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17 June 2022 | Story Dr Nitha Ramnath | Photo Vivid Images
Heads of Mission to South Africa
Representatives of Heads of Diplomatic Mission in South Africa

The Rector and Vice-Chancellor of the University of the Free State (UFS), Prof Francis Petersen, hosted the Heads of Diplomatic Mission breakfast in South Africa on 9 June in Pretoria.

Fifteen foreign missions attended the event, with representation from Argentina, Belgium, Egypt, the European Union, Italy, Japan, Kenya, Lesotho, Namibia, the Netherlands, Nigeria, Spain, Switzerland, the United States, and Zimbabwe. The programme included a presentation by the Rector, followed by an engagement session.

Prof Francis Petersen’s overarching message during his presentation was that the UFS is ready to engage, co-create, and collaborate in the international arena, and that it produces graduates who are holistically developed to engage the world of work in their respective areas of specialisation. “We cannot underestimate the value of co-creation and collaboration between the Global North and Global South institutions of higher learning as equal partners. The UFS has an array of expertise that we deem as core drivers of partnerships, which has the potential to offer immense value through collaboration,” said Prof Petersen.

The event offered the UFS the opportunity to reach out and engage the international community on potential partnerships and collaborations. The Rector provided insight into the UFS, while positioning the university as well as current and potential collaborations with institutions of higher learning and other sectors in the respective heads of mission countries.

The Heads of Diplomatic Mission Breakfast was a collaboration between the Department of Communication and Marketing, the Office for International Affairs, and Institutional Advancement.


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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