satellites was 1.381, a number which during the same month in 2020 reached the astonishing number of 3.372. The rapid development of the space sector combined with the cost reducing methods that private sectors have introduced, is showing that the imminent future seems to be very promising. Having said all of the above, this thesis aims at presenting a comprehensive analysis of all the required steps that a system engineer / designer must consider in order to build and deploy a fully functional and reliable satellite communication link. The methodology entails a fully description of the basic laws of the space environment as well as an extensive analysis of the orbital mechanics and parameters. The idea was to demonstrate how the theory can be utilized in an actual satellite project simulation as well as how it is affected by it. The last step was to design and build an actual satellite communication system on a specialized software and present the results. The main conclusion of the above implementation is the fact that through the use of a low Earth orbit satellite constellation combined with a geostationary satellite used as a relay, it’s possible to achieve a resilient and reliable communication link with exceptional high data rates and an almost worldwide coverage

SPICA:revealing the hearts of galaxies and forming planetary systems : approach and US contributions

How did the diversity of galaxies we see in the modern Universe come to be? When and where did stars within them forge the heavy elements that give rise to the complex chemistry of life? How do planetary systems, the Universe's home for life, emerge from interstellar material? Answering these questions requires techniques that penetrate dust to reveal the detailed contents and processes in obscured regions. The ESA-JAXA Space Infrared Telescope for Cosmology and Astrophysics (SPICA) mission is designed for this, with a focus on sensitive spectroscopy in the 12 to 230 micron range. SPICA offers massive sensitivity improvements with its 2.5-meter primary mirror actively cooled to below 8 K. SPICA one of 3 candidates for the ESA's Cosmic Visions M5 mission, and JAXA has is committed to their portion of the collaboration. ESA will provide the silicon-carbide telescope, science instrument assembly, satellite integration and testing, and the spacecraft bus. JAXA will provide the passive and active cooling system (supporting the

The Apertif Surveys:The First Six Months

Apertif is a new phased-array feed for the Westerbork Synthesis Radio Telescope (WSRT), greatly increasing its field of view and turning it into a natural survey instrument. In July 2019, the Apertif legacy surveys commenced; these are a time-domain survey and a two-tiered imaging survey, with a shallow and medium-deep component. The time-domain survey searches for new (millisecond) pulsars and fast radio bursts (FRBs). The imaging surveys provide neutral hydrogen (HI), radio continuum and polarization data products. With a bandwidth of 300 MHz, Apertif can detect HI out to a redshift of 0.26. The key science goals to be accomplished by Apertif include localization of FRBs (including real-time public alerts), the role of environment and interaction on galaxy properties and gas removal, finding the smallest galaxies, connecting cold gas to AGN, understanding the faint radio population, and studying magnetic fields in galaxies. After a proprietary period, survey data products will be publicly available through the Apertif Long Term Archive (ALTA, https://alta.astron.nl). I will review the progress of the surveys and present the first results from the Apertif surveys, including highlighting the currently available public data

ATHENA Research Book, Volume 2

ATHENA European University is an association of nine higher education institutions with the mission of promoting excellence in research and innovation by enabling international cooperation. The acronym ATHENA stands for Association of Advanced Technologies in Higher Education. Partner institutions are from France, Germany, Greece, Italy, Lithuania, Portugal and Slovenia: University of Orléans, University of Siegen, Hellenic Mediterranean University, Niccolò Cusano University, Vilnius Gediminas Technical University, Polytechnic Institute of Porto and University of Maribor. In 2022, two institutions joined the alliance: the Maria Curie-Skłodowska University from Poland and the University of Vigo from Spain. Also in 2022, an institution from Austria joined the alliance as an associate member: Carinthia University of Applied Sciences. This research book presents a selection of the research activities of ATHENA University's partners. It contains an overview of the research activities of individual members, a selection of the most important bibliographic works of members, peer-reviewed student theses, a descriptive list of ATHENA lectures and reports from individual working sections of the ATHENA project. The ATHENA Research Book provides a platform that encourages collaborative and interdisciplinary research projects by advanced and early career researchers