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17 February 2022 | Story Lacea Loader | Photo Sonia Small (Kaleidoscope Studios)
Dr Engela van Staden
Dr Engela van Staden, Vice Rector: Academic

The University of the Free State (UFS) has finalised the first part of the Council on Higher Education (CHE) Institutional Audit (IA), submitting its Institutional Self-Evaluation Report (SER) and Portfolio of Evidence (PoE) to the higher education quality assurance body. 

According to Dr Engela van Staden, Vice-Rector: Academic, the second part of the institutional audit will involve the participation of relevant stakeholders in a site visit to the institution. During the visit, scheduled between 9 and 13 May 2022, an external panel of experts will systematically assess the submitted SER and requisite documents by asking inquisitive questions to interviewees who will be participating in this process.  

“The focus will be on the quality of programme offerings with a view to improving student success in all spheres of the student walk – from registration to graduation. To this end, the university’s Integrated Quality Management Framework (IQMF) will be assessed in order to provide evidence that quality assurance is ingrained in the core functions of the UFS, i.e., student success; quality of teaching and research; and engaged scholarship.”

Dr Van Staden says by re-introducing the SER, the university will embark on a stakeholder engagement plan, engaging with staff in faculties, service units, directorates, centres, departments, or schools, to keep them informed and prepared for a productive contribution to the Institutional Audit process. 

- The CHE is an independent statutory body established in terms of the provisions of the Higher Education Act No. 101 of 1997, as amended. It advises the Minister responsible for Higher Education and Training and is the national authority for quality assurance and promotion in higher education.

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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