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22 November 2024 | Story Leonie Bolleurs | Photo Stephen Collett
SARIMA - 2024
The Directorate Research Development at the university proudly participates in the SARIMA Visibility Project, aimed at enhancing its global visibility and research excellence.

The University of the Free State (UFS) has been selected to participate in a high-impact initiative managed and coordinated by the Southern African Research and Innovation Management Association (SARIMA). The SARIMA Visibility Project, which focuses on elevating institutional prominence, aims to enhance the university’s global visibility and strengthen its capacity to secure international grants. By participating in this initiative, the UFS is positioning the Directorate for Research and Development (DRD) to benchmark against other leading Tier 1 institutions, adopting best practices in research management and innovation to fuel future growth.

Key outcomes already underway

Since joining the initiative, the university has implemented several key interventions. Most notably, the development and execution of standardised operating procedures have been introduced. These procedures ensure alignment with global standards, creating consistency across various functions within DRD. Such efforts not only improve operational efficiency, but also boost the university’s competitiveness in attracting international research collaborations and securing funding opportunities. Other platforms to promote visibility that the DRD has adopted this year include its newsletter, Research Nexus, webinars, and a presence on social media.

The SARIMA Visibility Project at the UFS is spearheaded by the DRD under the leadership of Dr Glen Taylor. As pioneers of the initiative, the DRD team is working closely with SARIMA to ensure the successful implementation of key strategies aimed at improving the research infrastructure and elevating the university’s global standing. Their leadership has been instrumental in driving efforts to meet the project's ambitious objectives. These objectives include promoting best practices in research and innovation management across the region. They aim to support the research and innovation ecosystem to drive regional social and economic development. Additionally, the project seeks to engage key stakeholders to strengthen collaboration. Another objective is to building capacity among research and innovation management practitioners through training and development initiatives.

The SARIMA project is closely aligned with the UFS’s Vision 130, a strategic roadmap designed to propel the institution into its 130th anniversary in 2034. Vision 130 seeks to elevate the university’s academic and research standing on the global stage. By enhancing international partnerships and refining research management practices, SARIMA is playing an important role in supporting the university in its goal of becoming a globally recognised research institution, in line with Vision 130.

Value added to the research environment

In the few months since its launch, the SARIMA initiative has already added significant value to the UFS Research Office. The introduction of standardised procedures has not only improved consistency across departments, but has also made the office more agile and responsive to the demands of international collaborations. Benchmarking exercises conducted as part of the project have allowed the university to identify key areas for improvement, adopting innovative solutions that further enhance the institution’s research capacity and global visibility.

The SARIMA Visibility Project marks a significant step forward for the university. It is not only a means of raising the institution’s profile, but also a platform for long-term sustainable research excellence. As the UFS continues to benefit from this initiative, it is setting the stage for a future of global recognition and academic achievement that will benefit both the institution and the broader academic community for years to come.

News Archive

Two scientists part of team that discovers the source of the highest energy cosmic rays at the centre of the Milky Way
2016-03-22

Description: Giant molecular clouds  Tags: Giant molecular clouds

Artist's impression of the giant molecular clouds surrounding the Galactic Centre, bombarded by very high energy protons accelerated in the vicinity of the central black hole and subsequently shining in gamma rays.
Artist's impression: © Dr Mark A. Garlick/ H.E.S.S. Collaboration

Spotlight photo:
Dr Brian van Soelen and Prof Pieter Meintjes of the UFS Department of Physics.
Photo: Charl Devenish

H.E.S.S. (High Energy Stereoscopic System) scientists publically revealed their latest galactic discovery in the international science journal, Nature, on 16 March 2016. These scientists were able to pinpoint the most powerful source of cosmic radiation – which, up to now, remained a mystery.

Part of this team of scientists are Prof Pieter Meintjes and Dr Brian van Soelen, both in the University of the Free State (UFS) Department of Physics. Dr Van Soelen explains that they have discovered a proton PeVatron – a source that can accelerate protons up to energies of ~1 PeV (10^15 eV) – at the centre of the Milky Way. The supermassive black hole called Sagittarius A has been identified as the most plausible source of this unprecedented acceleration of protons.

The protons are accelerated to Very High Energy (VHE) gamma rays. The energy of these protons are 100 times larger than those achieved by the Large Hadron Collider at CERN (the European Organization for Nuclear Research).

According to Dr Van Soelen, the fact that this research has been published in Nature demonstrates the importance and pioneering nature of the research conducted by H.E.S.S. The H.E.S.S. observatory – operational in Namibia – is a collaboration between 42 scientific institutions in 12 countries.

In 2006, H.E.S.S. was awarded the Descartes Prize of the European Commission – the highest recognition for collaborative research – and in 2010 the prestigious Rossi Prize of the American Astronomical Society. The extent of the observatory’s significance places it among the ranks of the Hubble Space Telescope and the telescopes of the European Southern Observatory in Chile.

“The next generation VHE gamma-ray telescope,” Dr Van Soelen says, “will be the Cherenkov Telescope Array (CTA), which is currently in the design and development stage.” Both Dr Van Soelen and Prof Meintjes are part of this project as well.

H.E.S.S. has issued a complete statement about the paper published in Nature.

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